This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q1b1x1_061447_TTUQ1b1x1_2992708_aEdEQksW
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.99 05:05:58.56 +47:42:36.0
160.11981 4.09229 galactic Aur Second-epoch detections are separated by 0.9" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J076.4937+47.7100 | 05:05:58.56 +47:42:36.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.824+/-0.033 (M)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:05:58.56 +47:42:36.0: 13.91 +/- 0.05 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:05:58.56 +47:42:36.0: 13.91 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.91 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J076.4937+47.7100,2461293.9679,12.99,0.05,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 J076.4937+47.7100 20260910.4679 12.99CV 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 09 10.4679 2461293.9679 13.53 05:01:05.42 +47:12:02.0
160.02321 3.12674 galactic Aur Second-epoch detections are separated by 1.9" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:01:05.42 +47:12:02.0 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=1.196+/-0.029 (M)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:01:05.42 +47:12:02.0: 14.88 +/- 0.11 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:01:05.42 +47:12:02.0: 14.63 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.73 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,13.53,0.05,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 20260910.4679 13.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.03 05:01:33.81 +47:06:14.0
160.14908 3.13111 galactic Aur Second-epoch detections are separated by 1.6" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J075.3925+47.1070 | 05:01:33.81 +47:06:14.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F6 (LAMOST DR5) J-Ks=0.515+/-0.030 (K)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:01:33.81 +47:06:14.0: 14.00 +/- 0.05 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:01:33.81 +47:06:14.0: 13.91 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.95 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J075.3925+47.1070,2461293.9679,13.03,0.05,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 J075.3925+47.1070 20260910.4679 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.18 05:03:17.00 +47:23:38.5
160.09704 3.53935 galactic Aur Second-epoch detections are separated by 0.7" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:03:17.00 +47:23:38.5 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.688+/-0.033 (K)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:03:17.00 +47:23:38.5: 14.03 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:03:17.00 +47:23:38.5: 14.09 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.06 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,13.18,0.05,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
target 20260910.4679 13.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.22 04:56:14.92 +46:48:03.1
159.82575 2.23105 galactic Aur Second-epoch detections are separated by 0.5" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.0647+46.7992 | 04:56:14.92 +46:48:03.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.367+/-0.037 (G)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:56:14.92 +46:48:03.1: 14.08 +/- 0.05 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:56:14.92 +46:48:03.1: 14.30 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.17 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J074.0647+46.7992,2461293.9679,13.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J074.0647+46.7992 20260910.4679 13.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.19 04:57:09.58 +46:41:30.8
160.00843 2.28499 galactic Aur Second-epoch detections are separated by 1.3" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.2871+46.7037 | 04:57:09.58 +46:41:30.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.594+/-0.032 (K)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:57:09.58 +46:41:30.8: 14.11 +/- 0.05 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:57:09.58 +46:41:30.8: 14.17 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.14 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J074.2871+46.7037,2461293.9679,13.19,0.05,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 J074.2871+46.7037 20260910.4679 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.12 05:02:43.61 +46:28:45.5
160.76610 2.90728 galactic Aur Second-epoch detections are separated by 1.3" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J075.6732+46.4866 | 05:02:43.61 +46:28:45.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.877+/-0.032 (M)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:02:43.61 +46:28:45.5: 14.14 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:02:43.61 +46:28:45.5: 13.99 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.06 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J075.6732+46.4866,2461293.9679,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J075.6732+46.4866 20260910.4679 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.29 05:00:07.07 +45:23:30.6
161.34777 1.88229 galactic Aur Second-epoch detections are separated by 1.5" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J075.0205+45.3820 | 05:00:07.07 +45:23:30.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.588+/-0.030 (K)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:00:07.07 +45:23:30.6: 14.20 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:00:07.07 +45:23:30.6: 14.13 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.17 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J075.0205+45.3820,2461293.9679,13.29,0.05,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 J075.0205+45.3820 20260910.4679 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.22 05:09:39.80 +47:44:34.2
160.46410 4.60971 galactic Aur Second-epoch detections are separated by 2.2" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J077.4160+47.7394 | 05:09:39.80 +47:44:34.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A9V (LAMOST DR5) J-Ks=0.307+/-0.040 (F)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:09:39.80 +47:44:34.2: 14.23 +/- 0.07 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:09:39.80 +47:44:34.2: 14.24 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.23 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J077.4160+47.7394,2461293.9679,13.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J077.4160+47.7394 20260910.4679 13.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.22 04:55:55.61 +46:52:26.0
159.73428 2.23378 galactic Aur Second-epoch detections are separated by 1.8" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:55:55.61 +46:52:26.0 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.932+/-0.034 (M)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:55:55.61 +46:52:26.0: 14.28 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:55:55.61 +46:52:26.0: 14.16 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.22 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,13.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260910.4679 13.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 11.91 05:00:43.60 +47:15:00.4
159.94608 3.10839 galactic Aur Second-epoch detections are separated by 0.3" and 5.8 pix
The object was found in VSX 1" ASASSN-V J050043.60+471459.8
Type: SRS
# Max. Min./Amp. JD0 Period
13.110 V 13.220 V 2458169.83000 27.148000000000
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:00:43.60 +47:15:00.4: 12.84 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:00:43.60 +47:15:00.4: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J050043.60+471459.8,2461293.9679,11.91,0.05,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
ASASSN-V J050043.60+471459.8 20260910.4679 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.29 05:01:48.06 +47:11:21.2
160.10622 3.21525 galactic Aur Second-epoch detections are separated by 1.0" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:01:48.06 +47:11:21.2 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.437+/-0.033 (G)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:01:48.06 +47:11:21.2: 14.35 +/- 0.07 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:01:48.06 +47:11:21.2: 14.30 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.33 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,13.29,0.05,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 20260910.4679 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.28 05:02:46.66 +47:04:27.5
160.29893 3.27672 galactic Aur Second-epoch detections are separated by 0.5" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 207018248304575744 | 05:02:46.65 +47:04:27.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K4 (LAMOST DR5) J-Ks=1.196+/-0.031 (M)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:02:46.66 +47:04:27.5: 13.28 +/- 0.03 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:02:46.66 +47:04:27.5: 13.25 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 207018248304575744,2461293.9679,12.28,0.05,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 207018248304575744 20260910.4679 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.60 05:06:35.10 +47:44:23.7
160.15742 4.19217 galactic Aur Second-epoch detections are separated by 1.0" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J076.6527+47.7374 | 05:06:35.10 +47:44:23.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.452+/-0.033 (G)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:06:35.10 +47:44:23.7: 13.42 +/- 0.03 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:06:35.10 +47:44:23.7: 13.50 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J076.6527+47.7374,2461293.9679,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J076.6527+47.7374 20260910.4679 12.60CV 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 09 10.4679 2461293.9679 12.85 05:05:25.05 +47:39:55.1
160.09894 3.99031 galactic Aur Second-epoch detections are separated by 1.1" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J076.3572+47.6643 | 05:05:25.05 +47:39:55.1 (user input) | IRR (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.772+/-0.030 (K)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:05:25.05 +47:39:55.1: 13.70 +/- 0.04 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:05:25.05 +47:39:55.1: 13.73 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.72 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J076.3572+47.6643,2461293.9679,12.85,0.05,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
ATO J076.3572+47.6643 20260910.4679 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.43 05:03:31.56 +46:58:40.6
160.45324 3.31935 galactic Aur Second-epoch detections are separated by 0.4" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:03:31.56 +46:58:40.6 (user input) | T | P | (position from user input) SpType: K7 (LAMOST DR5) J-Ks=1.270+/-0.030 (Very red! L if it's a dwarf)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:03:31.56 +46:58:40.6: 14.70 +/- 0.09 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:03:31.56 +46:58:40.6: 14.63 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.67 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,13.43,0.05,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 20260910.4679 13.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.89 05:03:31.64 +46:54:30.6
160.50864 3.27735 galactic Aur Second-epoch detections are separated by 0.3" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:03:31.64 +46:54:30.6 (user input) | T | P | (position from user input) J-Ks=0.438+/-0.032 (G)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:03:31.64 +46:54:30.6: 13.87 +/- 0.05 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:03:31.64 +46:54:30.6: 13.97 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.91 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,12.89,0.05,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
target 20260910.4679 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.86 04:56:59.62 +47:12:09.9
159.59082 2.58112 galactic Aur Second-epoch detections are separated by 0.4" and 5.7 pix
The object was found in VSX 1" ZTF J045659.69+471209.7
Type: SR
# Max. Min./Amp. JD0 Period
15.195 g Y 0.115 g 2458358.01650 21.705945100000
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:56:59.62 +47:12:09.9: 13.86 +/- 0.05 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:56:59.62 +47:12:09.9: 13.85 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.86 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J045659.69+471209.7,2461293.9679,12.86,0.05,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
ZTF J045659.69+471209.7 20260910.4679 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.95 05:03:20.09 +47:27:40.2
160.04891 3.58706 galactic Aur Second-epoch detections are separated by 2.1" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:03:20.09 +47:27:40.2 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.902+/-0.032 (M)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:03:20.09 +47:27:40.2: 13.85 +/- 0.05 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:03:20.09 +47:27:40.2: 13.93 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.89 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,12.95,0.05,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 20260910.4679 12.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.96 04:56:25.51 +49:06:48.8
158.03518 3.69803 galactic Aur Second-epoch detections are separated by 2.1" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:25.51 +49:06:48.8 (user input) | T | P | (position from user input) J-Ks=0.819+/-0.028 (M)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:56:25.51 +49:06:48.8: 13.85 +/- 0.05 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:56:25.51 +49:06:48.8: 13.92 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.88 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,12.96,0.05,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 20260910.4679 12.96CV 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 09 10.4679 2461293.9679 12.86 05:03:35.81 +47:14:27.9
160.25111 3.48868 galactic Aur Second-epoch detections are separated by 1.1" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:03:35.81 +47:14:27.9 (user input) | T | P | (position from user input) J-Ks=0.989+/-0.032 (M)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:03:35.81 +47:14:27.9: 13.84 +/- 0.05 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:03:35.81 +47:14:27.9: 13.85 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260910.4679 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.83 05:07:20.73 +47:39:06.0
160.30510 4.24191 galactic Aur Second-epoch detections are separated by 0.7" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J076.8328+47.6520 | 05:07:20.73 +47:39:06.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:07:20.73 +47:39:06.0: 13.82 +/- 0.05 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:07:20.73 +47:39:06.0: 13.84 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J076.8328+47.6520,2461293.9679,12.83,0.05,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
ATO J076.8328+47.6520 20260910.4679 12.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.87 04:56:58.66 +47:08:26.5
159.63771 2.54033 galactic Aur Second-epoch detections are separated by 0.9" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:58.66 +47:08:26.5 (user input) | T | P | (position from user input) J-Ks=1.110+/-0.032 (M)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:56:58.66 +47:08:26.5: 13.91 +/- 0.05 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:56:58.66 +47:08:26.5: 13.88 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.89 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,12.87,0.05,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 20260910.4679 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.89 05:00:35.52 +47:20:09.5
159.86418 3.14310 galactic Aur Second-epoch detections are separated by 0.6" and 5.9 pix
The object was found in VSX24" Gaia DR3 255074087621406464
Type: S
# Max. Min./Amp. JD0 Period
16.790 G 17.400 G A
ATTENTION: measured mag 12.89 is 3.9 mag brighter than the VSX record maximum brightness 16.79 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:00:35.52 +47:20:09.5: 13.81 +/- 0.05 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:00:35.52 +47:20:09.5: 13.81 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.81 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 255074087621406464,2461293.9679,12.89,0.05,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 255074087621406464 20260910.4679 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.91 05:02:36.25 +46:36:48.7
160.64669 2.97239 galactic Aur Second-epoch detections are separated by 1.3" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J075.6346+46.6117 | 05:02:36.25 +46:36:48.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.375+/-0.040 (G)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:02:36.25 +46:36:48.7: 13.81 +/- 0.05 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:02:36.25 +46:36:48.7: 13.84 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.82 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J075.6346+46.6117,2461293.9679,12.91,0.05,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 J075.6346+46.6117 20260910.4679 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.91 05:03:05.15 +47:31:04.4
159.97816 3.58812 galactic Aur Second-epoch detections are separated by 1.6" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:03:05.15 +47:31:04.4 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.888+/-0.032 (M)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:03:05.15 +47:31:04.4: 13.78 +/- 0.04 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:03:05.15 +47:31:04.4: 13.81 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.80 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,12.91,0.05,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 20260910.4679 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.97 05:04:47.65 +47:03:41.5
160.51777 3.54195 galactic Aur Second-epoch detections are separated by 0.4" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:04:47.65 +47:03:41.5 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.512+/-0.033 (K)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:04:47.65 +47:03:41.5: 13.81 +/- 0.05 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:04:47.65 +47:03:41.5: 13.90 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,12.97,0.05,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 20260910.4679 12.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.89 05:02:02.16 +47:13:54.5
160.09688 3.27286 galactic Aur Second-epoch detections are separated by 1.0" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:02:02.16 +47:13:54.5 (user input) | T | P | (position from user input) J-Ks=0.393+/-0.030 (G)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:02:02.16 +47:13:54.5: 13.80 +/- 0.04 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:02:02.16 +47:13:54.5: 13.77 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.78 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,12.89,0.05,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
target 20260910.4679 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.85 05:02:04.15 +47:22:05.2
159.99221 3.36056 galactic Aur Second-epoch detections are separated by 1.2" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:02:04.15 +47:22:05.2 (user input) | T | P | (position from user input) SpType: G1 (LAMOST DR5) J-Ks=0.862+/-0.031 (M)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:02:04.15 +47:22:05.2: 13.77 +/- 0.04 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:02:04.15 +47:22:05.2: 13.75 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.76 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,12.85,0.05,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 20260910.4679 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.71 05:01:46.05 +47:08:54.0
160.13513 3.18574 galactic Aur Second-epoch detections are separated by 0.8" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J075.4416+47.1482 | 05:01:46.00 +47:08:53.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: M1 (LAMOST DR5) J-Ks=1.497+/-0.029 (Very red! L if it's a dwarf)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:01:46.05 +47:08:54.0: 13.77 +/- 0.04 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:01:46.05 +47:08:54.0: 13.76 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.76 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J075.4416+47.1482,2461293.9679,12.71,0.05,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 J075.4416+47.1482 20260910.4679 12.71CV 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 09 10.4679 2461293.9679 12.86 05:03:32.20 +47:28:10.9
160.06287 3.61934 galactic Aur Second-epoch detections are separated by 1.8" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J075.8857+47.4721 | 05:03:32.20 +47:28:10.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.451+/-0.034 (G)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:03:32.20 +47:28:10.9: 13.76 +/- 0.04 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:03:32.20 +47:28:10.9: 13.71 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.74 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J075.8857+47.4721,2461293.9679,12.86,0.05,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
ATO J075.8857+47.4721 20260910.4679 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.78 05:09:53.78 +47:49:48.1
160.41676 4.69283 galactic Aur Second-epoch detections are separated by 1.8" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J077.4743+47.8298 | 05:09:53.78 +47:49:48.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A2V (LAMOST DR5) J-Ks=0.346+/-0.032 (G)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:09:53.78 +47:49:48.1: 13.77 +/- 0.04 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:09:53.78 +47:49:48.1: 13.77 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.77 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J077.4743+47.8298,2461293.9679,12.78,0.05,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 J077.4743+47.8298 20260910.4679 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.37 04:56:13.66 +47:10:14.6
159.53457 2.45945 galactic Aur Second-epoch detections are separated by 8.5" 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 | target | 04:56:13.66 +47:10:14.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:56:13.66 +47:10:14.6: 14.52 +/- 0.08 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:56:13.66 +47:10:14.6: 14.34 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.41 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,13.37,0.05,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 20260910.4679 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.76 05:03:42.60 +47:22:22.7
160.15773 3.58396 galactic Aur Second-epoch detections are separated by 0.9" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:03:42.60 +47:22:22.7 (user input) | T | P | (position from user input) J-Ks=0.843+/-0.030 (M)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:03:42.60 +47:22:22.7: 13.73 +/- 0.05 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:03:42.60 +47:22:22.7: 13.71 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.72 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,12.76,0.05,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
target 20260910.4679 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.85 05:04:07.93 +46:47:30.9
160.66431 3.28884 galactic Aur Second-epoch detections are separated by 0.8" and 5.8 pix
The object was found in VSX23" Gaia DR3 207030828265833728
Type:
# Max. Min./Amp. JD0 Period
16.620 G 17.350 G
ATTENTION: measured mag 12.85 is 3.8 mag brighter than the VSX record maximum brightness 16.62 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:04:07.93 +46:47:30.9: 13.72 +/- 0.04 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:04:07.93 +46:47:30.9: 13.70 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.71 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 207030828265833728,2461293.9679,12.85,0.05,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 207030828265833728 20260910.4679 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.78 05:02:21.07 +47:07:09.9
160.21879 3.24668 galactic Aur Second-epoch detections are separated by 0.7" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:02:21.07 +47:07:09.9 (user input) | T | P | (position from user input) J-Ks=0.432+/-0.030 (G)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:02:21.07 +47:07:09.9: 13.71 +/- 0.04 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:02:21.07 +47:07:09.9: 13.67 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.69 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,12.78,0.05,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 20260910.4679 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.84 05:10:08.50 +49:42:12.7
158.92109 5.83014 galactic Aur Second-epoch detections are separated by 0.4" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:10:08.50 +49:42:12.7 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.972+/-0.030 (M)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:10:08.50 +49:42:12.7: 13.70 +/- 0.04 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:10:08.50 +49:42:12.7: 13.79 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.74 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,12.84,0.05,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 20260910.4679 12.84CV 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 09 10.4679 2461293.9679 12.78 05:08:16.90 +47:45:08.9
160.31810 4.42846 galactic Aur Second-epoch detections are separated by 0.9" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J077.0620+47.7503 | 05:08:16.90 +47:45:08.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.456+/-0.035 (G)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:08:16.90 +47:45:08.9: 13.67 +/- 0.04 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:08:16.90 +47:45:08.9: 13.70 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.68 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J077.0620+47.7503,2461293.9679,12.78,0.05,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 J077.0620+47.7503 20260910.4679 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.70 05:02:33.36 +47:07:05.8
160.24098 3.27360 galactic Aur Second-epoch detections are separated by 1.2" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J075.6272+47.1147 | 05:02:33.36 +47:07:05.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.773+/-0.031 (K)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:02:33.36 +47:07:05.8: 13.66 +/- 0.04 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:02:33.36 +47:07:05.8: 13.62 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.64 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J075.6272+47.1147,2461293.9679,12.70,0.05,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 J075.6272+47.1147 20260910.4679 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.77 05:02:28.83 +47:27:00.5
159.96963 3.46574 galactic Aur Second-epoch detections are separated by 0.6" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:02:28.83 +47:27:00.5 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.846+/-0.031 (M)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:02:28.83 +47:27:00.5: 13.65 +/- 0.05 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:02:28.83 +47:27:00.5: 13.63 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.64 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,12.77,0.05,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
target 20260910.4679 12.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.70 04:55:34.54 +44:52:33.6
161.25355 0.93419 galactic Aur Second-epoch detections are separated by 0.2" and 5.8 pix
The object was found in VSX 2" NSV 16189
Type: VAR:
# Max. Min./Amp. JD0 Period
14.000 V
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:55:34.54 +44:52:33.6: 13.65 +/- 0.03 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:55:34.54 +44:52:33.6: 13.64 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSV 16189,2461293.9679,12.70,0.05,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
NSV 16189 20260910.4679 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.69 05:07:30.93 +47:42:45.0
160.27330 4.30119 galactic Aur Second-epoch detections are separated by 1.7" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J076.8717+47.7203 | 05:07:30.93 +47:42:45.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.371+/-0.034 (G)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:07:30.93 +47:42:45.0: 13.64 +/- 0.04 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:07:30.93 +47:42:45.0: 13.61 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.62 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J076.8717+47.7203,2461293.9679,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J076.8717+47.7203 20260910.4679 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.72 05:07:50.36 +47:40:37.3
160.33445 4.32376 galactic Aur Second-epoch detections are separated by 1.8" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:07:50.36 +47:40:37.3 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.358+/-0.030 (G)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:07:50.36 +47:40:37.3: 13.64 +/- 0.04 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:07:50.36 +47:40:37.3: 13.64 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.64 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,12.72,0.05,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 20260910.4679 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.70 05:08:14.44 +47:52:20.8
160.21727 4.49431 galactic Aur Second-epoch detections are separated by 1.0" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:08:14.44 +47:52:20.8 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.985+/-0.032 (M)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:08:14.44 +47:52:20.8: 13.66 +/- 0.04 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:08:14.44 +47:52:20.8: 13.62 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.64 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,12.70,0.05,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
target 20260910.4679 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.71 05:02:05.00 +47:01:49.7
160.26147 3.15626 galactic Aur Second-epoch detections are separated by 0.6" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:02:05.00 +47:01:49.7 (user input) | T | P | (position from user input) SpType: F4 (LAMOST DR5) J-Ks=0.323+/-0.031 (G)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:02:05.00 +47:01:49.7: 13.62 +/- 0.03 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:02:05.00 +47:01:49.7: 13.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.67 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,12.71,0.05,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 20260910.4679 12.71CV 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 09 10.4679 2461293.9679 12.65 05:03:25.57 +46:47:07.9
160.59595 3.18891 galactic Aur Second-epoch detections are separated by 1.1" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J075.8604+46.7841 | 05:03:25.57 +46:47:07.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.889+/-0.030 (M)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:03:25.57 +46:47:07.9: 13.58 +/- 0.03 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:03:25.57 +46:47:07.9: 13.61 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J075.8604+46.7841,2461293.9679,12.65,0.05,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 J075.8604+46.7841 20260910.4679 12.65CV 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 09 10.4679 2461293.9679 12.63 04:55:49.95 +46:58:38.6
159.64341 2.28601 galactic Aur Second-epoch detections are separated by 0.2" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:55:49.95 +46:58:38.6 (user input) | T | P | (position from user input) SpType: A7V (LAMOST DR5) J-Ks=0.319+/-0.042 (F)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:55:49.95 +46:58:38.6: 13.56 +/- 0.03 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:55:49.95 +46:58:38.6: 13.54 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.55 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,12.63,0.05,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 20260910.4679 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.46 05:01:38.46 +46:54:09.0
160.31668 3.01831 galactic Aur Second-epoch detections are separated by 2.5" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J075.4094+46.9025 | 05:01:38.46 +46:54:09.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.318+/-0.057 (F)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:01:38.46 +46:54:09.0: 14.56 +/- 0.09 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:01:38.46 +46:54:09.0: 14.55 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.55 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J075.4094+46.9025,2461293.9679,13.46,0.05,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
ATO J075.4094+46.9025 20260910.4679 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.49 05:02:23.86 +46:50:36.2
160.44267 3.08455 galactic Aur Second-epoch detections are separated by 0.8" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:02:23.86 +46:50:36.2 (user input) | T | P | (position from user input) J-Ks=0.506+/-0.032 (K)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:02:23.86 +46:50:36.2: 14.59 +/- 0.09 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:02:23.86 +46:50:36.2: 14.53 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.56 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,13.49,0.05,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 20260910.4679 13.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.68 05:09:56.19 +47:44:08.0
160.49723 4.64245 galactic Aur Second-epoch detections are separated by 0.3" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:09:56.19 +47:44:08.0 (user input) | T | P | (position from user input) J-Ks=0.180+/-0.035 (F)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:09:56.19 +47:44:08.0: 13.55 +/- 0.04 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:09:56.19 +47:44:08.0: 13.57 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,12.68,0.05,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
target 20260910.4679 12.68CV 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 09 10.4679 2461293.9679 13.43 04:55:43.24 +46:57:55.0
159.64090 2.26356 galactic Aur Second-epoch detections are separated by 0.9" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J073.9295+46.9633 | 04:55:43.24 +46:57:55.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.935+/-0.033 (M)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:55:43.24 +46:57:55.0: 14.58 +/- 0.09 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:55:43.24 +46:57:55.0: 14.61 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.59 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J073.9295+46.9633,2461293.9679,13.43,0.05,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 J073.9295+46.9633 20260910.4679 13.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.35 05:07:21.72 +47:44:26.5
160.23516 4.29731 galactic Aur Second-epoch detections are separated by 1.0" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J076.8340+47.7514 | 05:07:21.72 +47:44:26.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.343+/-0.036 (G)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:07:21.72 +47:44:26.5: 14.52 +/- 0.09 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:07:21.72 +47:44:26.5: 14.36 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.43 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J076.8340+47.7514,2461293.9679,13.35,0.05,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 J076.8340+47.7514 20260910.4679 13.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.53 05:07:32.06 +47:38:09.1
160.33685 4.25798 galactic Aur Second-epoch detections are separated by 0.3" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J076.8856+47.6381 | 05:07:32.06 +47:38:09.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.722+/-0.033 (K)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:07:32.06 +47:38:09.1: 13.45 +/- 0.03 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:07:32.06 +47:38:09.1: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.42 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J076.8856+47.6381,2461293.9679,12.53,0.05,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 J076.8856+47.6381 20260910.4679 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.52 05:02:40.21 +47:16:23.0
160.12989 3.38330 galactic Aur Second-epoch detections are separated by 0.3" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J075.6616+47.2643 | 05:02:40.21 +47:16:23.0 (user input) | NSINE (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.860+/-0.031 (M)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:02:40.21 +47:16:23.0: 13.45 +/- 0.03 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:02:40.21 +47:16:23.0: 13.44 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.44 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J075.6616+47.2643,2461293.9679,12.52,0.05,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 J075.6616+47.2643 20260910.4679 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.55 05:03:32.51 +47:07:52.2
160.33293 3.41453 galactic Aur Second-epoch detections are separated by 0.1" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J075.8911+47.1293 | 05:03:32.51 +47:07:52.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.380+/-0.033 (G)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:03:32.51 +47:07:52.2: 13.43 +/- 0.03 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:03:32.51 +47:07:52.2: 13.50 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J075.8911+47.1293,2461293.9679,12.55,0.05,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 J075.8911+47.1293 20260910.4679 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.57 05:07:53.70 +47:34:01.1
160.42867 4.26569 galactic Aur Second-epoch detections are separated by 0.2" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J076.9697+47.5545 | 05:07:53.70 +47:34:01.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.289+/-0.029 (F)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:07:53.70 +47:34:01.1: 13.44 +/- 0.04 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:07:53.70 +47:34:01.1: 13.50 +/- 0.04 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J076.9697+47.5545,2461293.9679,12.57,0.05,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
ATO J076.9697+47.5545 20260910.4679 12.57CV 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 09 10.4679 2461293.9679 12.51 04:57:24.94 +44:47:52.3
161.51850 1.13994 galactic Aur Second-epoch detections are separated by 1.1" and 5.8 pix
The object was found in VSX 1" ASASSN-V J045724.94+444751.6
Type: SR
# Max. Min./Amp. JD0 Period
13.760 V 13.910 V 2457021.71400 30.100000000000
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:57:24.94 +44:47:52.3: 13.39 +/- 0.03 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:57:24.94 +44:47:52.3: 13.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.42 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J045724.94+444751.6,2461293.9679,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J045724.94+444751.6 20260910.4679 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.49 05:02:51.87 +46:56:09.2
160.41792 3.20417 galactic Aur Second-epoch detections are separated by 1.1" and 5.6 pix
The object was found in VSX 9" Gaia DR3 207000351176300416
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
15.490 G 15.570 G F
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:02:51.87 +46:56:09.2: 13.38 +/- 0.03 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:02:51.87 +46:56:09.2: 13.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.38 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 207000351176300416,2461293.9679,12.49,0.05,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 207000351176300416 20260910.4679 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.47 05:08:26.15 +47:41:25.7
160.38356 4.41243 galactic Aur Second-epoch detections are separated by 1.6" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J077.1066+47.6938 | 05:08:26.15 +47:41:25.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A5V (LAMOST DR5) J-Ks=0.197+/-0.035 (F)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:08:26.15 +47:41:25.7: 13.33 +/- 0.03 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:08:26.15 +47:41:25.7: 13.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.33 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J077.1066+47.6938,2461293.9679,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J077.1066+47.6938 20260910.4679 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.43 05:00:01.28 +44:59:43.1
161.64963 1.62443 galactic Aur Second-epoch detections are separated by 1.0" and 5.9 pix
The object was found in VSX 0" ASASSN-V J050001.27+445942.8
Type: SR
# Max. Min./Amp. JD0 Period
14.840 g Y 0.220 g 2459067.94900 52.560000000000
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:00:01.28 +44:59:43.1: 13.36 +/- 0.03 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:00:01.28 +44:59:43.1: 13.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J050001.27+445942.8,2461293.9679,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J050001.27+445942.8 20260910.4679 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.46 04:55:49.53 +47:07:21.4
159.52933 2.37600 galactic Aur Second-epoch detections are separated by 3.2" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J073.9610+47.1221 | 04:55:49.53 +47:07:21.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:55:49.53 +47:07:21.4: 14.48 +/- 0.08 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:55:49.53 +47:07:21.4: 14.55 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.52 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J073.9610+47.1221,2461293.9679,13.46,0.05,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
ATO J073.9610+47.1221 20260910.4679 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.33 05:07:36.13 +47:32:31.7
160.41910 4.21122 galactic Aur Second-epoch detections are separated by 3.3" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J076.9060+47.5415 | 05:07:36.13 +47:32:31.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.965+/-0.032 (M)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:07:36.13 +47:32:31.7: 14.50 +/- 0.09 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:07:36.13 +47:32:31.7: 14.52 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.51 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J076.9060+47.5415,2461293.9679,13.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J076.9060+47.5415 20260910.4679 13.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.44 05:03:00.75 +47:02:30.2
160.34921 3.28861 galactic Aur Second-epoch detections are separated by 0.4" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J075.7565+47.0435 | 05:03:00.75 +47:02:30.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.340+/-0.032 (G)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:03:00.75 +47:02:30.2: 13.34 +/- 0.03 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:03:00.75 +47:02:30.2: 13.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J075.7565+47.0435,2461293.9679,12.44,0.05,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
ATO J075.7565+47.0435 20260910.4679 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.37 05:05:59.18 +45:00:01.5
162.28880 2.46347 galactic Aur Second-epoch detections are separated by 0.9" and 5.9 pix
The object was found in VSX 0" ZTF J050559.14+450001.6
Type: SR
# Max. Min./Amp. JD0 Period
13.601 r Y 0.293 r 2458464.10440 67.985030300000
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:05:59.18 +45:00:01.5: 14.50 +/- 0.09 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:05:59.18 +45:00:01.5: 14.48 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.49 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J050559.14+450001.6,2461293.9679,13.37,0.05,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
ZTF J050559.14+450001.6 20260910.4679 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.20 05:02:18.07 +47:05:10.0
160.24002 3.21962 galactic Aur Second-epoch detections are separated by 0.6" and 5.7 pix
The object was found in VSX 0" Gaia DR3 207017595469546496
Type: ROT
# Max. Min./Amp. JD0 Period
13.760 G 13.800 G K
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:02:18.07 +47:05:10.0: 14.44 +/- 0.07 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:02:18.07 +47:05:10.0: 14.22 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.31 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 207017595469546496,2461293.9679,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 207017595469546496 20260910.4679 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.35 05:03:01.45 +46:36:01.4
160.70113 3.02158 galactic Aur Second-epoch detections are separated by 1.2" and 5.7 pix
The object was found in VSX 1" Gaia DR3 206934204383116032
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.070 G 14.090 G A
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:03:01.45 +46:36:01.4: 14.49 +/- 0.09 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:03:01.45 +46:36:01.4: 14.42 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.45 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 206934204383116032,2461293.9679,13.35,0.05,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 206934204383116032 20260910.4679 13.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.26 05:07:16.82 +47:31:31.3
160.40006 4.15763 galactic Aur Second-epoch detections are separated by 1.7" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:07:16.82 +47:31:31.3 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:07:16.82 +47:31:31.3: 14.38 +/- 0.07 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:07:16.82 +47:31:31.3: 14.47 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.42 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,13.26,0.05,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 20260910.4679 13.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.31 04:55:35.82 +47:03:44.3
159.55200 2.30791 galactic Aur Second-epoch detections are separated by 0.6" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:55:35.82 +47:03:44.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:55:35.82 +47:03:44.3: 14.47 +/- 0.08 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:55:35.82 +47:03:44.3: 14.26 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.34 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,13.31,0.05,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
target 20260910.4679 13.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.18 05:08:10.13 +47:34:16.9
160.45272 4.30540 galactic Aur Second-epoch detections are separated by 0.4" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J077.0418+47.5671 | 05:08:10.13 +47:34:16.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A1IV (LAMOST DR5)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:08:10.13 +47:34:16.9: 13.05 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:08:10.13 +47:34:16.9: 13.02 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J077.0418+47.5671,2461293.9679,12.18,0.05,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 J077.0418+47.5671 20260910.4679 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.44 04:55:51.50 +47:13:07.2
159.45785 2.44048 galactic Aur Second-epoch detections are separated by 0.6" and 5.8 pix
The object was found in VSX 0" Gaia DR3 254920121634710016
Type: E
# Max. Min./Amp. JD0 Period
13.690 G 14.130 G 37.420000000000 K
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:55:51.50 +47:13:07.2: 14.41 +/- 0.07 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:55:51.50 +47:13:07.2: 14.52 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.45 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 254920121634710016,2461293.9679,13.44,0.05,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 254920121634710016 20260910.4679 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.32 05:07:51.14 +47:35:52.3
160.39949 4.27832 galactic Aur Second-epoch detections are separated by 0.6" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 207139405034380672 | 05:07:51.14 +47:35:52.3 (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) SpType: K5 (LAMOST DR5) J-Ks=0.631+/-0.034 (K)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:07:51.14 +47:35:52.3: 13.15 +/- 0.03 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:07:51.14 +47:35:52.3: 13.24 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.19 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 207139405034380672,2461293.9679,12.32,0.05,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
Large-amplitude variable Gaia DR2 207139405034380672 20260910.4679 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.41 04:55:40.99 +46:55:25.8
159.66922 2.23261 galactic Aur Second-epoch detections are separated by 1.9" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:55:40.99 +46:55:25.8 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.559+/-0.033 (K)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:55:40.99 +46:55:25.8: 14.42 +/- 0.07 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:55:40.99 +46:55:25.8: 14.47 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.44 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,13.41,0.05,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 20260910.4679 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.29 05:02:44.56 +47:05:11.2
160.28565 3.27939 galactic Aur Second-epoch detections are separated by 0.2" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:02:44.56 +47:05:11.2 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.369+/-0.032 (G)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:02:44.56 +47:05:11.2: 13.13 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:02:44.56 +47:05:11.2: 13.22 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.17 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,12.29,0.05,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 20260910.4679 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.20 05:09:33.17 +47:48:17.4
160.40294 4.63143 galactic Aur Second-epoch detections are separated by 0.3" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J077.3871+47.8025 | 05:09:33.16 +47:48:17.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: K7 (LAMOST DR5) J-Ks=1.127+/-0.032 (M)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:09:33.17 +47:48:17.4: 13.05 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:09:33.17 +47:48:17.4: 13.07 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J077.3871+47.8025,2461293.9679,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J077.3871+47.8025 20260910.4679 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.41 04:55:57.81 +47:09:53.3
159.51109 2.42071 galactic Aur Second-epoch detections are separated by 1.2" and 5.6 pix
The object was found in VSX 1" ZTF J045557.75+470953.6
Type: RS
# Max. Min./Amp. JD0 Period
14.553 g Y 0.076 g 2458380.97580 1.982845200000
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:55:57.81 +47:09:53.3: 14.38 +/- 0.07 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:55:57.81 +47:09:53.3: 14.55 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.45 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J045557.75+470953.6,2461293.9679,13.41,0.05,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
ZTF J045557.75+470953.6 20260910.4679 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.20 05:07:24.35 +47:21:45.7
160.54354 4.07744 galactic Aur Second-epoch detections are separated by 0.7" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J076.8514+47.3625 | 05:07:24.35 +47:21:45.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.420+/-0.033 (G)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:07:24.35 +47:21:45.7: 14.37 +/- 0.08 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:07:24.35 +47:21:45.7: 14.43 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.40 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J076.8514+47.3625,2461293.9679,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J076.8514+47.3625 20260910.4679 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.31 05:03:22.77 +47:20:53.9
160.14333 3.52451 galactic Aur Second-epoch detections are separated by 1.5" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:03:22.77 +47:20:53.9 (user input) | T | P | (position from user input) J-Ks=1.114+/-0.032 (M)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:03:22.77 +47:20:53.9: 14.34 +/- 0.08 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:03:22.77 +47:20:53.9: 14.26 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.30 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,13.31,0.05,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
target 20260910.4679 13.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.15 05:03:39.46 +47:19:39.7
160.18841 3.54944 galactic Aur Second-epoch detections are separated by 1.3" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J075.9144+47.3274 | 05:03:39.48 +47:19:38.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.310+/-0.028 (Very red! L if it's a dwarf)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:03:39.46 +47:19:39.7: 13.04 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:03:39.46 +47:19:39.7: 13.03 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.04 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J075.9144+47.3274,2461293.9679,12.15,0.05,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
ATO J075.9144+47.3274 20260910.4679 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.14 05:04:37.02 +46:41:29.7
160.79467 3.29421 galactic Aur Second-epoch detections are separated by 0.8" and 5.9 pix
The object was found in VSX 1" ASASSN-V J050437.03+464128.8
Type: SR
# Max. Min./Amp. JD0 Period
14.140 g Y 0.220 g 2459161.85000 46.150000000000
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:04:37.02 +46:41:29.7: 13.04 +/- 0.03 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:04:37.02 +46:41:29.7: 13.01 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J050437.03+464128.8,2461293.9679,12.14,0.05,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
ASASSN-V J050437.03+464128.8 20260910.4679 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.04 05:07:49.48 +47:34:59.4
160.40854 4.26582 galactic Aur Second-epoch detections are separated by 0.1" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J076.9588+47.5794 | 05:07:49.48 +47:34:59.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.663+/-0.032 (K)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:07:49.48 +47:34:59.4: 12.97 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:07:49.48 +47:34:59.4: 12.95 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J076.9588+47.5794,2461293.9679,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J076.9588+47.5794 20260910.4679 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.37 05:02:26.99 +47:23:31.5
160.01257 3.42624 galactic Aur Second-epoch detections are separated by 2.1" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J075.6101+47.3920 | 05:02:26.99 +47:23:31.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.861+/-0.031 (M)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:02:26.99 +47:23:31.5: 14.31 +/- 0.07 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:02:26.99 +47:23:31.5: 14.26 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.28 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J075.6101+47.3920,2461293.9679,13.37,0.05,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 J075.6101+47.3920 20260910.4679 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.34 05:08:15.96 +47:49:49.6
160.25367 4.47274 galactic Aur Second-epoch detections are separated by 0.9" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J077.0560+47.8397 | 05:08:15.96 +47:49:49.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.908+/-0.031 (M)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:08:15.96 +47:49:49.6: 14.31 +/- 0.07 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:08:15.96 +47:49:49.6: 14.29 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.30 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J077.0560+47.8397,2461293.9679,13.34,0.05,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
ATO J077.0560+47.8397 20260910.4679 13.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.31 05:01:53.73 +47:11:13.2
160.11781 3.22660 galactic Aur Second-epoch detections are separated by 2.1" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:01:53.73 +47:11:13.2 (user input) | T | P | (position from user input) J-Ks=0.173+/-0.040 (F)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:01:53.73 +47:11:13.2: 14.29 +/- 0.07 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:01:53.73 +47:11:13.2: 14.21 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.25 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,13.31,0.05,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
target 20260910.4679 13.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.36 04:53:04.08 +44:24:10.2
161.33972 0.28964 galactic Aur Second-epoch detections are separated by 1.5" and 6.0 pix
The object was found in VSX18" ZTF J045305.63+442404.8
Type: EA
# Max. Min./Amp. JD0 Period
15.141 r Y 0.206 r 2458425.83570 2.056358800000
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:53:04.08 +44:24:10.2: 14.32 +/- 0.07 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:53:04.08 +44:24:10.2: 14.31 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.32 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J045305.63+442404.8,2461293.9679,13.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J045305.63+442404.8 20260910.4679 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.18 05:04:06.32 +46:47:17.2
160.66455 3.28288 galactic Aur Second-epoch detections are separated by 2.9" and 6.2 pix
The object was found in VSX 8" Gaia DR3 207030828265833728
Type:
# Max. Min./Amp. JD0 Period
16.620 G 17.350 G
ATTENTION: measured mag 13.18 is 3.4 mag brighter than the VSX record maximum brightness 16.62 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:04:06.32 +46:47:17.2: 14.18 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:04:06.32 +46:47:17.2: 14.09 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.13 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 207030828265833728,2461293.9679,13.18,0.05,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 207030828265833728 20260910.4679 13.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.34 05:06:56.55 +47:28:49.4
160.40199 4.08500 galactic Aur Second-epoch detections are separated by 1.4" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J076.7478+47.4785 | 05:06:56.55 +47:28:49.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.427+/-0.036 (G)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:06:56.55 +47:28:49.4: 14.28 +/- 0.08 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:06:56.55 +47:28:49.4: 14.42 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.35 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J076.7478+47.4785,2461293.9679,13.34,0.05,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
ATO J076.7478+47.4785 20260910.4679 13.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.34 05:01:05.06 +47:06:23.0
160.09708 3.06819 galactic Aur Second-epoch detections are separated by 1.0" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J075.2788+47.1188 | 05:01:06.90 +47:06:53.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A1IV (LAMOST DR5) J-Ks=1.098+/-0.031 (M)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:01:05.06 +47:06:23.0: 14.24 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:01:05.06 +47:06:23.0: 14.26 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.25 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J075.2788+47.1188,2461293.9679,13.34,0.05,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
ATO J075.2788+47.1188 20260910.4679 13.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.35 04:56:26.97 +47:33:55.1
159.24961 2.73526 galactic Aur Second-epoch detections are separated by 1.3" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.1042+47.5685 | 04:56:26.97 +47:33:55.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.396+/-0.066 (G)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:56:26.97 +47:33:55.1: 14.29 +/- 0.07 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:56:26.97 +47:33:55.1: 14.31 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.30 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J074.1042+47.5685,2461293.9679,13.35,0.05,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 J074.1042+47.5685 20260910.4679 13.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.37 05:02:41.78 +47:22:29.3
160.05176 3.44880 galactic Aur Second-epoch detections are separated by 1.1" and 5.8 pix
The object was found in VSX 1" Gaia DR3 255063852717471104
Type: S
# Max. Min./Amp. JD0 Period
16.870 G 17.090 G
ATTENTION: measured mag 13.37 is 3.5 mag brighter than the VSX record maximum brightness 16.87 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:02:41.78 +47:22:29.3: 14.34 +/- 0.08 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:02:41.78 +47:22:29.3: 14.32 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.33 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 255063852717471104,2461293.9679,13.37,0.05,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 255063852717471104 20260910.4679 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.26 05:00:17.13 +47:22:52.0
159.79656 3.12990 galactic Aur Second-epoch detections are separated by 1.3" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:00:17.13 +47:22:52.0 (user input) | T | P | (position from user input) J-Ks=0.487+/-0.034 (K)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:00:17.13 +47:22:52.0: 14.35 +/- 0.08 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:00:17.13 +47:22:52.0: 14.41 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.38 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,13.26,0.05,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 20260910.4679 13.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.28 05:00:16.40 +47:05:20.2
160.02598 2.94856 galactic Aur Second-epoch detections are separated by 0.8" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:00:16.40 +47:05:20.2 (user input) | T | P | (position from user input) J-Ks=0.327+/-0.036 (G)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:00:16.40 +47:05:20.2: 14.30 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:00:16.40 +47:05:20.2: 14.38 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.34 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,13.28,0.05,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 20260910.4679 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 11.84 05:05:06.53 +47:40:24.4
160.06104 3.95374 galactic Aur Second-epoch detections are separated by 0.7" and 5.7 pix
The object was found in VSX 3" NSVS J0505068+474025
Type: L:
# Max. Min./Amp. JD0 Period
11.102 R1 Y 0.360 R1 90.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:05:06.53 +47:40:24.4: 12.80 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:05:06.53 +47:40:24.4: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.79 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J0505068+474025,2461293.9679,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0505068+474025 20260910.4679 11.84CV 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 09 10.4679 2461293.9679 13.31 05:01:07.78 +47:14:22.1
159.99652 3.15587 galactic Aur Second-epoch detections are separated by 0.6" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:01:07.78 +47:14:22.1 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.975+/-0.029 (M)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:01:07.78 +47:14:22.1: 14.28 +/- 0.07 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:01:07.78 +47:14:22.1: 14.28 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.28 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,13.31,0.05,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
target 20260910.4679 13.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.22 05:08:51.08 +47:46:01.6
160.36336 4.51416 galactic Aur Second-epoch detections are separated by 1.9" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J077.1971+47.7727 | 05:08:51.08 +47:46:01.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.979+/-0.031 (M)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:08:51.08 +47:46:01.6: 14.28 +/- 0.07 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:08:51.08 +47:46:01.6: 14.21 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.24 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J077.1971+47.7727,2461293.9679,13.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J077.1971+47.7727 20260910.4679 13.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.31 05:02:13.92 +46:39:46.1
160.56857 2.95185 galactic Aur Second-epoch detections are separated by 0.4" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:02:13.92 +46:39:46.1 (user input) | T | P | (position from user input) SpType: F6 (LAMOST DR5) J-Ks=0.441+/-0.031 (G)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:02:13.92 +46:39:46.1: 14.25 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:02:13.92 +46:39:46.1: 14.32 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.28 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,13.31,0.05,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
target 20260910.4679 13.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.30 04:55:58.38 +47:15:57.3
159.43315 2.48523 galactic Aur Second-epoch detections are separated by 1.7" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:55:58.38 +47:15:57.3 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.831+/-0.032 (M)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:55:58.38 +47:15:57.3: 14.27 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:55:58.38 +47:15:57.3: 14.32 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.29 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,13.30,0.05,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 20260910.4679 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.29 05:07:27.57 +47:22:16.1
160.54220 4.08977 galactic Aur Second-epoch detections are separated by 0.8" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J076.8514+47.3625 | 05:07:27.57 +47:22:16.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F6 (LAMOST DR5) J-Ks=0.425+/-0.033 (G)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:07:27.57 +47:22:16.1: 14.28 +/- 0.07 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:07:27.57 +47:22:16.1: 14.22 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.25 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J076.8514+47.3625,2461293.9679,13.29,0.05,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 J076.8514+47.3625 20260910.4679 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.25 05:00:37.93 +47:08:12.3
160.02580 3.02610 galactic Aur Second-epoch detections are separated by 1.3" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J075.1479+47.1343 | 05:00:37.93 +47:08:12.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.377+/-0.035 (G)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:00:37.93 +47:08:12.3: 14.27 +/- 0.07 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:00:37.93 +47:08:12.3: 14.17 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.21 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J075.1479+47.1343,2461293.9679,13.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J075.1479+47.1343 20260910.4679 13.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.27 05:03:18.46 +46:44:36.9
160.61695 3.14730 galactic Aur Second-epoch detections are separated by 0.7" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:03:18.46 +46:44:36.9 (user input) | T | P | (position from user input) SpType: A2V (LAMOST DR5) J-Ks=0.119+/-0.035 (A)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:03:18.46 +46:44:36.9: 14.25 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:03:18.46 +46:44:36.9: 14.17 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.21 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,13.27,0.05,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 20260910.4679 13.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.25 04:56:28.80 +47:02:13.9
159.66578 2.40955 galactic Aur Second-epoch detections are separated by 1.5" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:28.80 +47:02:13.9 (user input) | T | P | (position from user input) SpType: G4 (LAMOST DR5) J-Ks=0.503+/-0.036 (K)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:56:28.80 +47:02:13.9: 14.25 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:56:28.80 +47:02:13.9: 14.24 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.24 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,13.25,0.05,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 20260910.4679 13.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.25 05:01:40.77 +47:26:59.1
159.88712 3.35826 galactic Aur Second-epoch detections are separated by 2.5" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:01:40.77 +47:26:59.1 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.940+/-0.030 (M)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:01:40.77 +47:26:59.1: 14.26 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:01:40.77 +47:26:59.1: 14.40 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.32 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,13.25,0.05,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 20260910.4679 13.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.05 05:04:02.10 +46:59:48.2
160.49104 3.39974 galactic Aur Second-epoch detections are separated by 1.0" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:04:02.10 +46:59:48.2 (user input) | T | P | (position from user input) J-Ks=0.456+/-0.031 (G)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:04:02.10 +46:59:48.2: 14.24 +/- 0.07 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:04:02.10 +46:59:48.2: 14.01 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.10 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260910.4679 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 11.82 05:07:04.39 +47:35:51.3
160.32107 4.17279 galactic Aur Second-epoch detections are separated by 0.5" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J076.7683+47.5975 | 05:07:04.40 +47:35:51.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.128+/-0.029 (M)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:07:04.39 +47:35:51.3: 12.67 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:07:04.39 +47:35:51.3: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.68 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J076.7683+47.5975,2461293.9679,11.82,0.05,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 J076.7683+47.5975 20260910.4679 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.23 05:01:51.69 +47:14:47.1
160.06717 3.25834 galactic Aur Second-epoch detections are separated by 0.6" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:01:51.69 +47:14:47.1 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.284+/-0.032 (F)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:01:51.69 +47:14:47.1: 14.28 +/- 0.07 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:01:51.69 +47:14:47.1: 14.16 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.21 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,13.23,0.05,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 20260910.4679 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.21 04:55:49.40 +46:55:51.5
159.67865 2.25573 galactic Aur Second-epoch detections are separated by 1.0" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:55:49.40 +46:55:51.5 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=1.036+/-0.032 (M)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:55:49.40 +46:55:51.5: 14.22 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:55:49.40 +46:55:51.5: 14.20 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.21 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,13.21,0.05,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 20260910.4679 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.24 05:03:57.68 +46:42:44.9
160.70983 3.21741 galactic Aur Second-epoch detections are separated by 2.1" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J075.9962+46.7091 | 05:03:57.68 +46:42:44.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.398+/-0.035 (G)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:03:57.68 +46:42:44.9: 14.31 +/- 0.08 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:03:57.68 +46:42:44.9: 14.40 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.36 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J075.9962+46.7091,2461293.9679,13.24,0.05,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 J075.9962+46.7091 20260910.4679 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.16 05:02:55.51 +46:54:22.0
160.44790 3.19425 galactic Aur Second-epoch detections are separated by 0.1" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:02:55.51 +46:54:22.0 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.780+/-0.032 (K)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:02:55.51 +46:54:22.0: 14.23 +/- 0.07 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:02:55.51 +46:54:22.0: 14.20 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.21 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,13.16,0.05,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
target 20260910.4679 13.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.25 04:56:02.69 +47:02:27.8
159.61638 2.35409 galactic Aur Second-epoch detections are separated by 0.9" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:02.69 +47:02:27.8 (user input) | T | P | (position from user input) J-Ks=0.959+/-0.034 (M)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:56:02.69 +47:02:27.8: 14.25 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:56:02.69 +47:02:27.8: 14.23 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.24 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,13.25,0.05,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 20260910.4679 13.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.15 05:02:09.26 +47:15:09.8
160.09257 3.30154 galactic Aur Second-epoch detections are separated by 0.9" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:02:09.26 +47:15:09.8 (user input) | T | P | (position from user input) J-Ks=0.385+/-0.036 (G)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:02:09.26 +47:15:09.8: 14.23 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:02:09.26 +47:15:09.8: 14.19 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.21 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,13.15,0.05,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
target 20260910.4679 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.24 05:03:07.39 +46:44:39.5
160.59712 3.12265 galactic Aur Second-epoch detections are separated by 1.1" and 5.8 pix
The object was found in VSX19" Gaia DR3 206949047791037824
Type: E
# Max. Min./Amp. JD0 Period
18.880 G 19.080 G 2.020050000000
ATTENTION: measured mag 13.24 is 5.6 mag brighter than the VSX record maximum brightness 18.88 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:03:07.39 +46:44:39.5: 14.26 +/- 0.07 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:03:07.39 +46:44:39.5: 14.19 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.22 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 206949047791037824,2461293.9679,13.24,0.05,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 206949047791037824 20260910.4679 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.24 05:05:54.34 +47:28:38.5
160.29908 3.94301 galactic Aur Second-epoch detections are separated by 0.1" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J076.4781+47.4755 | 05:05:54.34 +47:28:38.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: K3 (LAMOST DR5) J-Ks=0.872+/-0.032 (M)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:05:54.34 +47:28:38.5: 14.21 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:05:54.34 +47:28:38.5: 14.16 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.19 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J076.4781+47.4755,2461293.9679,13.24,0.05,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 J076.4781+47.4755 20260910.4679 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.38 04:56:01.48 +49:13:39.8
157.90484 3.71810 galactic Aur Second-epoch detections are separated by 1.2" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:01.48 +49:13:39.8 (user input) | T | P | (position from user input) J-Ks=0.306+/-0.033 (F)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:56:01.48 +49:13:39.8: 14.25 +/- 0.07 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:56:01.48 +49:13:39.8: 14.30 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.28 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260910.4679 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.32 04:56:23.92 +47:18:55.6
159.43961 2.57253 galactic Aur Second-epoch detections are separated by 0.4" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:23.92 +47:18:55.6 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.333+/-0.068 (G)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:56:23.92 +47:18:55.6: 14.22 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:56:23.92 +47:18:55.6: 14.18 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.20 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,13.32,0.05,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 20260910.4679 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.26 05:02:42.25 +47:08:20.3
160.23993 3.30619 galactic Aur Second-epoch detections are separated by 0.9" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J075.6636+47.1417 | 05:02:42.25 +47:08:20.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.385+/-0.031 (G)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:02:42.25 +47:08:20.3: 14.19 +/- 0.07 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:02:42.25 +47:08:20.3: 14.14 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.16 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J075.6636+47.1417,2461293.9679,13.26,0.05,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 J075.6636+47.1417 20260910.4679 13.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.21 04:57:20.34 +47:11:17.2
159.63886 2.61791 galactic Aur Second-epoch detections are separated by 0.5" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.3450+47.1903 | 04:57:20.34 +47:11:17.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.831+/-0.029 (M)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:57:20.34 +47:11:17.2: 14.19 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:57:20.34 +47:11:17.2: 14.11 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.15 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J074.3450+47.1903,2461293.9679,13.21,0.05,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
ATO J074.3450+47.1903 20260910.4679 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.29 05:01:42.54 +47:08:57.3
160.12831 3.17843 galactic Aur Second-epoch detections are separated by 1.6" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J075.4416+47.1482 | 05:01:46.00 +47:08:53.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: M1 (LAMOST DR5) J-Ks=0.456+/-0.035 (G)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:01:42.54 +47:08:57.3: 14.21 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:01:42.54 +47:08:57.3: 14.20 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.20 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J075.4416+47.1482,2461293.9679,13.29,0.05,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 J075.4416+47.1482 20260910.4679 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.31 05:04:18.48 +46:32:29.1
160.88223 3.16109 galactic Aur Second-epoch detections are separated by 1.9" and 5.9 pix
The object was found in VSX 0" Gaia DR3 206836867541141632
Type: E
# Max. Min./Amp. JD0 Period
14.040 G 14.160 G 2.513010000000 A
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:04:18.48 +46:32:29.1: 14.17 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:04:18.48 +46:32:29.1: 14.30 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.23 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 206836867541141632,2461293.9679,13.31,0.05,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 206836867541141632 20260910.4679 13.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.27 05:02:06.22 +47:16:50.1
160.06522 3.31174 galactic Aur Second-epoch detections are separated by 0.6" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:02:06.22 +47:16:50.1 (user input) | T | P | (position from user input) J-Ks=0.832+/-0.029 (M)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:02:06.22 +47:16:50.1: 14.17 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:02:06.22 +47:16:50.1: 14.20 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.18 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,13.27,0.05,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 20260910.4679 13.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.23 05:02:29.62 +46:31:43.3
160.70241 2.90560 galactic Aur Second-epoch detections are separated by 1.1" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:02:29.62 +46:31:43.3 (user input) | T | P | (position from user input) J-Ks=0.222+/-0.032 (F)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:02:29.62 +46:31:43.3: 14.19 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:02:29.62 +46:31:43.3: 14.14 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.16 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,13.23,0.05,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 20260910.4679 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.30 04:59:53.13 +47:10:21.7
159.91923 2.94814 galactic Aur Second-epoch detections are separated by 1.8" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:59:53.13 +47:10:21.7 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.427+/-0.041 (G)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:59:53.13 +47:10:21.7: 14.20 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:59:53.13 +47:10:21.7: 14.23 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.21 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,13.30,0.05,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 20260910.4679 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.19 04:56:17.59 +47:03:46.5
159.62577 2.40077 galactic Aur Second-epoch detections are separated by 1.0" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:17.59 +47:03:46.5 (user input) | T | P | (position from user input) SpType: K3 (LAMOST DR5) J-Ks=0.600+/-0.032 (K)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:56:17.59 +47:03:46.5: 14.20 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:56:17.59 +47:03:46.5: 14.19 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.19 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,13.19,0.05,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 20260910.4679 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.18 05:02:52.91 +47:12:46.8
160.19953 3.37522 galactic Aur Second-epoch detections are separated by 1.1" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 207022818149774592 | 05:02:56.31 +47:13:04.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.483+/-0.033 (K)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:02:52.91 +47:12:46.8: 14.18 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:02:52.91 +47:12:46.8: 14.32 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.24 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 207022818149774592,2461293.9679,13.18,0.05,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 207022818149774592 20260910.4679 13.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.13 05:02:28.87 +46:45:41.4
160.51638 3.04592 galactic Aur Second-epoch detections are separated by 1.0" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:02:28.87 +46:45:41.4 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.436+/-0.036 (G)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:02:28.87 +46:45:41.4: 14.19 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:02:28.87 +46:45:41.4: 14.08 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.13 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,13.13,0.05,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 20260910.4679 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.12 05:02:21.53 +46:39:45.6
160.58198 2.96900 galactic Aur Second-epoch detections are separated by 2.7" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J075.5921+46.6636 | 05:02:21.53 +46:39:45.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.589+/-0.034 (K)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:02:21.53 +46:39:45.6: 14.16 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:02:21.53 +46:39:45.6: 14.11 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.14 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J075.5921+46.6636,2461293.9679,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J075.5921+46.6636 20260910.4679 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.13 05:01:43.58 +47:27:26.0
159.88604 3.36909 galactic Aur Second-epoch detections are separated by 1.7" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:01:43.58 +47:27:26.0 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.417+/-0.032 (G)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:01:43.58 +47:27:26.0: 14.16 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:01:43.58 +47:27:26.0: 14.09 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.13 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,13.13,0.05,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 20260910.4679 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.24 05:08:06.46 +47:56:07.5
160.15320 4.51387 galactic Aur Second-epoch detections are separated by 1.5" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J077.0087+47.9395 | 05:08:02.11 +47:56:22.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5) J-Ks=0.436+/-0.032 (G)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:08:06.46 +47:56:07.5: 14.17 +/- 0.07 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:08:06.46 +47:56:07.5: 14.17 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.17 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J077.0087+47.9395,2461293.9679,13.24,0.05,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 J077.0087+47.9395 20260910.4679 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.23 05:01:21.70 +47:17:11.4
159.98345 3.21579 galactic Aur Second-epoch detections are separated by 0.6" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J075.3416+47.2840 | 05:01:21.70 +47:17:11.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=1.129+/-0.031 (M)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:01:21.70 +47:17:11.4: 14.17 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:01:21.70 +47:17:11.4: 14.14 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.15 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J075.3416+47.2840,2461293.9679,13.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J075.3416+47.2840 20260910.4679 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.21 04:55:47.20 +47:06:08.1
159.54108 2.35810 galactic Aur Second-epoch detections are separated by 0.4" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J073.9598+47.1048 | 04:55:47.20 +47:06:08.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.733+/-0.030 (K)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:55:47.20 +47:06:08.1: 14.12 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:55:47.20 +47:06:08.1: 14.20 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.15 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J073.9598+47.1048,2461293.9679,13.21,0.05,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
ATO J073.9598+47.1048 20260910.4679 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.25 04:55:46.84 +46:45:13.0
159.81246 2.13898 galactic Aur Second-epoch detections are separated by 0.8" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:55:46.84 +46:45:13.0 (user input) | T | P | (position from user input) SpType: K4 (LAMOST DR5) J-Ks=1.315+/-0.032 (Very red! L if it's a dwarf)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:55:46.84 +46:45:13.0: 14.14 +/- 0.05 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:55:46.84 +46:45:13.0: 14.13 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.14 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,13.25,0.05,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 20260910.4679 13.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.23 04:58:05.50 +49:20:33.4
158.02470 4.05353 galactic Aur Second-epoch detections are separated by 1.1" and 5.6 pix
The object was found in VSX 1" Gaia DR3 256272039898315776
Type: ROT
# Max. Min./Amp. JD0 Period
13.740 G 13.770 G K
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:58:05.50 +49:20:33.4: 14.13 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:58:05.50 +49:20:33.4: 14.17 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.15 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 256272039898315776,2461293.9679,13.23,0.05,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 256272039898315776 20260910.4679 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.21 04:55:55.15 +47:11:21.2
159.48731 2.43011 galactic Aur Second-epoch detections are separated by 0.9" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J073.9644+47.1963 | 04:55:55.15 +47:11:21.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.284+/-0.042 (F)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:55:55.15 +47:11:21.2: 14.14 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:55:55.15 +47:11:21.2: 14.21 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.17 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J073.9644+47.1963,2461293.9679,13.21,0.05,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
ATO J073.9644+47.1963 20260910.4679 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.26 04:55:30.28 +44:47:41.5
161.30884 0.87348 galactic Aur Second-epoch detections are separated by 1.8" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:55:30.28 +44:47:41.5 (user input) | T | P | (position from user input) J-Ks=1.317+/-0.030 (Very red! L if it's a dwarf)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:55:30.28 +44:47:41.5: 14.14 +/- 0.07 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:55:30.28 +44:47:41.5: 14.20 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.17 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,13.26,0.05,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 20260910.4679 13.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.12 04:57:30.00 +47:12:41.8
159.63747 2.65394 galactic Aur Second-epoch detections are separated by 0.8" and 5.8 pix
The object was found in VSX 1" ZTF J045730.13+471241.5
Type: RS
# Max. Min./Amp. JD0 Period
14.100 r Y 0.036 r 2458353.99330 1.187690800000
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:57:30.00 +47:12:41.8: 14.13 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:57:30.00 +47:12:41.8: 14.10 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.11 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J045730.13+471241.5,2461293.9679,13.12,0.05,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
ZTF J045730.13+471241.5 20260910.4679 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.23 04:58:26.03 +44:28:39.9
161.88190 1.08275 galactic Aur Second-epoch detections are separated by 1.0" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:58:26.03 +44:28:39.9 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=1.180+/-0.031 (M)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:58:26.03 +44:28:39.9: 14.14 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:58:26.03 +44:28:39.9: 14.08 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.11 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,13.23,0.05,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 20260910.4679 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.18 05:02:19.62 +46:42:45.0
160.53911 2.99509 galactic Aur Second-epoch detections are separated by 2.6" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:02:19.62 +46:42:45.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:02:19.62 +46:42:45.0: 14.13 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:02:19.62 +46:42:45.0: 14.20 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.16 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,13.18,0.05,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
target 20260910.4679 13.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.18 05:00:15.82 +47:10:38.9
159.95508 3.00172 galactic Aur Second-epoch detections are separated by 1.1" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:00:15.82 +47:10:38.9 (user input) | T | P | (position from user input) J-Ks=0.953+/-0.033 (M)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:00:15.82 +47:10:38.9: 14.13 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:00:15.82 +47:10:38.9: 14.17 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.15 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,13.18,0.05,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
target 20260910.4679 13.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.22 04:44:00.58 +44:43:02.7
160.06001 -0.74221 galactic Per Second-epoch detections are separated by 0.8" and 5.7 pix
The object was found in VSX 1" ZTF J044400.59+444303.8
Type: SR
# Max. Min./Amp. JD0 Period
13.212 r Y 0.102 r 2458345.86650 31.197515900000
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:44:00.58 +44:43:02.7: 14.15 +/- 0.05 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:44:00.58 +44:43:02.7: 14.17 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.15 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 10.4679* 04 44 00.58 +44 43 02.7 13.2 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
ZTF J044400.59+444303.8,2461293.9679,13.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J044400.59+444303.8 20260910.4679 13.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.27 05:03:09.38 +46:36:57.9
160.70250 3.04915 galactic Aur Second-epoch detections are separated by 2.4" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:03:09.38 +46:36:57.9 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:03:09.38 +46:36:57.9: 14.10 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:03:09.38 +46:36:57.9: 14.22 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.15 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,13.27,0.05,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 20260910.4679 13.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.10 05:02:50.50 +47:06:23.4
160.28000 3.30497 galactic Aur Second-epoch detections are separated by 0.5" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J075.7194+47.0990 | 05:02:50.50 +47:06:23.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A5V (LAMOST DR5) J-Ks=0.381+/-0.035 (G)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:02:50.50 +47:06:23.4: 14.08 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:02:50.50 +47:06:23.4: 14.06 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.07 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J075.7194+47.0990,2461293.9679,13.10,0.05,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 J075.7194+47.0990 20260910.4679 13.10CV 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 09 10.4679 2461293.9679 13.22 05:07:12.57 +47:47:06.6
160.18404 4.30333 galactic Aur Second-epoch detections are separated by 0.7" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:07:12.57 +47:47:06.6 (user input) | T | P | (position from user input) J-Ks=0.667+/-0.030 (K)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:07:12.57 +47:47:06.6: 14.06 +/- 0.07 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:07:12.57 +47:47:06.6: 14.19 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.12 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,13.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260910.4679 13.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.03 05:02:50.91 +46:59:30.1
160.37192 3.23598 galactic Aur Second-epoch detections are separated by 0.5" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:02:50.91 +46:59:30.1 (user input) | T | P | (position from user input) J-Ks=0.490+/-0.033 (K)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:02:50.91 +46:59:30.1: 14.06 +/- 0.05 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:02:50.91 +46:59:30.1: 14.13 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.09 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,13.03,0.05,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 20260910.4679 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.94 05:03:15.72 +47:14:12.5
160.21993 3.44093 galactic Aur Second-epoch detections are separated by 0.9" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:03:15.72 +47:14:12.5 (user input) | T | P | (position from user input) J-Ks=0.970+/-0.031 (M)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:03:15.72 +47:14:12.5: 14.04 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:03:15.72 +47:14:12.5: 13.91 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.96 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260910.4679 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.14 04:58:05.82 +45:13:47.7
161.25507 1.50300 galactic Aur Second-epoch detections are separated by 2.2" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.5285+45.2276 | 04:58:05.82 +45:13:47.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=1.389+/-0.030 (Very red! L if it's a dwarf)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:58:05.82 +45:13:47.7: 14.05 +/- 0.05 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:58:05.82 +45:13:47.7: 14.00 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.03 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J074.5285+45.2276,2461293.9679,13.14,0.05,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 J074.5285+45.2276 20260910.4679 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.10 05:03:35.71 +47:32:26.7
160.01229 3.67031 galactic Aur Second-epoch detections are separated by 3.7" and 6.1 pix
The object was found in VSX22" ZTF J050336.57+473246.4
Type: EW
# Max. Min./Amp. JD0 Period
18.663 r Y 0.813 r 2458481.82380 0.259065800000
ATTENTION: measured mag 13.10 is 4.8 mag brighter than the VSX record maximum brightness 17.85 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:03:35.71 +47:32:26.7: 14.06 +/- 0.05 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:03:35.71 +47:32:26.7: 14.15 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.10 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J050336.57+473246.4,2461293.9679,13.10,0.05,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
ZTF J050336.57+473246.4 20260910.4679 13.10CV 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 09 10.4679 2461293.9679 13.12 05:08:47.02 +47:45:31.8
160.36327 4.50009 galactic Aur Second-epoch detections are separated by 2.8" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:08:47.02 +47:45:31.8 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:08:47.02 +47:45:31.8: 14.02 +/- 0.05 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:08:47.02 +47:45:31.8: 14.10 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.05 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,13.12,0.05,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 20260910.4679 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.13 05:10:04.10 +49:37:57.4
158.97171 5.77882 galactic Aur Second-epoch detections are separated by 0.8" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:10:04.10 +49:37:57.4 (user input) | T | P | (position from user input) J-Ks=0.328+/-0.034 (G)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:10:04.10 +49:37:57.4: 14.06 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:10:04.10 +49:37:57.4: 14.04 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.05 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,13.13,0.05,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 20260910.4679 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.04 05:04:18.25 +46:58:31.5
160.53587 3.42336 galactic Aur Second-epoch detections are separated by 1.5" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J076.0824+46.9755 | 05:04:21.20 +46:58:38.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:04:18.25 +46:58:31.5: 13.93 +/- 0.05 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:04:18.25 +46:58:31.5: 13.90 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.92 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J076.0824+46.9755,2461293.9679,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J076.0824+46.9755 20260910.4679 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.10 04:56:07.52 +44:36:13.5
161.52691 0.83963 galactic Aur Second-epoch detections are separated by 0.9" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:07.52 +44:36:13.5 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.792+/-0.030 (K)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:56:07.52 +44:36:13.5: 14.02 +/- 0.05 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:56:07.52 +44:36:13.5: 14.00 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.01 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,13.10,0.05,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 20260910.4679 13.10CV 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 09 10.4679 2461293.9679 12.85 05:06:24.25 +47:36:18.3
160.24733 4.08698 galactic Aur Second-epoch detections are separated by 1.3" and 5.9 pix
The object was found in VSX 2" ASASSN-V J050624.35+473617.1
Type: L
# Max. Min./Amp. JD0 Period
14.020 V 14.380 V
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:06:24.25 +47:36:18.3: 14.00 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:06:24.25 +47:36:18.3: 13.96 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.98 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J050624.35+473617.1,2461293.9679,12.85,0.05,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
ASASSN-V J050624.35+473617.1 20260910.4679 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.09 05:03:16.97 +47:03:26.6
160.36481 3.33470 galactic Aur Second-epoch detections are separated by 0.9" and 5.9 pix
The object was found in VSX13" Gaia DR3 207005711295440768
Type: RS
# Max. Min./Amp. JD0 Period
15.080 G 15.260 G K
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:03:16.97 +47:03:26.6: 14.04 +/- 0.05 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:03:16.97 +47:03:26.6: 14.20 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.11 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 207005711295440768,2461293.9679,13.09,0.05,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 207005711295440768 20260910.4679 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.88 05:02:45.01 +47:00:24.5
160.34969 3.23189 galactic Aur Second-epoch detections are separated by 0.3" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J075.6881+47.0067 | 05:02:45.01 +47:00:24.5 (user input) | IRR (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.250+/-0.030 (M)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:02:45.01 +47:00:24.5: 14.03 +/- 0.05 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:02:45.01 +47:00:24.5: 13.89 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.95 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J075.6881+47.0067,2461293.9679,12.88,0.05,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 J075.6881+47.0067 20260910.4679 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.12 05:03:52.33 +47:10:05.6
160.33756 3.48166 galactic Aur Second-epoch detections are separated by 2.4" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J075.9721+47.1701 | 05:03:52.33 +47:10:05.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:03:52.33 +47:10:05.6: 14.02 +/- 0.05 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:03:52.33 +47:10:05.6: 14.14 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.07 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J075.9721+47.1701,2461293.9679,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J075.9721+47.1701 20260910.4679 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.13 05:06:55.04 +47:17:28.4
160.55133 3.96835 galactic Aur Second-epoch detections are separated by 2.3" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:06:55.04 +47:17:28.4 (user input) | T | P | (position from user input) J-Ks=0.434+/-0.035 (G)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:06:55.04 +47:17:28.4: 13.99 +/- 0.05 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:06:55.04 +47:17:28.4: 14.02 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.00 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,13.13,0.05,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 20260910.4679 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.10 05:06:41.75 +47:41:11.2
160.21155 4.17506 galactic Aur Second-epoch detections are separated by 0.6" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:06:41.75 +47:41:11.2 (user input) | T | P | (position from user input) SpType: K4 (LAMOST DR5) J-Ks=0.896+/-0.030 (M)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:06:41.75 +47:41:11.2: 13.98 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:06:41.75 +47:41:11.2: 13.97 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.98 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,13.10,0.05,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 20260910.4679 13.10CV 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 09 10.4679 2461293.9679 13.04 04:56:02.20 +46:56:59.8
159.68665 2.29601 galactic Aur Second-epoch detections are separated by 0.2" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:02.20 +46:56:59.8 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.395+/-0.033 (G)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:56:02.20 +46:56:59.8: 13.97 +/- 0.05 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:56:02.20 +46:56:59.8: 13.94 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.95 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,13.04,0.05,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 20260910.4679 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.04 05:08:51.82 +47:35:29.6
160.50631 4.41162 galactic Aur Second-epoch detections are separated by 1.1" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:08:51.82 +47:35:29.6 (user input) | T | P | (position from user input) SpType: G1 (LAMOST DR5) J-Ks=0.336+/-0.033 (G)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:08:51.82 +47:35:29.6: 13.97 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:08:51.82 +47:35:29.6: 13.89 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.93 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,13.04,0.05,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 20260910.4679 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.07 04:56:13.20 +44:48:36.1
161.37655 0.98187 galactic Aur Second-epoch detections are separated by 1.5" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.0586+44.8085 | 04:56:13.20 +44:48:36.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.383+/-0.034 (G)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:56:13.20 +44:48:36.1: 13.93 +/- 0.05 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:56:13.20 +44:48:36.1: 14.03 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.98 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J074.0586+44.8085,2461293.9679,13.07,0.05,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
ATO J074.0586+44.8085 20260910.4679 13.07CV 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 09 10.4679 2461293.9679 13.03 05:03:26.09 +46:48:24.6
160.57990 3.20303 galactic Aur Second-epoch detections are separated by 0.5" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J075.8549+46.8080 | 05:03:26.09 +46:48:24.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.366+/-0.035 (G)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:03:26.09 +46:48:24.6: 13.95 +/- 0.05 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:03:26.09 +46:48:24.6: 13.99 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.97 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J075.8549+46.8080,2461293.9679,13.03,0.05,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 J075.8549+46.8080 20260910.4679 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.96 04:56:14.86 +47:13:00.3
159.50073 2.49087 galactic Aur Second-epoch detections are separated by 0.5" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:14.86 +47:13:00.3 (user input) | T | P | (position from user input) J-Ks=0.178+/-0.034 (F)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:56:14.86 +47:13:00.3: 13.95 +/- 0.05 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:56:14.86 +47:13:00.3: 13.87 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,12.96,0.05,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 20260910.4679 12.96CV 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 09 10.4679 2461293.9679 12.98 04:56:05.00 +47:04:00.0
159.60049 2.37522 galactic Aur Second-epoch detections are separated by 1.4" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.0178+47.0666 | 04:56:05.00 +47:04:00.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.340+/-0.034 (G)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:56:05.00 +47:04:00.0: 13.93 +/- 0.05 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:56:05.00 +47:04:00.0: 13.87 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J074.0178+47.0666,2461293.9679,12.98,0.05,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 J074.0178+47.0666 20260910.4679 12.98CV 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 09 10.4679 2461293.9679 12.94 05:02:15.69 +46:43:26.4
160.52313 2.99322 galactic Aur Second-epoch detections are separated by 0.4" and 5.8 pix
The object was found in VSX 1" ZTF J050215.64+464325.9
Type: SR
# Max. Min./Amp. JD0 Period
13.135 r Y 0.133 r 2458471.75030 28.903499400000
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:02:15.69 +46:43:26.4: 13.93 +/- 0.05 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:02:15.69 +46:43:26.4: 13.98 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.95 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J050215.64+464325.9,2461293.9679,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J050215.64+464325.9 20260910.4679 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.96 05:02:09.96 +46:52:58.4
160.38713 3.07730 galactic Aur Second-epoch detections are separated by 0.5" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:02:09.96 +46:52:58.4 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.389+/-0.031 (G)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:02:09.96 +46:52:58.4: 13.92 +/- 0.05 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:02:09.96 +46:52:58.4: 13.89 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,12.96,0.05,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 20260910.4679 12.96CV 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 09 10.4679 2461293.9679 12.88 04:56:05.57 +47:09:05.4
159.53524 2.42954 galactic Aur Second-epoch detections are separated by 1.5" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:05.57 +47:09:05.4 (user input) | T | P | (position from user input) J-Ks=0.901+/-0.031 (M)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:56:05.57 +47:09:05.4: 13.92 +/- 0.05 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:56:05.57 +47:09:05.4: 13.88 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,12.88,0.05,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 20260910.4679 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.02 05:11:01.03 +47:55:42.9
160.44803 4.90274 galactic Aur Second-epoch detections are separated by 0.6" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J077.7742+47.9214 | 05:11:04.58 +47:55:18.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.891+/-0.031 (M)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:11:01.03 +47:55:42.9: 13.98 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:11:01.03 +47:55:42.9: 14.12 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.04 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J077.7742+47.9214,2461293.9679,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J077.7742+47.9214 20260910.4679 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.97 05:00:40.64 +47:14:42.2
159.94493 3.09868 galactic Aur Second-epoch detections are separated by 0.6" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ASASSN-V J050043.60+471459.8 | 05:00:43.60 +47:14:59.8 (Gaia DR3) | SRS (local) | 27.148000000000 (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.981+/-0.029 (M)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:00:40.64 +47:14:42.2: 13.91 +/- 0.05 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:00:40.64 +47:14:42.2: 13.88 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.89 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J050043.60+471459.8,2461293.9679,12.97,0.05,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
ASASSN-V J050043.60+471459.8 20260910.4679 12.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.82 05:02:51.56 +47:19:11.6
160.11225 3.43726 galactic Aur Second-epoch detections are separated by 0.6" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:02:51.56 +47:19:11.6 (user input) | T | P | (position from user input) J-Ks=12.215+/- (unrealisitic color!)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:02:51.56 +47:19:11.6: 13.90 +/- 0.05 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:02:51.56 +47:19:11.6: 13.87 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.88 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,12.82,0.05,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 20260910.4679 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.03 05:08:05.72 +47:43:34.3
160.32058 4.38765 galactic Aur Second-epoch detections are separated by 0.6" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:08:05.72 +47:43:34.3 (user input) | T | P | (position from user input) J-Ks=0.467+/-0.033 (K)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:08:05.72 +47:43:34.3: 13.92 +/- 0.05 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:08:05.72 +47:43:34.3: 13.95 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.93 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,13.03,0.05,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 20260910.4679 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.99 05:06:33.48 +47:43:12.8
160.17050 4.17673 galactic Aur Second-epoch detections are separated by 0.7" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J076.6436+47.7195 | 05:06:33.48 +47:43:12.8 (user input) | IRR (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.895+/-0.033 (M)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:06:33.48 +47:43:12.8: 13.93 +/- 0.05 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:06:33.48 +47:43:12.8: 13.99 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.96 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J076.6436+47.7195,2461293.9679,12.99,0.05,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 J076.6436+47.7195 20260910.4679 12.99CV 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 09 10.4679 2461293.9679 13.02 04:54:04.75 +45:00:58.7
160.97788 0.81662 galactic Aur Second-epoch detections are separated by 0.9" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:54:04.75 +45:00:58.7 (user input) | T | P | (position from user input) J-Ks=1.254+/-0.031 (M)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:54:04.75 +45:00:58.7: 13.90 +/- 0.05 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:54:04.75 +45:00:58.7: 13.92 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.91 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,13.02,0.05,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 20260910.4679 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.85 05:03:07.74 +47:14:56.0
160.19657 3.43036 galactic Aur Second-epoch detections are separated by 0.5" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J075.7777+47.2508 | 05:03:07.74 +47:14:56.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.963+/-0.030 (M)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:03:07.74 +47:14:56.0: 13.91 +/- 0.05 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:03:07.74 +47:14:56.0: 13.81 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.85 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J075.7777+47.2508,2461293.9679,12.85,0.05,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
ATO J075.7777+47.2508 20260910.4679 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.94 04:56:13.61 +47:09:40.9
159.54179 2.45348 galactic Aur Second-epoch detections are separated by 0.5" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:13.61 +47:09:40.9 (user input) | T | P | (position from user input) J-Ks=0.193+/-0.031 (F)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:56:13.61 +47:09:40.9: 13.85 +/- 0.04 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:56:13.61 +47:09:40.9: 13.84 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.85 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260910.4679 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.97 05:02:56.42 +47:16:43.4
160.15334 3.42310 galactic Aur Second-epoch detections are separated by 0.2" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:02:56.42 +47:16:43.4 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=1.027+/-0.032 (M)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:02:56.42 +47:16:43.4: 13.89 +/- 0.05 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:02:56.42 +47:16:43.4: 13.90 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,12.97,0.05,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 20260910.4679 12.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.99 04:56:26.45 +47:11:39.2
159.53885 2.50241 galactic Aur Second-epoch detections are separated by 0.2" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.1122+47.1980 | 04:56:26.45 +47:11:39.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.575+/-0.046 (K)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:56:26.45 +47:11:39.2: 13.90 +/- 0.05 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:56:26.45 +47:11:39.2: 13.97 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.94 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J074.1122+47.1980,2461293.9679,12.99,0.05,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 J074.1122+47.1980 20260910.4679 12.99CV 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 09 10.4679 2461293.9679 13.09 05:03:32.97 +47:02:39.9
160.40277 3.36289 galactic Aur Second-epoch detections are separated by 0.5" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:03:32.97 +47:02:39.9 (user input) | T | P | (position from user input) J-Ks=0.690+/-0.030 (K)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:03:32.97 +47:02:39.9: 13.89 +/- 0.04 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:03:32.97 +47:02:39.9: 13.99 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.93 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260910.4679 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 12.93 04:56:02.49 +47:09:35.8
159.52319 2.42801 galactic Aur Second-epoch detections are separated by 1.6" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.0095+47.1640 | 04:56:02.49 +47:09:35.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A1V (LAMOST DR5) J-Ks=0.201+/-0.035 (F)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:56:02.49 +47:09:35.8: 13.85 +/- 0.04 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:56:02.49 +47:09:35.8: 13.93 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.89 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J074.0095+47.1640,2461293.9679,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J074.0095+47.1640 20260910.4679 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4679 2461293.9679 13.54 05:02:55.19 +46:59:41.7
160.37678 3.24759 galactic Aur Second-epoch detections are separated by 1.2" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:02:55.19 +46:59:41.7 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.949+/-0.032 (M)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:02:55.19 +46:59:41.7: 14.88 +/- 0.11 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:02:55.19 +46:59:41.7: 14.70 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.78 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9679,13.54,0.05,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
target 20260910.4679 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461093.60953049 22.02.2026 02:37:33.434 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
First image: 2461093.60953049 22.02.2026 02:37:33.434 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
Last image: 2461293.96823412 10.09.2026 11:14:05.428 /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q1b1x1_061447_TTUQ1b1x1_2992708_aEdEQksW/fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.73
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: 5 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 22164
Objects passed selection criteria: 22065
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 16096
Average stars matched: 15652.8 (97.2462 %)
Memory usage VmPeak: 247008 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Sep 10 02:28:55 CDT 2026
VaST build number 1.0rc89-204-g1bee8b93
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Sep 10 06:15:56 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: 2461093.60953049 22.02.2026 02:37:33.434 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
First image: 2461093.60953049 22.02.2026 02:37:33.434 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
Last image: 2461293.96823412 10.09.2026 11:14:05.428 /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q1b1x1_061447_TTUQ1b1x1_2992708_aEdEQksW/fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 346
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.37
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: 55 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 177670
Objects passed selection criteria: 177244
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 132664
Average stars matched: 127942 (96.4403 %)
Memory usage VmPeak: 640648 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Sep 10 02:28:55 CDT 2026
VaST build number 1.0rc89-204-g1bee8b93
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Sep 10 06:17:34 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 --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q1b1x1_061447_TTUQ1b1x1_2992708_aEdEQksW/fd_Per-03-Q1b1x1_2026-09-10_06-13-14_20.00sec_-0.00C_LIGHTs_0081.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q1b1x1_061447_TTUQ1b1x1_2992708_aEdEQksW/fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082.fits
SExtractor catalog cache: saved Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.cat to cache
SExtractor catalog cache: saved Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.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/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q1b1x1_061447_TTUQ1b1x1_2992708_aEdEQksW/fd_Per-03-Q1b1x1_2026-09-10_06-13-14_20.00sec_-0.00C_LIGHTs_0081.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q1b1x1_061447_TTUQ1b1x1_2992708_aEdEQksW/fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082.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: 2461293.96764399
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_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits exists and is non-empty
wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits exists and is non-empty
wcs_fd_Per-03-Q1b1x1_2026-09-10_06-13-14_20.00sec_-0.00C_LIGHTs_0081.fits exists and is non-empty
wcs_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits (1st reference image)
verification OK: wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
Image size: 941.6'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 04:48:00.727 +45:59:45.06 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Per-03-Q1b1x1_2026-09-10_06-13-14_20.00sec_-0.00C_LIGHTs_0081.fits (1st new image)
verification OK: wcs_fd_Per-03-Q1b1x1_2026-09-10_06-13-14_20.00sec_-0.00C_LIGHTs_0081.fits
Image size: 941.1'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 04:48:01.936 +46:00:08.71 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 04:48:00.727 +45:59:45.06
Second-epoch image center 04:48:01.936 +46:00:08.71
Angular distance between the image centers 0.0074 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082.fits (2nd new image)
verification OK: wcs_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082.fits
Image size: 941.1'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 04:48:03.423 +46:00:39.02 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 04:48:00.727 +45:59:45.06
Second-epoch image center 04:48:03.423 +46:00:39.02
Angular distance between the image centers 0.0169 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 04:48:01.936 +46:00:08.71
Second-epoch second image center 04:48:03.423 +46:00:39.02
Angular distance between the image centers 0.00946 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits &> /tmp/tmp.BAKyOgIAKi
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits &> /tmp/tmp.WyGwopptf4
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q1b1x1_061447_TTUQ1b1x1_2992708_aEdEQksW/fd_Per-03-Q1b1x1_2026-09-10_06-13-14_20.00sec_-0.00C_LIGHTs_0081.fits &> /tmp/tmp.qcY8lhDOK1
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q1b1x1_061447_TTUQ1b1x1_2992708_aEdEQksW/fd_Per-03-Q1b1x1_2026-09-10_06-13-14_20.00sec_-0.00C_LIGHTs_0081.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q1b1x1_061447_TTUQ1b1x1_2992708_aEdEQksW/fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082.fits &> /tmp/tmp.0WRRcn9dhT
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q1b1x1_061447_TTUQ1b1x1_2992708_aEdEQksW/fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082.fits
Calibrating the magnitude scale
Found non-empty wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.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_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits and wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits and wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat
Found non-empty wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits and wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat
The reference image (wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits) and catalog (wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat) found
'wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat' -> 'wcsmag.cat'
Read 23847 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 59.9496 to 84.6399 deg, Dec +39.9317 to +51.3292 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 59.9496 to 84.6399 deg, Dec 39.9317 to 51.3292 deg
Loaded 12139 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): 8124 out of 9276 total matches.
Matched with Tycho-2 9276 out of 23847 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.951350
a=0.000000 b=1.000000 c=22.951350
From vast_summary.log: estimated ref. image limiting mag.: -7.73
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.22
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.22
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 23847 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 59.9496 to 84.6399 deg, Dec +39.9317 to +51.3292 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 59.9496 to 84.6399 deg, Dec 39.9317 to 51.3292 deg
Loaded 12139 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): 8124 out of 9276 total matches.
Matched with Tycho-2 9276 out of 23847 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
Forced-photometry filter: calibrated wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits -> calib.txt_param_ref_wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits (aperture=6.1)
Read 23965 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 59.9494 to 84.6297 deg, Dec +39.9321 to +51.3293 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 59.9494 to 84.6297 deg, Dec 39.9321 to 51.3293 deg
Loaded 12131 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): 8135 out of 9280 total matches.
Matched with Tycho-2 9280 out of 23965 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
Forced-photometry filter: calibrated wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits -> calib.txt_param_ref_wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits (aperture=6.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 4 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
2.1 pix Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
2.8 pix fd_Per-03-Q1b1x1_2026-09-10_06-13-14_20.00sec_-0.00C_LIGHTs_0081.fits
2.7 pix fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082.fits
Limiting magnitude estimates:
15.2 mag. Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
15.2 mag. Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
13.4 mag. fd_Per-03-Q1b1x1_2026-09-10_06-13-14_20.00sec_-0.00C_LIGHTs_0081.fits
13.4 mag. fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082.fits
All-image limiting magnitude estimate: 13.4 (SNR ) 11.1 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.BAKyOgIAKi (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-10_CI_Per-03-Q1b1x1_061447_TTUQ1b1x1_2992708_aEdEQksW/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits' -> 'wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
WCS_IMAGE_NAME=wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
WCS-calibrated image found: wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
Checking if the catalog wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat corresponding to the image wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits alredy exist and is non-empty...
Catalog wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat corresponding to the image wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
WCS catalog name: wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2564, bad_region=0, passed=23847
Got 23847 stars (including 21254 good ones) from the SExtractor catalog wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat
util/solve_plate_with_UCAC5 got 23847 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.3)
Done reading UCAC5 zone files...
Matched 4918 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4871 matched stars entering correct_measured_positions(), 4871 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4871 matched stars entering correct_measured_positions(), 23847 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.3)
Done reading UCAC5 zone files...
Matched 4918 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4872 matched stars entering correct_measured_positions(), 23847 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 4872 matched stars entering correct_measured_positions(), 23847 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 4872 stars left (next iteration limit 5358)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits N_match=4872 sigma_overall_arcsec=0.443 sigma_q1_arcsec=0.581 sigma_q2_arcsec=0.429 sigma_q3_arcsec=0.440 sigma_q4_arcsec=0.341 n_q1=1102 n_q2=1035 n_q3=1609 n_q4=1126 worst_quadrant_to_overall_ratio=1.312
The image catalog is written to wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits -region wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.WyGwopptf4 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-10_CI_Per-03-Q1b1x1_061447_TTUQ1b1x1_2992708_aEdEQksW/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits' -> 'wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
WCS_IMAGE_NAME=wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
WCS-calibrated image found: wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
Checking if the catalog wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat corresponding to the image wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits alredy exist and is non-empty...
Catalog wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat corresponding to the image wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
WCS catalog name: wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2577, bad_region=0, passed=23965
Got 23965 stars (including 21358 good ones) from the SExtractor catalog wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat
util/solve_plate_with_UCAC5 got 23965 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.3)
Done reading UCAC5 zone files...
Matched 4914 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4868 matched stars entering correct_measured_positions(), 4868 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4868 matched stars entering correct_measured_positions(), 23965 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.3)
Done reading UCAC5 zone files...
Matched 4914 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4869 matched stars entering correct_measured_positions(), 23965 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 4869 matched stars entering correct_measured_positions(), 23965 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 4869 stars left (next iteration limit 5354)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits N_match=4869 sigma_overall_arcsec=0.448 sigma_q1_arcsec=0.587 sigma_q2_arcsec=0.429 sigma_q3_arcsec=0.436 sigma_q4_arcsec=0.343 n_q1=1104 n_q2=1036 n_q3=1603 n_q4=1126 worst_quadrant_to_overall_ratio=1.308
The image catalog is written to wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits -region wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.qcY8lhDOK1 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-10_CI_Per-03-Q1b1x1_061447_TTUQ1b1x1_2992708_aEdEQksW/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q1b1x1_061447_TTUQ1b1x1_2992708_aEdEQksW/fd_Per-03-Q1b1x1_2026-09-10_06-13-14_20.00sec_-0.00C_LIGHTs_0081.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q1b1x1_061447_TTUQ1b1x1_2992708_aEdEQksW/fd_Per-03-Q1b1x1_2026-09-10_06-13-14_20.00sec_-0.00C_LIGHTs_0081.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q1b1x1_061447_TTUQ1b1x1_2992708_aEdEQksW/fd_Per-03-Q1b1x1_2026-09-10_06-13-14_20.00sec_-0.00C_LIGHTs_0081.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q1b1x1_061447_TTUQ1b1x1_2992708_aEdEQksW/fd_Per-03-Q1b1x1_2026-09-10_06-13-14_20.00sec_-0.00C_LIGHTs_0081.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q1b1x1_061447_TTUQ1b1x1_2992708_aEdEQksW/fd_Per-03-Q1b1x1_2026-09-10_06-13-14_20.00sec_-0.00C_LIGHTs_0081.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q1b1x1_061447_TTUQ1b1x1_2992708_aEdEQksW/fd_Per-03-Q1b1x1_2026-09-10_06-13-14_20.00sec_-0.00C_LIGHTs_0081.fits
WCS_IMAGE_NAME=wcs_fd_Per-03-Q1b1x1_2026-09-10_06-13-14_20.00sec_-0.00C_LIGHTs_0081.fits
WCS-calibrated image found: wcs_fd_Per-03-Q1b1x1_2026-09-10_06-13-14_20.00sec_-0.00C_LIGHTs_0081.fits
Checking if the catalog wcs_fd_Per-03-Q1b1x1_2026-09-10_06-13-14_20.00sec_-0.00C_LIGHTs_0081.fits.wcscat corresponding to the image wcs_fd_Per-03-Q1b1x1_2026-09-10_06-13-14_20.00sec_-0.00C_LIGHTs_0081.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-03-Q1b1x1_2026-09-10_06-13-14_20.00sec_-0.00C_LIGHTs_0081.fits.wcscat corresponding to the image wcs_fd_Per-03-Q1b1x1_2026-09-10_06-13-14_20.00sec_-0.00C_LIGHTs_0081.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-03-Q1b1x1_2026-09-10_06-13-14_20.00sec_-0.00C_LIGHTs_0081.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q1b1x1_061447_TTUQ1b1x1_2992708_aEdEQksW/fd_Per-03-Q1b1x1_2026-09-10_06-13-14_20.00sec_-0.00C_LIGHTs_0081.fits
WCS catalog name: wcs_fd_Per-03-Q1b1x1_2026-09-10_06-13-14_20.00sec_-0.00C_LIGHTs_0081.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=354, bad_region=0, passed=8804
Got 8804 stars (including 8441 good ones) from the SExtractor catalog wcs_fd_Per-03-Q1b1x1_2026-09-10_06-13-14_20.00sec_-0.00C_LIGHTs_0081.fits.wcscat
util/solve_plate_with_UCAC5 got 8804 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (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 0.010457 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.0 to 51.4)
Done reading UCAC5 zone files...
Matched 4913 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4848 matched stars entering correct_measured_positions(), 4848 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4848 matched stars entering correct_measured_positions(), 8804 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.0 to 51.4)
Done reading UCAC5 zone files...
Matched 4914 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4850 matched stars entering correct_measured_positions(), 8804 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4850 matched stars entering correct_measured_positions(), 8804 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 4850 stars left (next iteration limit 5332)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4850 robust_rms=9.968 arcsec worst_quadrant_rms=12.011 arcsec
SIP_REFIT: SIP order 3 trial: matched=4850 robust_rms=0.388 arcsec worst_quadrant_rms=0.410 arcsec
SIP_REFIT: SIP order 5 trial: matched=4850 robust_rms=0.331 arcsec worst_quadrant_rms=0.377 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4850 robust_rms_before=0.851 arcsec robust_rms_before_corrected=0.398 arcsec robust_rms_after=0.331 arcsec worst_quadrant_rms_before=0.463 worst_quadrant_rms_after=0.377
verification OK: wcs_fd_Per-03-Q1b1x1_2026-09-10_06-13-14_20.00sec_-0.00C_LIGHTs_0081.fits
verification OK: wcs_fd_Per-03-Q1b1x1_2026-09-10_06-13-14_20.00sec_-0.00C_LIGHTs_0081.fits
Image size: 941.3'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 04:48:01.954 +46:00:07.99 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 8804 stars ###
'wcs_fd_Per-03-Q1b1x1_2026-09-10_06-13-14_20.00sec_-0.00C_LIGHTs_0081.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-09-10_CI_Per-03-Q1b1x1_061447_TTUQ1b1x1_2992708_aEdEQksW/correct_sextractor_wcs_catalog_usingxy2sky3001189.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 0.851 -> 0.331 arcsec)
SIP_REFIT: re-matching the catalog with the refit solution (search radius 3.0 arcsec, 4850 pairs from the initial matching)
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.0 to 51.4)
Done reading UCAC5 zone files...
Matched 4665 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
SIP_REFIT: re-match found 4665 pairs (4850 from the initial matching)
SIP_REFIT: SIP order 2 trial: matched=4665 robust_rms=9.625 arcsec worst_quadrant_rms=11.867 arcsec
SIP_REFIT: SIP order 3 trial: matched=4665 robust_rms=0.386 arcsec worst_quadrant_rms=0.406 arcsec
SIP_REFIT: SIP order 5 trial: matched=4665 robust_rms=0.330 arcsec worst_quadrant_rms=0.374 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4665 robust_rms_before=0.329 arcsec robust_rms_before_corrected=0.329 arcsec robust_rms_after=0.330 arcsec worst_quadrant_rms_before=0.374 worst_quadrant_rms_after=0.374
SIP_REFIT: the refit on the re-matched pairs is worse than the solution it would replace (worst-quadrant 0.374 vs 0.374 arcsec) - keeping the current solution
SIP_REFIT: the second refit on the re-matched pairs was not applied - keeping the first refit solution
Accuracy estimation diagnostic: 4665 matched stars entering correct_measured_positions(), 8804 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 4665 matched stars entering correct_measured_positions(), 8804 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
WCS_QUALITY_DIAG: file=fd_Per-03-Q1b1x1_2026-09-10_06-13-14_20.00sec_-0.00C_LIGHTs_0081.fits N_match=4665 sigma_overall_arcsec=0.360 sigma_q1_arcsec=0.381 sigma_q2_arcsec=0.406 sigma_q3_arcsec=0.304 sigma_q4_arcsec=0.341 n_q1=1086 n_q2=1407 n_q3=930 n_q4=1242 worst_quadrant_to_overall_ratio=1.127
The image catalog is written to wcs_fd_Per-03-Q1b1x1_2026-09-10_06-13-14_20.00sec_-0.00C_LIGHTs_0081.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-03-Q1b1x1_2026-09-10_06-13-14_20.00sec_-0.00C_LIGHTs_0081.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q1b1x1_061447_TTUQ1b1x1_2992708_aEdEQksW/fd_Per-03-Q1b1x1_2026-09-10_06-13-14_20.00sec_-0.00C_LIGHTs_0081.fits -region wcs_fd_Per-03-Q1b1x1_2026-09-10_06-13-14_20.00sec_-0.00C_LIGHTs_0081.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-03-Q1b1x1_2026-09-10_06-13-14_20.00sec_-0.00C_LIGHTs_0081.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.0WRRcn9dhT (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-10_CI_Per-03-Q1b1x1_061447_TTUQ1b1x1_2992708_aEdEQksW/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q1b1x1_061447_TTUQ1b1x1_2992708_aEdEQksW/fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q1b1x1_061447_TTUQ1b1x1_2992708_aEdEQksW/fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q1b1x1_061447_TTUQ1b1x1_2992708_aEdEQksW/fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q1b1x1_061447_TTUQ1b1x1_2992708_aEdEQksW/fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q1b1x1_061447_TTUQ1b1x1_2992708_aEdEQksW/fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q1b1x1_061447_TTUQ1b1x1_2992708_aEdEQksW/fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082.fits
WCS_IMAGE_NAME=wcs_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082.fits
WCS-calibrated image found: wcs_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082.fits
Checking if the catalog wcs_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082.fits.wcscat corresponding to the image wcs_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082.fits.wcscat corresponding to the image wcs_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q1b1x1_061447_TTUQ1b1x1_2992708_aEdEQksW/fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082.fits
WCS catalog name: wcs_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=322, bad_region=0, passed=8136
Got 8136 stars (including 7806 good ones) from the SExtractor catalog wcs_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082.fits.wcscat
util/solve_plate_with_UCAC5 got 8136 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (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 0.010457 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.0 to 51.4)
Done reading UCAC5 zone files...
Matched 4902 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4833 matched stars entering correct_measured_positions(), 4833 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4833 matched stars entering correct_measured_positions(), 8136 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.0 to 51.4)
Done reading UCAC5 zone files...
Matched 4905 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4835 matched stars entering correct_measured_positions(), 8136 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 4835 matched stars entering correct_measured_positions(), 8136 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 4835 stars left (next iteration limit 5316)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4835 robust_rms=9.653 arcsec worst_quadrant_rms=11.508 arcsec
SIP_REFIT: SIP order 3 trial: matched=4835 robust_rms=0.413 arcsec worst_quadrant_rms=0.446 arcsec
SIP_REFIT: SIP order 5 trial: matched=4835 robust_rms=0.356 arcsec worst_quadrant_rms=0.380 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4835 robust_rms_before=0.872 arcsec robust_rms_before_corrected=0.408 arcsec robust_rms_after=0.356 arcsec worst_quadrant_rms_before=0.453 worst_quadrant_rms_after=0.380
verification OK: wcs_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082.fits
verification OK: wcs_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082.fits
Image size: 941.2'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 04:48:03.447 +46:00:38.33 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 8136 stars ###
'wcs_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-09-10_CI_Per-03-Q1b1x1_061447_TTUQ1b1x1_2992708_aEdEQksW/correct_sextractor_wcs_catalog_usingxy2sky3001180.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 0.872 -> 0.356 arcsec)
SIP_REFIT: re-matching the catalog with the refit solution (search radius 3.0 arcsec, 4835 pairs from the initial matching)
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.0 to 51.4)
Done reading UCAC5 zone files...
Matched 4649 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
SIP_REFIT: re-match found 4649 pairs (4835 from the initial matching)
SIP_REFIT: SIP order 2 trial: matched=4649 robust_rms=9.374 arcsec worst_quadrant_rms=11.262 arcsec
SIP_REFIT: SIP order 3 trial: matched=4649 robust_rms=0.405 arcsec worst_quadrant_rms=0.443 arcsec
SIP_REFIT: SIP order 5 trial: matched=4649 robust_rms=0.351 arcsec worst_quadrant_rms=0.373 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4649 robust_rms_before=0.353 arcsec robust_rms_before_corrected=0.353 arcsec robust_rms_after=0.351 arcsec worst_quadrant_rms_before=0.375 worst_quadrant_rms_after=0.373
verification OK: wcs_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082.fits
verification OK: wcs_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082.fits
Image size: 941.2'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 04:48:03.448 +46:00:38.33 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 8136 stars ###
'wcs_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-09-10_CI_Per-03-Q1b1x1_061447_TTUQ1b1x1_2992708_aEdEQksW/correct_sextractor_wcs_catalog_usingxy2sky3001858.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 0.353 -> 0.351 arcsec)
Accuracy estimation diagnostic: 4649 matched stars entering correct_measured_positions(), 8136 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 4649 matched stars entering correct_measured_positions(), 8136 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
WCS_QUALITY_DIAG: file=fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082.fits N_match=4649 sigma_overall_arcsec=0.373 sigma_q1_arcsec=0.389 sigma_q2_arcsec=0.396 sigma_q3_arcsec=0.329 sigma_q4_arcsec=0.368 n_q1=1173 n_q2=1574 n_q3=846 n_q4=1056 worst_quadrant_to_overall_ratio=1.063
The image catalog is written to wcs_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q1b1x1_061447_TTUQ1b1x1_2992708_aEdEQksW/fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082.fits -region wcs_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits to local_wcs_cache/
'wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits' -> 'local_wcs_cache/wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits'
Saving the final (post-refit) wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits to local_wcs_cache/
'wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits' -> 'local_wcs_cache/wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits'
Saving the final (post-refit) wcs_fd_Per-03-Q1b1x1_2026-09-10_06-13-14_20.00sec_-0.00C_LIGHTs_0081.fits to local_wcs_cache/
'wcs_fd_Per-03-Q1b1x1_2026-09-10_06-13-14_20.00sec_-0.00C_LIGHTs_0081.fits' -> 'local_wcs_cache/wcs_fd_Per-03-Q1b1x1_2026-09-10_06-13-14_20.00sec_-0.00C_LIGHTs_0081.fits'
Saving the final (post-refit) wcs_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082.fits to local_wcs_cache/
'wcs_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082.fits' -> 'local_wcs_cache/wcs_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits sigma_overall=0.443 worst_q_ratio=1.312
ref2=Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits sigma_overall=0.448 worst_q_ratio=1.308
new1=fd_Per-03-Q1b1x1_2026-09-10_06-13-14_20.00sec_-0.00C_LIGHTs_0081.fits sigma_overall=0.360 worst_q_ratio=1.127
new2=fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082.fits sigma_overall=0.373 worst_q_ratio=1.063
reference average sigma_overall=0.4455 worst_q_ratio=1.31
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044_astrometric_residuals.png (4872 matched stars from wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.40 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045_astrometric_residuals.png (4869 matched stars from wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.40 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Per-03-Q1b1x1_2026-09-10_06-13-14_20.00sec_-0.00C_LIGHTs_0081_astrometric_residuals.png (4665 matched stars from wcs_fd_Per-03-Q1b1x1_2026-09-10_06-13-14_20.00sec_-0.00C_LIGHTs_0081.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.28 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082_astrometric_residuals.png (4649 matched stars from wcs_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.28 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Per-03-Q1b1x1_2026-09-10_06-13-14_20.00sec_-0.00C_LIGHTs_0081.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Per-03-Q1b1x1_2026-09-10_06-13-14_20.00sec_-0.00C_LIGHTs_0081.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q1b1x1_061447_TTUQ1b1x1_2992708_aEdEQksW/wcs_fd_Per-03-Q1b1x1_2026-09-10_06-13-14_20.00sec_-0.00C_LIGHTs_0081.fits'
Saving fully-calibrated image wcs_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q1b1x1_061447_TTUQ1b1x1_2992708_aEdEQksW/wcs_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082.fits'
Preparing the HTML report for the field Per-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
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: 0s
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Considering the candidate 31719_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 31719_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:58:31.53 +40:46:20.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31749_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 31749_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:32:36.69 +45:40:13.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 07304_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 07304_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 05:03:12.46 +47:09:04.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 00847_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 00847_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
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Considering the candidate 223900_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 223900_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:28:38.19 +42:48:21.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 223912_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 223912_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
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Considering the candidate 223922_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 223922_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:52:14.19 +48:50:44.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 223925_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 223925_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:57:16.08 +40:54:55.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 223928_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 223928_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
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Considering the candidate 223931_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 223931_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
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Considering the candidate 223934_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 223934_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:19:15.98 +44:38:20.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 223936_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 223936_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
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Considering the candidate 223937_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 223937_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 05:27:21.49 +44:01:16.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 223939_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 223939_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
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Considering the candidate 223940_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 223940_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:51:55.88 +42:03:20.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 223942_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 223942_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
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Considering the candidate 223943_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 223943_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:16:51.34 +46:30:12.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 223944_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 223944_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:29:40.38 +42:26:03.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 223946_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 223946_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:12:28.17 +44:21:27.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 223955_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 223955_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:20:48.08 +46:24:02.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 223956_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 223956_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
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Considering the candidate 223957_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 223957_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:27:23.83 +44:27:02.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 223959_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 223959_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:17:10.38 +44:27:37.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 223963_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 223963_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
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Considering the candidate 223964_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 223964_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:18:34.64 +43:02:51.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 223966_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 223966_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
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Considering the candidate 223967_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 223967_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:28:50.99 +41:45:03.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 223968_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 223968_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
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Considering the candidate 223969_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 223969_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:56:51.21 +42:50:51.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 223970_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 223970_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:30:26.76 +41:49:49.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 223971_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 223971_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:30:19.04 +45:56:09.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 223972_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 223972_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:22:17.61 +47:18:35.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 223974_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 223974_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:03:55.88 +47:05:01.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 223975_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 223975_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 05:19:02.98 +49:02:03.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 223976_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 223976_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 223977_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 223977_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 223980_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 223980_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:13:27.47 +43:54:15.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 223989_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 223989_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 223990_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 223990_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:11:04.21 +45:12:25.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 223994_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 223994_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:51:01.41 +41:27:12.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 223995_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 223995_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:58:31.56 +40:46:20.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224041_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224041_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224062_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224062_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:55:46.93 +43:10:21.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224077_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224077_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:23:59.66 +41:56:29.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224098_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224098_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 05:18:54.60 +41:06:56.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224099_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224099_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 05:19:05.99 +49:03:07.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224102_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224102_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:16:39.52 +45:38:10.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224107_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224107_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:47:24.60 +46:00:22.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224110_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224110_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 05:06:36.91 +46:13:49.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224114_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224114_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 05:19:53.25 +44:25:23.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224121_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224121_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:52:57.33 +42:34:49.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224141_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224141_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:43:07.71 +45:37:58.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224145_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224145_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:17:16.06 +46:11:55.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224146_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224146_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:24:24.71 +41:42:26.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224150_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224150_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 05:12:14.35 +45:35:48.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224155_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224155_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:15:09.61 +50:40:22.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224160_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224160_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:43:31.99 +49:59:18.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224169_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224169_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224172_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224172_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:49:32.86 +46:30:01.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224180_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224180_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224181_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224181_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 05:01:52.82 +43:51:45.9 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224182_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224182_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:58:01.73 +49:10:32.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224183_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224183_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:51:41.70 +42:03:19.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224186_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224186_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224188_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224188_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:55:24.17 +43:25:00.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224192_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224192_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:10:26.14 +46:31:19.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224194_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224194_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224197_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224197_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:07:24.20 +43:17:40.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224201_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224201_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:26:26.73 +46:09:30.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224204_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224204_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 05:11:47.07 +45:38:45.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224207_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224207_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:36:40.86 +45:01:00.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224211_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224211_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:35:36.67 +45:11:49.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224213_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224213_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 05:11:12.03 +42:54:38.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224215_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224215_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224216_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224216_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:57:58.07 +49:13:15.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224220_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224220_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224222_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224222_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:15:03.56 +47:53:25.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224228_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224228_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:56:55.95 +43:08:00.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224234_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224234_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:58:54.60 +41:03:07.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224236_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224236_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 05:02:06.29 +43:47:14.2 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224237_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224237_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224240_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224240_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:55:20.34 +43:23:43.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224245_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224245_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:56:47.30 +49:14:01.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224252_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224252_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 05:09:50.26 +42:30:42.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224257_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224257_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:46:21.01 +42:21:55.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224266_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224266_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:54:55.11 +42:57:04.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224269_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224269_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224272_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224272_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:03:38.56 +46:47:28.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224274_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224274_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:48:58.13 +43:57:59.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224277_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224277_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:53:16.18 +42:56:27.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224286_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224286_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224288_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224288_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:27:48.30 +46:15:02.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224289_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224289_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
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Considering the candidate 224295_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224295_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
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Considering the candidate 224299_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224299_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 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 224307_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224307_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 05:13:55.28 +43:33:25.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 224313_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224313_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 05:04:16.07 +45:48:23.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 224314_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224314_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 05:02:02.12 +41:20:06.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 224318_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224318_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:55:39.07 +46:07:51.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 224319_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224319_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:48:56.61 +43:59:04.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 224324_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224324_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:12:41.31 +43:31:45.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 224339_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224339_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:32:38.45 +44:53:37.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 224348_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224348_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:45:54.80 +43:23:21.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 224363_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224363_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
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Considering the candidate 224365_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224365_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:46:35.27 +42:20:25.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 224373_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 224373_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:55:56.92 +44:32:01.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53525_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 53525_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 63541_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 63541_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 65185_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 65185_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 59606_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 59606_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 72036_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 72036_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 73768_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 73768_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 76073_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 76073_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 68794_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 68794_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
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Considering the candidate 96771_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 96771_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 51777_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 51777_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 70798_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 70798_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 63112_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 63112_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 63594_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 63594_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 65486_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 65486_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 52913_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 52913_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 73587_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 73587_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
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Considering the candidate 54442_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 54442_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 66845_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 66845_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 68150_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 68150_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 64661_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 64661_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 82117_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 82117_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 05:13:19.27 +45:57:06.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 58504_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 58504_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 32052_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 32052_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 62226_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 62226_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 54169_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 54169_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 65765_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 65765_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 73213_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 73213_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:58:46.46 +46:42:00.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 61412_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 61412_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 73792_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 73792_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 57703_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 57703_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 64972_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 64972_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 62834_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 62834_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 60482_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 60482_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 64452_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 64452_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 58327_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 58327_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 50385_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 50385_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 65332_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 65332_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 59920_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 59920_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 70125_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 70125_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 58360_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 58360_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 05:06:40.34 +47:24:49.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 64666_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 64666_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 78122_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 78122_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
Rejecting candidate due to large distance (31.0") between the two second-epoch detections
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Considering the candidate 19054_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 19054_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 137026_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 137026_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:43:26.54 +43:32:45.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213345_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 213345_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
Rejecting candidate due to large distance (32.4") between the two second-epoch detections
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Considering the candidate 52140_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 52140_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 81676_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 81676_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
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Considering the candidate 64687_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 64687_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 58994_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 58994_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 107628_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 107628_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 52992_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 52992_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 53491_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 53491_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 50152_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 50152_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 209862_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 209862_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:55:11.99 +46:44:16.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 0.325 254701804154714880 073.79990905963 +46.73805601507 14.2559 13.6304 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.325#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 66448_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 66448_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 208822_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 208822_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
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Considering the candidate 165825_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 165825_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:42:28.73 +41:32:33.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 70442_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 70442_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 68987_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 68987_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 68800_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 68800_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 70302_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 70302_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
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Considering the candidate 69610_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 69610_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 51790_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 51790_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 25749_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 25749_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:21:35.30 +49:37:16.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 69179_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 69179_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 52507_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 52507_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 21587_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 21587_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
Rejecting candidate due to large distance (32.0") between the two second-epoch detections
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Considering the candidate 54325_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 54325_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 62028_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 62028_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 64210_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 64210_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 55353_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 55353_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 108499_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 108499_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 67993_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 67993_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 100177_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 100177_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:51:14.03 +45:18:59.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53141_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 53141_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 104075_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 104075_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 66259_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 66259_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 55785_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 55785_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 66011_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 66011_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 102022_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 102022_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 143365_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 143365_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:41:48.92 +43:14:51.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100793_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 100793_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
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Considering the candidate 65274_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 65274_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 26689_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 26689_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:02:56.91 +49:18:56.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 146956_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 146956_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
Rejecting candidate due to large distance (32.2") between the two second-epoch detections
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Considering the candidate 73776_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 73776_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 56210_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 56210_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 67460_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 67460_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 43200_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 43200_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 05:10:56.93 +48:12:54.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 138372_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 138372_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:39:20.30 +43:29:31.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 128870_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 128870_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 05:11:02.28 +43:30:53.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55149_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 55149_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 64539_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 64539_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 54820_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 54820_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 70176_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 70176_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 65305_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 65305_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 63316_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 63316_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
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Considering the candidate 62695_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 62695_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
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Considering the candidate 156863_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 156863_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 05:09:44.56 +40:44:26.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 50811_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 50811_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 65495_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 65495_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 59241_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 59241_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 05:02:32.88 +47:27:38.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 58949_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 58949_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 93325_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 93325_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:52:33.44 +45:41:38.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 60402_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 60402_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 60707_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 60707_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 102423_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 102423_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
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Considering the candidate 71880_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 71880_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 34523_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 34523_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:53:24.09 +49:00:04.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 11204_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 11204_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
Rejecting candidate due to large distance (32.9") between the two second-epoch detections
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Considering the candidate 71768_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 71768_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
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Considering the candidate 55146_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 55146_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 58525_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 58525_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
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Considering the candidate 79546_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 79546_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
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Considering the candidate 170083_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 170083_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:27:32.45 +41:47:04.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 62828_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 62828_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
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Considering the candidate 59841_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 59841_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 50667_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 50667_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 63637_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 63637_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 116947_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 116947_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 70126_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 70126_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 57075_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 57075_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 65327_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 65327_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 58516_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 58516_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 60091_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 60091_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 60708_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 60708_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 65780_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 65780_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 54836_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 54836_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 62947_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 62947_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 51560_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 51560_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 72968_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 72968_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 63730_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 63730_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 98748_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 98748_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 05:02:48.46 +45:16:21.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 58773_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 58773_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 64836_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 64836_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 71155_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 71155_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 67793_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 67793_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 06844_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 06844_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 05:27:03.74 +50:07:26.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 59217_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 59217_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 66411_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 66411_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 55147_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 55147_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 62648_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 62648_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 69724_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 69724_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 131612_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 131612_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
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Considering the candidate 71432_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 71432_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 68366_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 68366_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 67814_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 67814_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 62369_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 62369_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 71191_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 71191_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 57483_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 57483_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 30259_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 30259_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 62723_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 62723_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 64226_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 64226_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 64760_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 64760_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 64406_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 64406_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 106055_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 106055_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:57:32.60 +44:55:12.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 74510_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 74510_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 61917_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 61917_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 75293_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 75293_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 64409_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 64409_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 67371_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 67371_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 62929_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 62929_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 50258_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 50258_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 05:18:55.92 +47:37:04.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 61503_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 61503_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
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Considering the candidate 71147_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 71147_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 72863_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 72863_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 58986_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 58986_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 64981_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 64981_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 05:03:12.43 +47:09:04.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193050_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 193050_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:23:13.92 +42:49:37.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 85966_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 85966_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:54:36.26 +46:04:42.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 49020_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 49020_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 62097_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 62097_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 66718_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 66718_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 72990_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 72990_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 27997_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 27997_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 65145_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 65145_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 108953_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 108953_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 64386_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 64386_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 114117_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 114117_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 134124_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 134124_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
Rejecting candidate due to large distance (35.2") between the two second-epoch detections
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Considering the candidate 72188_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 72188_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 64339_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 64339_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 145470_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 145470_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:40:30.15 +43:11:52.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 112461_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 112461_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 73609_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 73609_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 64757_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 64757_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 51848_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 51848_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 66916_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 66916_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 62404_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 62404_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 100279_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 100279_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 57076_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 57076_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 51715_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 51715_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19899_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 19899_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 66762_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 66762_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112393_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 112393_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115576_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 115576_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:55:42.03 +44:26:00.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55212_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 55212_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 73410_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 73410_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 05:04:11.73 +46:36:32.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 183613_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 183613_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:07:58.00 +42:13:23.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 65491_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 65491_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 66630_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 66630_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 63740_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 63740_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 60270_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 60270_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 95776_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 95776_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 04:32:36.72 +45:40:13.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53699_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 53699_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 69385_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 69385_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 89424_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 89424_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
**** FOUND 05:02:35.60 +45:45:36.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54535_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 54535_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 162399_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
The candidate 162399_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 108399_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 108399_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70052_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 70052_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 64571_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 64571_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 67289_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 67289_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 71858_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 71858_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 69055_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 69055_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
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Considering the candidate 65716_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 65716_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 48161_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 48161_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 63053_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 63053_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61007_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 61007_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52525_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 52525_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53164_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 53164_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 105114_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 105114_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62227_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 62227_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 65545_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 65545_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61771_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 61771_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 64992_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 64992_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 65635_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 65635_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 65541_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 65541_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 66721_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
Preparing report for the candidate 66721_fd_Per-03-Q1b1x1_2026-09-10_06-14-05_20.00sec_-0.00C_LIGHTs_0082
make_report_in_HTML.sh Phase 2 (HTML assembly): 14s
make_report_in_HTML.sh TOTAL: 292s
Prepared the HTML report for the field Per-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
04:58:05.82 +45:13:47.7
05:05:59.18 +45:00:01.5
05:00:01.28 +44:59:43.1
04:54:04.75 +45:00:58.7
04:55:34.54 +44:52:33.6
04:56:13.20 +44:48:36.1
04:57:24.94 +44:47:52.3
04:55:30.28 +44:47:41.5
04:56:07.52 +44:36:13.5
04:44:00.58 +44:43:02.7
04:58:26.03 +44:28:39.9
04:53:04.08 +44:24:10.2
05:10:08.50 +49:42:12.7
05:10:04.10 +49:37:57.4
04:58:05.50 +49:20:33.4
04:56:01.48 +49:13:39.8
04:56:25.51 +49:06:48.8
05:11:01.03 +47:55:42.9
05:08:06.46 +47:56:07.5
05:08:14.44 +47:52:20.8
05:09:53.78 +47:49:48.1
05:08:15.96 +47:49:49.6
05:09:33.17 +47:48:17.4
05:08:51.08 +47:46:01.6
05:08:47.02 +47:45:31.8
05:09:39.80 +47:44:34.2
05:09:56.19 +47:44:08.0
05:07:12.57 +47:47:06.6
05:08:16.90 +47:45:08.9
05:07:21.72 +47:44:26.5
05:08:05.72 +47:43:34.3
05:06:35.10 +47:44:23.7
05:07:30.93 +47:42:45.0
05:08:26.15 +47:41:25.7
05:06:33.48 +47:43:12.8
05:07:50.36 +47:40:37.3
05:05:58.56 +47:42:36.0
05:06:41.75 +47:41:11.2
05:07:20.73 +47:39:06.0
05:07:32.06 +47:38:09.1
05:05:25.05 +47:39:55.1
05:08:51.82 +47:35:29.6
05:07:51.14 +47:35:52.3
05:05:06.53 +47:40:24.4
05:07:49.48 +47:34:59.4
05:07:04.39 +47:35:51.3
05:08:10.13 +47:34:16.9
05:06:24.25 +47:36:18.3
05:07:53.70 +47:34:01.1
05:07:36.13 +47:32:31.7
05:07:16.82 +47:31:31.3
05:06:56.55 +47:28:49.4
05:03:35.71 +47:32:26.7
05:05:54.34 +47:28:38.5
05:03:05.15 +47:31:04.4
05:03:32.20 +47:28:10.9
05:03:20.09 +47:27:40.2
04:56:26.97 +47:33:55.1
05:07:27.57 +47:22:16.1
05:07:24.35 +47:21:45.7
05:01:43.58 +47:27:26.0
05:02:28.83 +47:27:00.5
05:01:40.77 +47:26:59.1
05:03:17.00 +47:23:38.5
05:02:26.99 +47:23:31.5
05:03:42.60 +47:22:22.7
05:02:41.78 +47:22:29.3
05:06:55.04 +47:17:28.4
05:03:22.77 +47:20:53.9
05:02:04.15 +47:22:05.2
05:03:39.46 +47:19:39.7
05:00:17.13 +47:22:52.0
05:02:51.56 +47:19:11.6
05:00:35.52 +47:20:09.5
05:02:56.42 +47:16:43.4
05:02:06.22 +47:16:50.1
05:02:40.21 +47:16:23.0
05:01:21.70 +47:17:11.4
05:03:35.81 +47:14:27.9
05:03:07.74 +47:14:56.0
05:02:09.26 +47:15:09.8
05:03:15.72 +47:14:12.5
05:01:51.69 +47:14:47.1
04:56:23.92 +47:18:55.6
05:02:02.16 +47:13:54.5
05:02:52.91 +47:12:46.8
05:01:07.78 +47:14:22.1
05:00:40.64 +47:14:42.2
05:00:43.60 +47:15:00.4
05:01:05.42 +47:12:02.0
05:01:48.06 +47:11:21.2
05:01:53.73 +47:11:13.2
04:55:58.38 +47:15:57.3
05:03:52.33 +47:10:05.6
05:03:32.51 +47:07:52.2
05:02:42.25 +47:08:20.3
05:00:15.82 +47:10:38.9
04:57:30.00 +47:12:41.8
05:01:42.54 +47:08:57.3
04:59:53.13 +47:10:21.7
05:01:46.05 +47:08:54.0
04:55:51.50 +47:13:07.2
04:56:14.86 +47:13:00.3
04:56:59.62 +47:12:09.9
05:02:21.07 +47:07:09.9
05:02:33.36 +47:07:05.8
05:02:50.50 +47:06:23.4
04:57:20.34 +47:11:17.2
05:00:37.93 +47:08:12.3
05:04:47.65 +47:03:41.5
04:56:26.45 +47:11:39.2
04:55:55.15 +47:11:21.2
05:01:33.81 +47:06:14.0
05:02:18.07 +47:05:10.0
05:02:44.56 +47:05:11.2
05:01:05.06 +47:06:23.0
04:56:13.66 +47:10:14.6
05:02:46.66 +47:04:27.5
05:03:16.97 +47:03:26.6
04:55:57.81 +47:09:53.3
04:56:02.49 +47:09:35.8
04:56:13.61 +47:09:40.9
05:03:32.97 +47:02:39.9
04:56:05.57 +47:09:05.4
04:56:58.66 +47:08:26.5
05:00:16.40 +47:05:20.2
05:03:00.75 +47:02:30.2
04:55:49.53 +47:07:21.4
05:04:02.10 +46:59:48.2
05:02:05.00 +47:01:49.7
05:02:45.01 +47:00:24.5
04:55:47.20 +47:06:08.1
05:02:55.19 +46:59:41.7
05:04:18.25 +46:58:31.5
05:03:31.56 +46:58:40.6
05:02:50.91 +46:59:30.1
04:56:05.00 +47:04:00.0
04:56:17.59 +47:03:46.5
04:55:35.82 +47:03:44.3
04:56:28.80 +47:02:13.9
04:56:02.69 +47:02:27.8
05:02:51.87 +46:56:09.2
05:03:31.64 +46:54:30.6
05:02:55.51 +46:54:22.0
05:01:38.46 +46:54:09.0
04:55:49.95 +46:58:38.6
05:02:09.96 +46:52:58.4
04:55:43.24 +46:57:55.0
04:56:02.20 +46:56:59.8
05:02:23.86 +46:50:36.2
04:55:49.40 +46:55:51.5
05:03:26.09 +46:48:24.6
05:04:07.93 +46:47:30.9
05:04:06.32 +46:47:17.2
04:55:40.99 +46:55:25.8
05:03:25.57 +46:47:07.9
04:55:55.61 +46:52:26.0
05:02:28.87 +46:45:41.4
05:03:18.46 +46:44:36.9
05:03:07.39 +46:44:39.5
05:03:57.68 +46:42:44.9
05:02:15.69 +46:43:26.4
05:04:37.02 +46:41:29.7
04:56:14.92 +46:48:03.1
05:02:19.62 +46:42:45.0
05:02:21.53 +46:39:45.6
05:02:13.92 +46:39:46.1
04:55:46.84 +46:45:13.0
05:03:09.38 +46:36:57.9
04:57:09.58 +46:41:30.8
05:03:01.45 +46:36:01.4
05:02:36.25 +46:36:48.7
05:04:18.48 +46:32:29.1
05:02:29.62 +46:31:43.3
05:02:43.61 +46:28:45.5
05:00:07.07 +45:23:30.6
########### Completed Per-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 ####
05:05:58.56 +47:42:36.0
05:01:05.42 +47:12:02.0
05:01:33.81 +47:06:14.0
05:03:17.00 +47:23:38.5
04:56:14.92 +46:48:03.1
04:57:09.58 +46:41:30.8
05:02:43.61 +46:28:45.5
05:00:07.07 +45:23:30.6
05:09:39.80 +47:44:34.2
04:55:55.61 +46:52:26.0
05:00:43.60 +47:15:00.4
05:01:48.06 +47:11:21.2
05:02:46.66 +47:04:27.5
05:06:35.10 +47:44:23.7
05:05:25.05 +47:39:55.1
05:03:31.56 +46:58:40.6
05:03:31.64 +46:54:30.6
04:56:59.62 +47:12:09.9
05:03:20.09 +47:27:40.2
04:56:25.51 +49:06:48.8
05:03:35.81 +47:14:27.9
05:07:20.73 +47:39:06.0
04:56:58.66 +47:08:26.5
05:00:35.52 +47:20:09.5
05:02:36.25 +46:36:48.7
05:03:05.15 +47:31:04.4
05:04:47.65 +47:03:41.5
05:02:02.16 +47:13:54.5
05:02:04.15 +47:22:05.2
05:01:46.05 +47:08:54.0
05:03:32.20 +47:28:10.9
05:09:53.78 +47:49:48.1
04:56:13.66 +47:10:14.6
05:03:42.60 +47:22:22.7
05:04:07.93 +46:47:30.9
05:02:21.07 +47:07:09.9
05:10:08.50 +49:42:12.7
05:08:16.90 +47:45:08.9
05:02:33.36 +47:07:05.8
05:02:28.83 +47:27:00.5
04:55:34.54 +44:52:33.6
05:07:30.93 +47:42:45.0
05:07:50.36 +47:40:37.3
05:08:14.44 +47:52:20.8
05:02:05.00 +47:01:49.7
05:03:25.57 +46:47:07.9
04:55:49.95 +46:58:38.6
05:01:38.46 +46:54:09.0
05:02:23.86 +46:50:36.2
05:09:56.19 +47:44:08.0
04:55:43.24 +46:57:55.0
05:07:21.72 +47:44:26.5
05:07:32.06 +47:38:09.1
05:02:40.21 +47:16:23.0
05:03:32.51 +47:07:52.2
05:07:53.70 +47:34:01.1
04:57:24.94 +44:47:52.3
05:02:51.87 +46:56:09.2
05:08:26.15 +47:41:25.7
05:00:01.28 +44:59:43.1
04:55:49.53 +47:07:21.4
05:07:36.13 +47:32:31.7
05:03:00.75 +47:02:30.2
05:05:59.18 +45:00:01.5
05:02:18.07 +47:05:10.0
05:03:01.45 +46:36:01.4
05:07:16.82 +47:31:31.3
04:55:35.82 +47:03:44.3
05:08:10.13 +47:34:16.9
04:55:51.50 +47:13:07.2
05:07:51.14 +47:35:52.3
04:55:40.99 +46:55:25.8
05:02:44.56 +47:05:11.2
05:09:33.17 +47:48:17.4
04:55:57.81 +47:09:53.3
05:07:24.35 +47:21:45.7
05:03:22.77 +47:20:53.9
05:03:39.46 +47:19:39.7
05:04:37.02 +46:41:29.7
05:07:49.48 +47:34:59.4
05:02:26.99 +47:23:31.5
05:08:15.96 +47:49:49.6
05:01:53.73 +47:11:13.2
04:53:04.08 +44:24:10.2
05:04:06.32 +46:47:17.2
05:06:56.55 +47:28:49.4
05:01:05.06 +47:06:23.0
04:56:26.97 +47:33:55.1
05:02:41.78 +47:22:29.3
05:00:17.13 +47:22:52.0
05:00:16.40 +47:05:20.2
05:05:06.53 +47:40:24.4
05:01:07.78 +47:14:22.1
05:08:51.08 +47:46:01.6
05:02:13.92 +46:39:46.1
04:55:58.38 +47:15:57.3
05:07:27.57 +47:22:16.1
05:00:37.93 +47:08:12.3
05:03:18.46 +46:44:36.9
04:56:28.80 +47:02:13.9
05:01:40.77 +47:26:59.1
05:04:02.10 +46:59:48.2
05:07:04.39 +47:35:51.3
05:01:51.69 +47:14:47.1
04:55:49.40 +46:55:51.5
05:03:57.68 +46:42:44.9
05:02:55.51 +46:54:22.0
04:56:02.69 +47:02:27.8
05:02:09.26 +47:15:09.8
05:03:07.39 +46:44:39.5
05:05:54.34 +47:28:38.5
04:56:01.48 +49:13:39.8
04:56:23.92 +47:18:55.6
05:02:42.25 +47:08:20.3
04:57:20.34 +47:11:17.2
05:01:42.54 +47:08:57.3
05:04:18.48 +46:32:29.1
05:02:06.22 +47:16:50.1
05:02:29.62 +46:31:43.3
04:59:53.13 +47:10:21.7
04:56:17.59 +47:03:46.5
05:02:52.91 +47:12:46.8
05:02:28.87 +46:45:41.4
05:02:21.53 +46:39:45.6
05:01:43.58 +47:27:26.0
05:08:06.46 +47:56:07.5
05:01:21.70 +47:17:11.4
04:55:47.20 +47:06:08.1
04:55:46.84 +46:45:13.0
04:58:05.50 +49:20:33.4
04:55:55.15 +47:11:21.2
04:55:30.28 +44:47:41.5
04:57:30.00 +47:12:41.8
04:58:26.03 +44:28:39.9
05:02:19.62 +46:42:45.0
05:00:15.82 +47:10:38.9
04:44:00.58 +44:43:02.7
05:03:09.38 +46:36:57.9
05:02:50.50 +47:06:23.4
05:07:12.57 +47:47:06.6
05:02:50.91 +46:59:30.1
05:03:15.72 +47:14:12.5
04:58:05.82 +45:13:47.7
05:03:35.71 +47:32:26.7
05:08:47.02 +47:45:31.8
05:10:04.10 +49:37:57.4
05:04:18.25 +46:58:31.5
04:56:07.52 +44:36:13.5
05:06:24.25 +47:36:18.3
05:03:16.97 +47:03:26.6
05:02:45.01 +47:00:24.5
05:03:52.33 +47:10:05.6
05:06:55.04 +47:17:28.4
05:06:41.75 +47:41:11.2
04:56:02.20 +46:56:59.8
05:08:51.82 +47:35:29.6
04:56:13.20 +44:48:36.1
05:03:26.09 +46:48:24.6
04:56:14.86 +47:13:00.3
04:56:05.00 +47:04:00.0
05:02:15.69 +46:43:26.4
05:02:09.96 +46:52:58.4
04:56:05.57 +47:09:05.4
05:11:01.03 +47:55:42.9
05:00:40.64 +47:14:42.2
05:02:51.56 +47:19:11.6
05:08:05.72 +47:43:34.3
05:06:33.48 +47:43:12.8
04:54:04.75 +45:00:58.7
05:03:07.74 +47:14:56.0
04:56:13.61 +47:09:40.9
05:02:56.42 +47:16:43.4
04:56:26.45 +47:11:39.2
05:03:32.97 +47:02:39.9
04:56:02.49 +47:09:35.8
05:02:55.19 +46:59:41.7
###################################################################################
05:05:58.56 +47:42:36.0 -- not an asteroid (will add it to exclusion list)
05:01:05.42 +47:12:02.0 -- not an asteroid (will add it to exclusion list)
05:01:33.81 +47:06:14.0 -- not an asteroid (will add it to exclusion list)
05:03:17.00 +47:23:38.5 -- not an asteroid (will add it to exclusion list)
04:56:14.92 +46:48:03.1 -- not an asteroid (will add it to exclusion list)
04:57:09.58 +46:41:30.8 -- not an asteroid (will add it to exclusion list)
05:02:43.61 +46:28:45.5 -- not an asteroid (will add it to exclusion list)
05:00:07.07 +45:23:30.6 -- not an asteroid (will add it to exclusion list)
05:09:39.80 +47:44:34.2 -- not an asteroid (will add it to exclusion list)
04:55:55.61 +46:52:26.0 -- not an asteroid (will add it to exclusion list)
05:00:43.60 +47:15:00.4 -- not an asteroid (will add it to exclusion list)
05:01:48.06 +47:11:21.2 -- not an asteroid (will add it to exclusion list)
05:02:46.66 +47:04:27.5 -- not an asteroid (will add it to exclusion list)
05:06:35.10 +47:44:23.7 -- not an asteroid (will add it to exclusion list)
05:05:25.05 +47:39:55.1 -- not an asteroid (will add it to exclusion list)
05:03:31.56 +46:58:40.6 -- not an asteroid (will add it to exclusion list)
05:03:31.64 +46:54:30.6 -- not an asteroid (will add it to exclusion list)
04:56:59.62 +47:12:09.9 -- not an asteroid (will add it to exclusion list)
05:03:20.09 +47:27:40.2 -- not an asteroid (will add it to exclusion list)
04:56:25.51 +49:06:48.8 -- not an asteroid (will add it to exclusion list)
05:03:35.81 +47:14:27.9 -- not an asteroid (will add it to exclusion list)
05:07:20.73 +47:39:06.0 -- not an asteroid (will add it to exclusion list)
04:56:58.66 +47:08:26.5 -- not an asteroid (will add it to exclusion list)
05:00:35.52 +47:20:09.5 -- not an asteroid (will add it to exclusion list)
05:02:36.25 +46:36:48.7 -- not an asteroid (will add it to exclusion list)
05:03:05.15 +47:31:04.4 -- not an asteroid (will add it to exclusion list)
05:04:47.65 +47:03:41.5 -- not an asteroid (will add it to exclusion list)
05:02:02.16 +47:13:54.5 -- not an asteroid (will add it to exclusion list)
05:02:04.15 +47:22:05.2 -- not an asteroid (will add it to exclusion list)
05:01:46.05 +47:08:54.0 -- not an asteroid (will add it to exclusion list)
05:03:32.20 +47:28:10.9 -- not an asteroid (will add it to exclusion list)
05:09:53.78 +47:49:48.1 -- not an asteroid (will add it to exclusion list)
04:56:13.66 +47:10:14.6 -- not an asteroid (will add it to exclusion list)
05:03:42.60 +47:22:22.7 -- not an asteroid (will add it to exclusion list)
05:04:07.93 +46:47:30.9 -- not an asteroid (will add it to exclusion list)
05:02:21.07 +47:07:09.9 -- not an asteroid (will add it to exclusion list)
05:10:08.50 +49:42:12.7 -- not an asteroid (will add it to exclusion list)
05:08:16.90 +47:45:08.9 -- not an asteroid (will add it to exclusion list)
05:02:33.36 +47:07:05.8 -- not an asteroid (will add it to exclusion list)
05:02:28.83 +47:27:00.5 -- not an asteroid (will add it to exclusion list)
04:55:34.54 +44:52:33.6 -- not an asteroid (will add it to exclusion list)
05:07:30.93 +47:42:45.0 -- not an asteroid (will add it to exclusion list)
05:07:50.36 +47:40:37.3 -- not an asteroid (will add it to exclusion list)
05:08:14.44 +47:52:20.8 -- not an asteroid (will add it to exclusion list)
05:02:05.00 +47:01:49.7 -- not an asteroid (will add it to exclusion list)
05:03:25.57 +46:47:07.9 -- not an asteroid (will add it to exclusion list)
04:55:49.95 +46:58:38.6 -- not an asteroid (will add it to exclusion list)
05:01:38.46 +46:54:09.0 -- not an asteroid (will add it to exclusion list)
05:02:23.86 +46:50:36.2 -- not an asteroid (will add it to exclusion list)
05:09:56.19 +47:44:08.0 -- not an asteroid (will add it to exclusion list)
04:55:43.24 +46:57:55.0 -- not an asteroid (will add it to exclusion list)
05:07:21.72 +47:44:26.5 -- not an asteroid (will add it to exclusion list)
05:07:32.06 +47:38:09.1 -- not an asteroid (will add it to exclusion list)
05:02:40.21 +47:16:23.0 -- not an asteroid (will add it to exclusion list)
05:03:32.51 +47:07:52.2 -- not an asteroid (will add it to exclusion list)
05:07:53.70 +47:34:01.1 -- not an asteroid (will add it to exclusion list)
04:57:24.94 +44:47:52.3 -- not an asteroid (will add it to exclusion list)
05:02:51.87 +46:56:09.2 -- not an asteroid (will add it to exclusion list)
05:08:26.15 +47:41:25.7 -- not an asteroid (will add it to exclusion list)
05:00:01.28 +44:59:43.1 -- not an asteroid (will add it to exclusion list)
04:55:49.53 +47:07:21.4 -- not an asteroid (will add it to exclusion list)
05:07:36.13 +47:32:31.7 -- not an asteroid (will add it to exclusion list)
05:03:00.75 +47:02:30.2 -- not an asteroid (will add it to exclusion list)
05:05:59.18 +45:00:01.5 -- not an asteroid (will add it to exclusion list)
05:02:18.07 +47:05:10.0 -- not an asteroid (will add it to exclusion list)
05:03:01.45 +46:36:01.4 -- not an asteroid (will add it to exclusion list)
05:07:16.82 +47:31:31.3 -- not an asteroid (will add it to exclusion list)
04:55:35.82 +47:03:44.3 -- not an asteroid (will add it to exclusion list)
05:08:10.13 +47:34:16.9 -- not an asteroid (will add it to exclusion list)
04:55:51.50 +47:13:07.2 -- not an asteroid (will add it to exclusion list)
05:07:51.14 +47:35:52.3 -- not an asteroid (will add it to exclusion list)
04:55:40.99 +46:55:25.8 -- not an asteroid (will add it to exclusion list)
05:02:44.56 +47:05:11.2 -- not an asteroid (will add it to exclusion list)
05:09:33.17 +47:48:17.4 -- not an asteroid (will add it to exclusion list)
04:55:57.81 +47:09:53.3 -- not an asteroid (will add it to exclusion list)
05:07:24.35 +47:21:45.7 -- not an asteroid (will add it to exclusion list)
05:03:22.77 +47:20:53.9 -- not an asteroid (will add it to exclusion list)
05:03:39.46 +47:19:39.7 -- not an asteroid (will add it to exclusion list)
05:04:37.02 +46:41:29.7 -- not an asteroid (will add it to exclusion list)
05:07:49.48 +47:34:59.4 -- not an asteroid (will add it to exclusion list)
05:02:26.99 +47:23:31.5 -- not an asteroid (will add it to exclusion list)
05:08:15.96 +47:49:49.6 -- not an asteroid (will add it to exclusion list)
05:01:53.73 +47:11:13.2 -- not an asteroid (will add it to exclusion list)
04:53:04.08 +44:24:10.2 -- not an asteroid (will add it to exclusion list)
05:04:06.32 +46:47:17.2 -- not an asteroid (will add it to exclusion list)
05:06:56.55 +47:28:49.4 -- not an asteroid (will add it to exclusion list)
05:01:05.06 +47:06:23.0 -- not an asteroid (will add it to exclusion list)
04:56:26.97 +47:33:55.1 -- not an asteroid (will add it to exclusion list)
05:02:41.78 +47:22:29.3 -- not an asteroid (will add it to exclusion list)
05:00:17.13 +47:22:52.0 -- not an asteroid (will add it to exclusion list)
05:00:16.40 +47:05:20.2 -- not an asteroid (will add it to exclusion list)
05:05:06.53 +47:40:24.4 -- not an asteroid (will add it to exclusion list)
05:01:07.78 +47:14:22.1 -- not an asteroid (will add it to exclusion list)
05:08:51.08 +47:46:01.6 -- not an asteroid (will add it to exclusion list)
05:02:13.92 +46:39:46.1 -- not an asteroid (will add it to exclusion list)
04:55:58.38 +47:15:57.3 -- not an asteroid (will add it to exclusion list)
05:07:27.57 +47:22:16.1 -- not an asteroid (will add it to exclusion list)
05:00:37.93 +47:08:12.3 -- not an asteroid (will add it to exclusion list)
05:03:18.46 +46:44:36.9 -- not an asteroid (will add it to exclusion list)
04:56:28.80 +47:02:13.9 -- not an asteroid (will add it to exclusion list)
05:01:40.77 +47:26:59.1 -- not an asteroid (will add it to exclusion list)
05:04:02.10 +46:59:48.2 -- not an asteroid (will add it to exclusion list)
05:07:04.39 +47:35:51.3 -- not an asteroid (will add it to exclusion list)
05:01:51.69 +47:14:47.1 -- not an asteroid (will add it to exclusion list)
04:55:49.40 +46:55:51.5 -- not an asteroid (will add it to exclusion list)
05:03:57.68 +46:42:44.9 -- not an asteroid (will add it to exclusion list)
05:02:55.51 +46:54:22.0 -- not an asteroid (will add it to exclusion list)
04:56:02.69 +47:02:27.8 -- not an asteroid (will add it to exclusion list)
05:02:09.26 +47:15:09.8 -- not an asteroid (will add it to exclusion list)
05:03:07.39 +46:44:39.5 -- not an asteroid (will add it to exclusion list)
05:05:54.34 +47:28:38.5 -- not an asteroid (will add it to exclusion list)
04:56:01.48 +49:13:39.8 -- not an asteroid (will add it to exclusion list)
04:56:23.92 +47:18:55.6 -- not an asteroid (will add it to exclusion list)
05:02:42.25 +47:08:20.3 -- not an asteroid (will add it to exclusion list)
04:57:20.34 +47:11:17.2 -- not an asteroid (will add it to exclusion list)
05:01:42.54 +47:08:57.3 -- not an asteroid (will add it to exclusion list)
05:04:18.48 +46:32:29.1 -- not an asteroid (will add it to exclusion list)
05:02:06.22 +47:16:50.1 -- not an asteroid (will add it to exclusion list)
05:02:29.62 +46:31:43.3 -- not an asteroid (will add it to exclusion list)
04:59:53.13 +47:10:21.7 -- not an asteroid (will add it to exclusion list)
04:56:17.59 +47:03:46.5 -- not an asteroid (will add it to exclusion list)
05:02:52.91 +47:12:46.8 -- not an asteroid (will add it to exclusion list)
05:02:28.87 +46:45:41.4 -- not an asteroid (will add it to exclusion list)
05:02:21.53 +46:39:45.6 -- not an asteroid (will add it to exclusion list)
05:01:43.58 +47:27:26.0 -- not an asteroid (will add it to exclusion list)
05:08:06.46 +47:56:07.5 -- not an asteroid (will add it to exclusion list)
05:01:21.70 +47:17:11.4 -- not an asteroid (will add it to exclusion list)
04:55:47.20 +47:06:08.1 -- not an asteroid (will add it to exclusion list)
04:55:46.84 +46:45:13.0 -- not an asteroid (will add it to exclusion list)
04:58:05.50 +49:20:33.4 -- not an asteroid (will add it to exclusion list)
04:55:55.15 +47:11:21.2 -- not an asteroid (will add it to exclusion list)
04:55:30.28 +44:47:41.5 -- not an asteroid (will add it to exclusion list)
04:57:30.00 +47:12:41.8 -- not an asteroid (will add it to exclusion list)
04:58:26.03 +44:28:39.9 -- not an asteroid (will add it to exclusion list)
05:02:19.62 +46:42:45.0 -- not an asteroid (will add it to exclusion list)
05:00:15.82 +47:10:38.9 -- not an asteroid (will add it to exclusion list)
04:44:00.58 +44:43:02.7 -- not an asteroid (will add it to exclusion list)
05:03:09.38 +46:36:57.9 -- not an asteroid (will add it to exclusion list)
05:02:50.50 +47:06:23.4 -- not an asteroid (will add it to exclusion list)
05:07:12.57 +47:47:06.6 -- not an asteroid (will add it to exclusion list)
05:02:50.91 +46:59:30.1 -- not an asteroid (will add it to exclusion list)
05:03:15.72 +47:14:12.5 -- not an asteroid (will add it to exclusion list)
04:58:05.82 +45:13:47.7 -- not an asteroid (will add it to exclusion list)
05:03:35.71 +47:32:26.7 -- not an asteroid (will add it to exclusion list)
05:08:47.02 +47:45:31.8 -- not an asteroid (will add it to exclusion list)
05:10:04.10 +49:37:57.4 -- not an asteroid (will add it to exclusion list)
05:04:18.25 +46:58:31.5 -- not an asteroid (will add it to exclusion list)
04:56:07.52 +44:36:13.5 -- not an asteroid (will add it to exclusion list)
05:06:24.25 +47:36:18.3 -- not an asteroid (will add it to exclusion list)
05:03:16.97 +47:03:26.6 -- not an asteroid (will add it to exclusion list)
05:02:45.01 +47:00:24.5 -- not an asteroid (will add it to exclusion list)
05:03:52.33 +47:10:05.6 -- not an asteroid (will add it to exclusion list)
05:06:55.04 +47:17:28.4 -- not an asteroid (will add it to exclusion list)
05:06:41.75 +47:41:11.2 -- not an asteroid (will add it to exclusion list)
04:56:02.20 +46:56:59.8 -- not an asteroid (will add it to exclusion list)
05:08:51.82 +47:35:29.6 -- not an asteroid (will add it to exclusion list)
04:56:13.20 +44:48:36.1 -- not an asteroid (will add it to exclusion list)
05:03:26.09 +46:48:24.6 -- not an asteroid (will add it to exclusion list)
04:56:14.86 +47:13:00.3 -- not an asteroid (will add it to exclusion list)
04:56:05.00 +47:04:00.0 -- not an asteroid (will add it to exclusion list)
05:02:15.69 +46:43:26.4 -- not an asteroid (will add it to exclusion list)
05:02:09.96 +46:52:58.4 -- not an asteroid (will add it to exclusion list)
04:56:05.57 +47:09:05.4 -- not an asteroid (will add it to exclusion list)
05:11:01.03 +47:55:42.9 -- not an asteroid (will add it to exclusion list)
05:00:40.64 +47:14:42.2 -- not an asteroid (will add it to exclusion list)
05:02:51.56 +47:19:11.6 -- not an asteroid (will add it to exclusion list)
05:08:05.72 +47:43:34.3 -- not an asteroid (will add it to exclusion list)
05:06:33.48 +47:43:12.8 -- not an asteroid (will add it to exclusion list)
04:54:04.75 +45:00:58.7 -- not an asteroid (will add it to exclusion list)
05:03:07.74 +47:14:56.0 -- not an asteroid (will add it to exclusion list)
04:56:13.61 +47:09:40.9 -- not an asteroid (will add it to exclusion list)
05:02:56.42 +47:16:43.4 -- not an asteroid (will add it to exclusion list)
04:56:26.45 +47:11:39.2 -- not an asteroid (will add it to exclusion list)
05:03:32.97 +47:02:39.9 -- not an asteroid (will add it to exclusion list)
04:56:02.49 +47:09:35.8 -- not an asteroid (will add it to exclusion list)
05:02:55.19 +46:59:41.7 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
04:44:00.58 +44:43:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:53:04.08 +44:24:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:54:04.75 +45:00:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:30.28 +44:47:41.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:34.54 +44:52:33.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:35.82 +47:03:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:40.99 +46:55:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:43.24 +46:57:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:46.84 +46:45:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:47.20 +47:06:08.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:49.40 +46:55:51.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:49.53 +47:07:21.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:49.95 +46:58:38.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:51.50 +47:13:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:55.15 +47:11:21.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:55.61 +46:52:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:57.81 +47:09:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:58.38 +47:15:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:01.48 +49:13:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:02.20 +46:56:59.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:02.49 +47:09:35.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:02.69 +47:02:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:05.00 +47:04:00.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:05.57 +47:09:05.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:07.52 +44:36:13.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:13.20 +44:48:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:13.61 +47:09:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:13.66 +47:10:14.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:14.86 +47:13:00.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:14.92 +46:48:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:17.59 +47:03:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:23.92 +47:18:55.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:25.51 +49:06:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:26.45 +47:11:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:26.97 +47:33:55.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:28.80 +47:02:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:58.66 +47:08:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:59.62 +47:12:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:09.58 +46:41:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:20.34 +47:11:17.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:24.94 +44:47:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:30.00 +47:12:41.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:05.50 +49:20:33.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:05.82 +45:13:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:26.03 +44:28:39.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:53.13 +47:10:21.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:00:01.28 +44:59:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:00:07.07 +45:23:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:00:15.82 +47:10:38.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:00:16.40 +47:05:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:00:17.13 +47:22:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:00:35.52 +47:20:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:00:37.93 +47:08:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:00:40.64 +47:14:42.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:00:43.60 +47:15:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:01:05.06 +47:06:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:01:05.42 +47:12:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:01:07.78 +47:14:22.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:01:21.70 +47:17:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:01:33.81 +47:06:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:01:38.46 +46:54:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:01:40.77 +47:26:59.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:01:42.54 +47:08:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:01:43.58 +47:27:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:01:46.05 +47:08:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:01:48.06 +47:11:21.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:01:51.69 +47:14:47.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:01:53.73 +47:11:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:02:02.16 +47:13:54.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:02:04.15 +47:22:05.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:02:05.00 +47:01:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:02:06.22 +47:16:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:02:09.26 +47:15:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:02:09.96 +46:52:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:02:13.92 +46:39:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:02:15.69 +46:43:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:02:18.07 +47:05:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:02:19.62 +46:42:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:02:21.07 +47:07:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:02:21.53 +46:39:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:02:23.86 +46:50:36.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:02:26.99 +47:23:31.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:02:28.83 +47:27:00.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:02:28.87 +46:45:41.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:02:29.62 +46:31:43.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:02:33.36 +47:07:05.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:02:36.25 +46:36:48.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:02:40.21 +47:16:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:02:41.78 +47:22:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:02:42.25 +47:08:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:02:43.61 +46:28:45.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:02:44.56 +47:05:11.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:02:45.01 +47:00:24.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:02:46.66 +47:04:27.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:02:50.50 +47:06:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:02:50.91 +46:59:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:02:51.56 +47:19:11.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:02:51.87 +46:56:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:02:52.91 +47:12:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:02:55.19 +46:59:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:02:55.51 +46:54:22.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:02:56.42 +47:16:43.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:03:00.75 +47:02:30.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:03:01.45 +46:36:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:03:05.15 +47:31:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:03:07.39 +46:44:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:03:07.74 +47:14:56.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:03:09.38 +46:36:57.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:03:15.72 +47:14:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:03:16.97 +47:03:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:03:17.00 +47:23:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:03:18.46 +46:44:36.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:03:20.09 +47:27:40.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:03:22.77 +47:20:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:03:25.57 +46:47:07.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:03:26.09 +46:48:24.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:03:31.56 +46:58:40.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:03:31.64 +46:54:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:03:32.20 +47:28:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:03:32.51 +47:07:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:03:32.97 +47:02:39.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:03:35.71 +47:32:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:03:35.81 +47:14:27.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:03:39.46 +47:19:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:03:42.60 +47:22:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:03:52.33 +47:10:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:03:57.68 +46:42:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:04:02.10 +46:59:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:04:06.32 +46:47:17.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:04:07.93 +46:47:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:04:18.25 +46:58:31.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:04:18.48 +46:32:29.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:04:37.02 +46:41:29.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:04:47.65 +47:03:41.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:05:06.53 +47:40:24.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:05:25.05 +47:39:55.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:05:54.34 +47:28:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:05:58.56 +47:42:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:05:59.18 +45:00:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:06:24.25 +47:36:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:06:33.48 +47:43:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:06:35.10 +47:44:23.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:06:41.75 +47:41:11.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:06:55.04 +47:17:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:06:56.55 +47:28:49.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:04.39 +47:35:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:12.57 +47:47:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:16.82 +47:31:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:20.73 +47:39:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:21.72 +47:44:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:24.35 +47:21:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:27.57 +47:22:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:30.93 +47:42:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:32.06 +47:38:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:36.13 +47:32:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:49.48 +47:34:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:50.36 +47:40:37.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:51.14 +47:35:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:53.70 +47:34:01.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:08:05.72 +47:43:34.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:08:06.46 +47:56:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:08:10.13 +47:34:16.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:08:14.44 +47:52:20.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:08:15.96 +47:49:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:08:16.90 +47:45:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:08:26.15 +47:41:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:08:47.02 +47:45:31.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:08:51.08 +47:46:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:08:51.82 +47:35:29.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:09:33.17 +47:48:17.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:09:39.80 +47:44:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:09:53.78 +47:49:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:09:56.19 +47:44:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:10:04.10 +49:37:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:10:08.50 +49:42:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:11:01.03 +47:55:42.9 -- 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)
04:44:00.58 +44:43:02.7 -- a known variable star
04:53:04.08 +44:24:10.2 -- a known variable star
04:54:04.75 +45:00:58.7 -- not a known variable star
04:55:30.28 +44:47:41.5 -- not a known variable star
04:55:34.54 +44:52:33.6 -- a known variable star
04:55:35.82 +47:03:44.3 -- not a known variable star
04:55:40.99 +46:55:25.8 -- not a known variable star
04:55:43.24 +46:57:55.0 -- not a known variable star
04:55:46.84 +46:45:13.0 -- not a known variable star
04:55:47.20 +47:06:08.1 -- not a known variable star
04:55:49.40 +46:55:51.5 -- not a known variable star
04:55:49.53 +47:07:21.4 -- not a known variable star
04:55:49.95 +46:58:38.6 -- not a known variable star
04:55:51.50 +47:13:07.2 -- a known variable star
04:55:55.15 +47:11:21.2 -- not a known variable star
04:55:55.61 +46:52:26.0 -- not a known variable star
04:55:57.81 +47:09:53.3 -- a known variable star
04:55:58.38 +47:15:57.3 -- not a known variable star
04:56:01.48 +49:13:39.8 -- not a known variable star
04:56:02.20 +46:56:59.8 -- not a known variable star
04:56:02.49 +47:09:35.8 -- not a known variable star
04:56:02.69 +47:02:27.8 -- not a known variable star
04:56:05.00 +47:04:00.0 -- not a known variable star
04:56:05.57 +47:09:05.4 -- not a known variable star
04:56:07.52 +44:36:13.5 -- not a known variable star
04:56:13.20 +44:48:36.1 -- not a known variable star
04:56:13.61 +47:09:40.9 -- not a known variable star
04:56:13.66 +47:10:14.6 -- not a known variable star
04:56:14.86 +47:13:00.3 -- not a known variable star
04:56:14.92 +46:48:03.1 -- not a known variable star
04:56:17.59 +47:03:46.5 -- not a known variable star
04:56:23.92 +47:18:55.6 -- not a known variable star
04:56:25.51 +49:06:48.8 -- not a known variable star
04:56:26.45 +47:11:39.2 -- not a known variable star
04:56:26.97 +47:33:55.1 -- not a known variable star
04:56:28.80 +47:02:13.9 -- not a known variable star
04:56:58.66 +47:08:26.5 -- not a known variable star
04:56:59.62 +47:12:09.9 -- a known variable star
04:57:09.58 +46:41:30.8 -- not a known variable star
04:57:20.34 +47:11:17.2 -- not a known variable star
04:57:24.94 +44:47:52.3 -- a known variable star
04:57:30.00 +47:12:41.8 -- a known variable star
04:58:05.50 +49:20:33.4 -- a known variable star
04:58:05.82 +45:13:47.7 -- not a known variable star
04:58:26.03 +44:28:39.9 -- not a known variable star
04:59:53.13 +47:10:21.7 -- not a known variable star
05:00:01.28 +44:59:43.1 -- a known variable star
05:00:07.07 +45:23:30.6 -- not a known variable star
05:00:15.82 +47:10:38.9 -- not a known variable star
05:00:16.40 +47:05:20.2 -- not a known variable star
05:00:17.13 +47:22:52.0 -- not a known variable star
05:00:35.52 +47:20:09.5 -- a known variable star
05:00:37.93 +47:08:12.3 -- not a known variable star
05:00:40.64 +47:14:42.2 -- not a known variable star
05:00:43.60 +47:15:00.4 -- a known variable star
05:01:05.06 +47:06:23.0 -- not a known variable star
05:01:05.42 +47:12:02.0 -- not a known variable star
05:01:07.78 +47:14:22.1 -- not a known variable star
05:01:21.70 +47:17:11.4 -- not a known variable star
05:01:33.81 +47:06:14.0 -- not a known variable star
05:01:38.46 +46:54:09.0 -- not a known variable star
05:01:40.77 +47:26:59.1 -- not a known variable star
05:01:42.54 +47:08:57.3 -- not a known variable star
05:01:43.58 +47:27:26.0 -- not a known variable star
05:01:46.05 +47:08:54.0 -- not a known variable star
05:01:48.06 +47:11:21.2 -- not a known variable star
05:01:51.69 +47:14:47.1 -- not a known variable star
05:01:53.73 +47:11:13.2 -- not a known variable star
05:02:02.16 +47:13:54.5 -- not a known variable star
05:02:04.15 +47:22:05.2 -- not a known variable star
05:02:05.00 +47:01:49.7 -- not a known variable star
05:02:06.22 +47:16:50.1 -- not a known variable star
05:02:09.26 +47:15:09.8 -- not a known variable star
05:02:09.96 +46:52:58.4 -- not a known variable star
05:02:13.92 +46:39:46.1 -- not a known variable star
05:02:15.69 +46:43:26.4 -- a known variable star
05:02:18.07 +47:05:10.0 -- a known variable star
05:02:19.62 +46:42:45.0 -- not a known variable star
05:02:21.07 +47:07:09.9 -- not a known variable star
05:02:21.53 +46:39:45.6 -- not a known variable star
05:02:23.86 +46:50:36.2 -- not a known variable star
05:02:26.99 +47:23:31.5 -- not a known variable star
05:02:28.83 +47:27:00.5 -- not a known variable star
05:02:28.87 +46:45:41.4 -- not a known variable star
05:02:29.62 +46:31:43.3 -- not a known variable star
05:02:33.36 +47:07:05.8 -- not a known variable star
05:02:36.25 +46:36:48.7 -- not a known variable star
05:02:40.21 +47:16:23.0 -- not a known variable star
05:02:41.78 +47:22:29.3 -- a known variable star
05:02:42.25 +47:08:20.3 -- not a known variable star
05:02:43.61 +46:28:45.5 -- not a known variable star
05:02:44.56 +47:05:11.2 -- not a known variable star
05:02:45.01 +47:00:24.5 -- not a known variable star
05:02:46.66 +47:04:27.5 -- not a known variable star
05:02:50.50 +47:06:23.4 -- not a known variable star
05:02:50.91 +46:59:30.1 -- not a known variable star
05:02:51.56 +47:19:11.6 -- not a known variable star
05:02:51.87 +46:56:09.2 -- a known variable star
05:02:52.91 +47:12:46.8 -- not a known variable star
05:02:55.19 +46:59:41.7 -- not a known variable star
05:02:55.51 +46:54:22.0 -- not a known variable star
05:02:56.42 +47:16:43.4 -- not a known variable star
05:03:00.75 +47:02:30.2 -- not a known variable star
05:03:01.45 +46:36:01.4 -- a known variable star
05:03:05.15 +47:31:04.4 -- not a known variable star
05:03:07.39 +46:44:39.5 -- a known variable star
05:03:07.74 +47:14:56.0 -- not a known variable star
05:03:09.38 +46:36:57.9 -- not a known variable star
05:03:15.72 +47:14:12.5 -- not a known variable star
05:03:16.97 +47:03:26.6 -- a known variable star
05:03:17.00 +47:23:38.5 -- not a known variable star
05:03:18.46 +46:44:36.9 -- not a known variable star
05:03:20.09 +47:27:40.2 -- not a known variable star
05:03:22.77 +47:20:53.9 -- not a known variable star
05:03:25.57 +46:47:07.9 -- not a known variable star
05:03:26.09 +46:48:24.6 -- not a known variable star
05:03:31.56 +46:58:40.6 -- not a known variable star
05:03:31.64 +46:54:30.6 -- not a known variable star
05:03:32.20 +47:28:10.9 -- not a known variable star
05:03:32.51 +47:07:52.2 -- not a known variable star
05:03:32.97 +47:02:39.9 -- not a known variable star
05:03:35.71 +47:32:26.7 -- a known variable star
05:03:35.81 +47:14:27.9 -- not a known variable star
05:03:39.46 +47:19:39.7 -- not a known variable star
05:03:42.60 +47:22:22.7 -- not a known variable star
05:03:52.33 +47:10:05.6 -- not a known variable star
05:03:57.68 +46:42:44.9 -- not a known variable star
05:04:02.10 +46:59:48.2 -- not a known variable star
05:04:06.32 +46:47:17.2 -- a known variable star
05:04:07.93 +46:47:30.9 -- a known variable star
05:04:18.25 +46:58:31.5 -- not a known variable star
05:04:18.48 +46:32:29.1 -- a known variable star
05:04:37.02 +46:41:29.7 -- a known variable star
05:04:47.65 +47:03:41.5 -- not a known variable star
05:05:06.53 +47:40:24.4 -- a known variable star
05:05:25.05 +47:39:55.1 -- not a known variable star
05:05:54.34 +47:28:38.5 -- not a known variable star
05:05:58.56 +47:42:36.0 -- not a known variable star
05:05:59.18 +45:00:01.5 -- a known variable star
05:06:24.25 +47:36:18.3 -- a known variable star
05:06:33.48 +47:43:12.8 -- not a known variable star
05:06:35.10 +47:44:23.7 -- not a known variable star
05:06:41.75 +47:41:11.2 -- not a known variable star
05:06:55.04 +47:17:28.4 -- not a known variable star
05:06:56.55 +47:28:49.4 -- not a known variable star
05:07:04.39 +47:35:51.3 -- not a known variable star
05:07:12.57 +47:47:06.6 -- not a known variable star
05:07:16.82 +47:31:31.3 -- not a known variable star
05:07:20.73 +47:39:06.0 -- not a known variable star
05:07:21.72 +47:44:26.5 -- not a known variable star
05:07:24.35 +47:21:45.7 -- not a known variable star
05:07:27.57 +47:22:16.1 -- not a known variable star
05:07:30.93 +47:42:45.0 -- not a known variable star
05:07:32.06 +47:38:09.1 -- not a known variable star
05:07:36.13 +47:32:31.7 -- not a known variable star
05:07:49.48 +47:34:59.4 -- not a known variable star
05:07:50.36 +47:40:37.3 -- not a known variable star
05:07:51.14 +47:35:52.3 -- not a known variable star
05:07:53.70 +47:34:01.1 -- not a known variable star
05:08:05.72 +47:43:34.3 -- not a known variable star
05:08:06.46 +47:56:07.5 -- not a known variable star
05:08:10.13 +47:34:16.9 -- not a known variable star
05:08:14.44 +47:52:20.8 -- not a known variable star
05:08:15.96 +47:49:49.6 -- not a known variable star
05:08:16.90 +47:45:08.9 -- not a known variable star
05:08:26.15 +47:41:25.7 -- not a known variable star
05:08:47.02 +47:45:31.8 -- not a known variable star
05:08:51.08 +47:46:01.6 -- not a known variable star
05:08:51.82 +47:35:29.6 -- not a known variable star
05:09:33.17 +47:48:17.4 -- not a known variable star
05:09:39.80 +47:44:34.2 -- not a known variable star
05:09:53.78 +47:49:48.1 -- not a known variable star
05:09:56.19 +47:44:08.0 -- not a known variable star
05:10:04.10 +49:37:57.4 -- not a known variable star
05:10:08.50 +49:42:12.7 -- not a known variable star
05:11:01.03 +47:55:42.9 -- not a known variable star
Found 149 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
176 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 176 (excluding asteroids and hot pixels, 149 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)2461293.96764399 -observatory V36
11:58:30.52 +00:59:19.7 Mercury (-0.7mag)
13:43:47.37 -15:41:07.7 Venus (-4.7mag)
07:22:30.69 +22:46:04.3 Mars (1.2mag)
09:11:38.71 +16:46:32.1 Jupiter (-1.8mag)
00:50:58.99 +02:33:21.1 Saturn (0.4mag)
04:13:42.59 +21:02:03.2 Uranus (5.7mag)
00:13:26.61 -00:05:16.1 Neptune (7.7mag)
20:25:22.86 -23:40:18.8 Pluto (14.5mag)
10:43:13.91 +06:57:47.5 Moon (99.9mag)
-rw-r--r-- 1 apache apache 362 Sep 10 06:15 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461293.96764399:
09:11:46.07 +16:45:56.1 Io (6.2mag)
09:11:40.92 +16:46:22.2 Europa (6.3mag)
09:11:27.40 +16:47:30.9 Ganymede (5.7mag)
09:11:39.64 +16:46:29.5 Callisto (6.9mag)
09:09:31.75 +17:04:25.0 Himalia (15.7mag)
09:11:38.62 +16:46:32.8 Thebe (16.6mag)
09:09:06.83 +16:58:18.3 Elara (17.7mag)
09:15:27.57 +16:13:11.7 Pasiphae (17.9mag)
09:12:29.95 +17:05:11.2 Carme (19.0mag)
00:50:44.88 +02:33:25.6 Titan (8.3mag)
00:50:57.69 +02:33:25.7 Rhea (9.6mag)
00:51:05.40 +02:35:32.0 Iapetus (11.0mag)
00:51:13.65 +02:33:15.4 Hyperion (14.3mag)
00:49:42.49 +02:22:47.9 Phoebe (16.4mag)
-rw-r--r-- 1 apache apache 568 Sep 10 06:15 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461293.96764399:
22:29:19.24 +04:14:16.1 JWST
18:35:03.28 +17:19:01.7 Chandra
07:02:22.03 -03:38:07.3 XMM-Newton
-rw-r--r-- 1 apache apache 96 Sep 10 06:15 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461293.96764399 -observatory V36
03:42:11.97 +19:28:54.6 17.3mag P/1996 R2 (Lagerkvist)
18:04:06.75 -34:09:06.1 14.4mag P/2010 H2 (Vales)
07:21:50.13 -70:28:44.7 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:16:01.68 +33:46:59.5 17.7mag C/2017 K2 (PANSTARRS)
22:10:58.95 +28:16:39.2 17.5mag C/2022 E2 (ATLAS)
07:12:33.23 +25:55:14.4 16.9mag C/2022 N2 (PANSTARRS)
10:52:25.03 +27:06:51.2 17.1mag C/2022 QE78 (ATLAS)
09:50:40.51 +05:12:55.6 18.0mag C/2022 R6 (PANSTARRS)
15:28:45.08 -15:55:37.7 14.9mag C/2023 R1 (PANSTARRS)
08:41:07.84 +33:05:30.7 15.8mag C/2024 E1 (Wierzchos)
15:07:01.81 +15:17:12.0 17.9mag C/2024 G6 (ATLAS)
18:31:43.62 +43:02:52.4 13.7mag C/2024 J3 (ATLAS)
20:21:53.86 +49:07:10.2 17.4mag C/2024 R4 (PANSTARRS)
05:37:14.73 -13:04:17.9 15.1mag C/2024 T5 (ATLAS)
07:12:40.07 +17:54:17.6 17.8mag C/2025 J1 (Borisov)
11:23:07.10 +18:31:14.2 16.8mag C/2025 V2 (Rankin)
13:22:15.76 -00:08:26.1 16.8mag C/2025 Y1 (ATLAS)
16:49:59.28 +73:29:50.0 16.0mag C/2026 A2 (Bok)
03:04:06.86 +46:01:31.3 17.5mag C/2026 B2 (Sun-Gao)
12:16:13.19 +11:32:32.3 17.5mag A/2026 E1
22:28:37.85 -35:11:57.6 13.5mag 10P/Tempel
01:24:25.95 +37:39:25.0 17.8mag 11P/Tempel-Swift-LINEAR
11:50:17.98 -05:42:27.4 16.3mag 29P/Schwassmann-Wachmann
12:14:57.46 -06:05:42.2 17.7mag 63P/Wild
06:45:24.46 +19:00:16.5 13.7mag 78P/Gehrels
03:17:18.49 +15:01:47.4 17.2mag 88P/Howell
05:48:49.76 +29:50:13.7 16.9mag 112P/Urata-Niijima
07:41:08.76 +23:59:19.3 15.9mag 114P/Wiseman-Skiff
10:34:57.34 +20:11:30.0 14.8mag 123P/West-Hartley
12:53:36.98 -22:26:14.4 17.5mag 124P/Mrkos
06:21:12.47 +20:32:19.3 15.9mag 128P/Shoemaker-Holt
02:18:48.14 -17:10:43.5 14.9mag 161P/Hartley-IRAS
09:01:46.49 +37:28:15.3 16.4mag 162P/Siding Spring
09:33:19.72 +11:52:10.3 13.2mag 169P/NEAT
03:26:55.51 +08:12:11.9 14.5mag 220P/McNaught
04:56:32.70 +37:18:00.3 15.2mag 260P/McNaught
08:40:19.49 +35:21:27.8 17.3mag 295P/LINEAR
15:27:19.78 -00:36:15.9 17.9mag 391P/Kowalski
09:30:30.73 +16:41:19.0 17.8mag 450P/LONEOS
-rw-r--r-- 1 apache apache 2.0K Sep 10 06:15 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
19:45:06.20 +18:22:48.80 V488 2026-08-30.13 9.37
18:25:12.74 -22:25:28.60 V8055 2026-08-30.22 10.89
17:17:45.96 +64:31:40.10 ASASSN-26ez 2026-08-25.13 10.87
19:02:47.09 +58:08:21.00 AT2026zwo 2026-08-24.16 15.78
04:20:07.58 -42:26:59.90 AT2026zjy 2026-08-23.03 15.91
03:08:18.02 +11:54:46.50 SN2026ymb 2026-08-23.4 16.44
20:22:32.48 -50:45:14.30 SN2026yid 2026-08-22.82 15.13
04:24:28.39 -56:20:21.60 ASASSN-26ey 2026-08-20.02 15.55
16:46:37.81 -63:14:59.80 ASASSN-26ex 2026-08-18.78 3.63
21:28:47.85 +20:31:03.60 SN 2026sfn 2026-08-16.3 17.09
23:01:28.67 -61:00:39.00 SN 2026yib 2026-08-14.85 17.36
00:22:23.20 -32:16:02.70 SN 2026whu 2026-08-14.96 16.5
19:56:21.71 -37:24:19.90 ASASSN-26ew 2026-08-13.82 14.73
13:53:14.21 +00:26:52.00 SN 2026wkv 2026-08-10.12 15.83
05:21:07.61 +23:38:20.10 TCP J05210763+2338194 2026-08-10.59 9.34
01:28:20.49 +40:13:27.10 SN2026wpd 2026-08-9.34 16.37
23:47:50.89 +49:28:51.30 SN2026wjs 2026-08-9.24 17.09
16:03:20.92 +17:43:23.70 AT2026xau 2026-08-9.3 17.71
01:10:22.05 -09:34:08.50 SN2026weo 2026-08-7.46 15.76
00:56:54.35 -35:55:29.40 AT2026wdy 2026-08-5.05 16.08
22:08:07.63 -53:03:58.90 AT2026wek 2026-08-3.82 17.17
14:51:51.34 +66:13:24.60 ASASSN-26ev 2026-08-2.15 14.02
12:06:50.79 -36:16:06.20 SN2026wgm 2026-08-1.73 15.61
16:56:36.90 -59:29:26.00 ASASSN-26er 2026-07-25.82 15.09
01:21:27.83 -10:37:05.00 SN2026vbh 2026-07-25.61 15.97
21:17:31.59 +22:25:50.90 ASASSN-26eq 2026-07-24.37 15.13
18:53:36.89 +16:56:43.60 ASASSN-26ep 2026-07-23.47 -4.06
12:18:47.98 -30:48:47.50 ASASSN-26et 2026-07-22.76 13.98
13:00:47.82 +15:42:17.60 SN2026uwk 2026-07-21.75 16.38
18:52:31.11 -32:28:00.90 ASASSN-26en 2026-07-21.77 14.63
14:42:58.01 -62:32:59.10 ASASSN-26es 2026-07-20.79 15.36
20:12:45.57 -32:53:13.00 ASASSN-26em 2026-07-20.94 16.83
18:54:24.33 -46:11:51.70 ASASSN-26eu 2026-07-20.93 14.86
03:18:56.99 -80:55:10.40 AT2026ugi 2026-07-20.03 17.12
18:43:58.40 +24:22:41.80 ASASSN-26eo 2026-07-19.36 16.16
04:50:01.03 -02:22:33.80 ASASSN-26ej 2026-07-16.17 17.02
18:34:55.28 -31:41:00.90 ASASSN-26ek 2026-07-16.24 15.73
17:07:43.61 -44:21:53.50 ASASSN-26el 2026-07-15.86 16.01
14:45:08.35 +24:13:12.30 ASASSN-26ei 2026-07-16.17 16.46
10:00:46.44 -32:36:31.10 AT 2023mhb 2026-07-14.73 16.67
14:39:37.45 -11:22:36.20 AT 2026unl 2026-07-15.27 17.11
10:49:42.57 -11:25:55.80 ASASSN-26eh 2026-07-14.72 16.58
19:33:53.06 -07:15:00.80 ASASSN-22le 2026-07-14.15 15.5
02:45:40.52 -27:55:30.30 ASASSN-26ef 2026-07-12.35 15.86
23:26:43.80 +04:42:39.70 SN 2026qtn 2026-07-12.22 16.47
02:19:17.26 +28:57:15.40 ASASSN-26ec 2026-07-11.53 2.78
18:31:15.56 -05:34:31.50 AT2026stb 2026-07-11.28 -1.29
13:36:08.24 +23:29:05.00 AT2026pjf 2026-07-10.18 -0.72
17:33:39.82 +04:22:36.70 SN2026pir 2026-07-9.86 -0.66
11:21:41.26 -50:33:36.30 ASASSN-26ed 2026-07-8.8 -1.3
23:41:42.11 +26:29:49.10 AT2026qil 2026-07-9.3 16.15
20:21:30.50 -32:03:40.10 ASASSN-26ee 2026-07-7.22 15.53
19:37:44.09 -05:35:42.80 AT2026ryu 2026-07-7.17 14.88
11:06:55.46 -04:07:04.50 AT2026qqg 2026-07-5.01 16.82
19:07:23.69 -74:13:37.30 AT2026qly 2026-07-5.02 17.31
17:57:43.80 +27:18:40.10 ASASSN-26ea 2026-07-5.07 16.67
19:59:01.43 -32:07:34.30 ASASSN-26eb 2026-07-4.97 15.52
18:46:50.35 -57:44:13.20 SN 2026qqp 2026-07-5.03 -0.92
19:17:31.69 -39:55:29.90 ASASSN-26dz 2026-07-5.14 15.91
19:14:31.37 +12:03:52.90 AT 2026rdg 2026-07-3.43 11.81
04:05:50.09 -70:24:34.40 AT 2026qpr 2026-06-30.4 15.96
13:45:37.49 -05:59:35.80 SN 2026pub 2026-06-30.09 16.01
16:41:15.63 +39:17:14.70 SN 2026pel 2026-06-26.38 16.07
10:14:40.19 -35:38:21.30 ASASSN-26dy 2026-06-25.99 15.63
14:47:21.56 -40:15:51.30 ASASSN-26dv 2026-06-23.03 14.62
13:38:49.79 -77:21:06.70 ASASSN-26dw 2026-06-23.04 16.09
00:59:27.90 +33:08:13.20 SN 2026mke 2026-06-22.39 17.13
11:10:44.73 -30:20:45.50 SN 2026nmv 2026-06-22.06 16.56
21:36:15.68 -21:19:12.50 AT2026oxh 2026-06-22.15 17.14
17:31:38.38 -56:05:51.90 ASASSN-26dx 2026-06-22.02 14.72
14:10:13.44 -38:46:46.10 AT2026pvk 2026-06-22.06 16.53
20:56:47.23 -18:31:05.20 AT2026plb 2026-06-21.31 16.4
15:44:29.68 +21:00:59.30 SN2026ore 2026-06-21.29 17.57
23:50:05.98 -14:01:41.30 AT2026oxl 2026-06-21.52 17.64
17:36:54.73 -18:10:04.20 AT2026ouj 2026-06-20.92 15.15
00:34:04.08 -30:22:09.20 AT2026ntk 2026-06-18.09 17.34
20:49:13.39 +25:17:59.20 ASASSN-26du 2026-06-15.39 15.93
23:09:30.84 +32:40:42.00 SN2026oxc 2026-06-14.35 16.83
02:02:26.78 +32:04:21.30 AT2026ovz 2026-06-14.59 15.39
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:33.11 -68:48:32.90 ASASSN-26no 2026-05-24.03 8.35
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.59 -58:37:47.40 ASASSN-26dn 2026-05-20.01 14.59
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
-rw-r--r-- 1 apache apache 5.7K Sep 10 06:15 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
00:44:56.43 +41:57:41.6 PNV J00445643+4157416 2026-07-13.8026 17.98Cmag
00:42:55.36 +41:17:27.0 PNV J00425536+4117270 2026-07-20.1813 17.7mag
20:35:43.64 +61:31:32.9 TCP J20354364+6131329 2026-07-20.5443 14.4mag
21:17:31.48 +22:25:51.0 TCP J21173148+2225510 2026-07-23.5577 14.8mag
00:41:24.04 +40:49:02.8 PNV J00412404+4049028 2026-07-25.0157 18.7mag
00:43:04.26 +41:02:28.6 PNV J00430426+4102286 2026-07-26.1512 20mag
14:51:51.40 +66:13:24.0 TCP J14515140+6613240 2026-07-29.2561 13.5mag
00:43:06.15 +41:22:08.2 PNV J00430615+4122082 2026-07-30.0085 19.4mag
00:41:33.23 +41:10:12.2 PNV J00413323+4110122 2026-08-02.8913 17.1mag
05:21:07.63 +23:38:19.4 TCP J05210763+2338194 2026-08-06.4109 11.2mag
22:57:17.96 +47:07:41.8 TCP J22571796+4707418 2026-08-09.3289 14.3mag
09:13:38.17 +76:28:18.1 PSN J09133817+7628181 2026-08-09.8037 15.4mag
00:43:17.29 +41:26:48.6 PNV J00431729+4126486 2026-08-14.0920 16.8mag
00:42:52.82 +41:10:58.6 PNV J00425282+4110586 2026-08-17.7723 19.9mag
00:42:52.83 +41:10:59.6 PNV J00425283+4110596 2026-08-18.6119 19.3mag
18:25:12.76 -22:25:29.3 TCP J18251276-2225293 2026-08-19.1062 9.4mag
18:03:09.04 +12:18:14.0 TCP J18030904+1218140 2026-08-19.5199 14.9mag
19:45:06.48 +18:22:42.2 PNV J19450648+1822422 2026-08-25.1278 9.0mag
00:42:54.65 +41:22:59.3 PNV J00425465+4122593 2026-08-25.4712 18.9mag
00:42:50.38 +41:18:58.76 PNV J00425038+4118587 2026-09-04.1512 18.2mag
-rw-r--r-- 1 apache apache 190K Sep 10 06:15 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
14:52:44.979 +53:35:27.83 AT 2026yxt 2026-08-05.18 20.8609
00:56:58.931 +27:08:48.44 SN 2026yxs 2026-08-15.06 19.27
20:48:19.872 +12:39:21.21 AT 2026yxr 2026-08-14.95 19.84
20:41:35.957 -01:18:45.35 AT 2026yxq 2026-08-13.46 18.76
17:37:53.890 +29:59:34.82 AT 2026yxp 2026-08-09.34 19.71
03:09:25.134 -42:47:32.92 AT 2026yxo 2026-08-14.06 19.072
02:37:44.043 +40:27:03.94 AT 2026yxn 2026-08-04.59 18.578
05:19:33.597 +03:36:27.44 AT 2026yxm 2026-08-08.49 19.2775
14:07:42.574 -42:50:59.33 AT 2026yxl 2026-08-01.76 19.154
17:33:41.970 +47:31:32.02 AT 2026yxk 2026-08-13.32 19.3
01:00:56.278 +39:19:38.93 AT 2026yxj 2026-08-12.14 19.374
18:33:47.958 +33:41:57.46 TDE 2026yxi 2026-08-13.37 19.405
20:18:57.682 -57:26:56.68 AT 2026yxh 2026-08-13.91 19.279
16:55:55.783 +16:34:53.69 AT 2026yxg 2026-08-08.33 19.2
02:35:11.630 +31:31:51.19 AT 2026yxf 2026-08-11.14 19.013
23:29:52.284 +44:53:18.83 AT 2026yxe 2026-08-12.10 20.038
15:42:53.416 -23:39:31.36 AT 2026yxd 2026-08-11.27 18.614
14:30:47.853 +24:42:11.36 AT 2026yxc 2026-08-14.26 20.32
17:42:05.972 +65:39:19.45 AT 2026yxb 2026-08-14.32 19.566
18:29:10.333 +08:12:57.93 AT 2026yxa 2026-08-04.21 17.5357
-rw-r--r-- 1 apache apache 88K Sep 10 06:15 tns_transients_list.txt
