This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Tau-03-Q1b1x1_051136_TTUQ1b1x1_635740_EPMM3l3i
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 04 11 31.68 +20 56 25.5 7.9 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461258.9235,7.89,0.05,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
VARIABLE_NAME 20260806.4235 7.89CV 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 04 11 31.70 +20 56 26.3 7.8 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461258.9235,7.77,0.05,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
VARIABLE_NAME 20260806.4235 7.77CV 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 08 06.4235 2461258.9235 10.89 04:08:24.73 +26:55:28.9
168.22865 -18.15354 galactic Tau Second-epoch detections are separated by 0.9" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 162669485452619648 | 04:08:24.79 +26:55:29.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 1968AbaOB..38...93M [M69] +26 36 J-Ks=0.422+/-0.029 (G)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:08:24.73 +26:55:28.9: 11.88 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:08:24.73 +26:55:28.9: 11.82 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.85 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 04 08 24.73 +26 55 28.9 10.9 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 162669485452619648,2461258.9235,10.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 162669485452619648 20260806.4235 10.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 11.09 04:57:05.43 +16:49:52.6
183.89786 -15.99634 galactic Tau Second-epoch detections are separated by 2.5" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3405604878964493440 | 04:57:05.38 +16:49:53.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.912+/-0.032 (M)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:57:05.43 +16:49:52.6: 11.90 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:57:05.43 +16:49:52.6: 11.93 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.91 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 04 57 05.43 +16 49 52.6 11.1 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3405604878964493440,2461258.9235,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3405604878964493440 20260806.4235 11.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 10.94 04:07:26.43 +26:48:49.6
168.15042 -18.38535 galactic Tau Second-epoch detections are separated by 1.5" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 162664262772436480 | 04:07:26.46 +26:48:50.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 1968AbaOB..38...93M [M69] +26 11 J-Ks=0.393+/-0.033 (G)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:07:26.43 +26:48:49.6: 11.97 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:07:26.43 +26:48:49.6: 11.97 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.97 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 04 07 26.43 +26 48 49.6 10.9 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 162664262772436480,2461258.9235,10.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 162664262772436480 20260806.4235 10.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 10.90 04:05:57.40 +26:14:11.4
168.33365 -19.02823 galactic Tau Second-epoch detections are separated by 1.0" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J061.5005+26.2425 | 04:05:57.39 +26:14:10.9 (Gaia DR3) | NSINE (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5) J-Ks=0.442+/-0.030 (G)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:05:57.40 +26:14:11.4: 11.99 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:05:57.40 +26:14:11.4: 11.90 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.94 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 04 05 57.40 +26 14 11.4 10.9 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J061.5005+26.2425,2461258.9235,10.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J061.5005+26.2425 20260806.4235 10.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 11.20 04:59:49.11 +17:12:39.3
183.97020 -15.24498 galactic Tau Second-epoch detections are separated by 0.7" and 5.5 pix
The object was found in VSX 1" ASASSN-V J045949.13+171238.5
Type: SR
# Max. Min./Amp. JD0 Period
12.780 V 12.950 V 2457388.00000 812.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:59:49.11 +17:12:39.3: 12.40 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:59:49.11 +17:12:39.3: 12.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.40 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 04 59 49.11 +17 12 39.3 11.2 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J045949.13+171238.5,2461258.9235,11.20,0.05,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
ASASSN-V J045949.13+171238.5 20260806.4235 11.20CV 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 08 06.4235 2461258.9235 11.44 05:04:44.76 +16:45:37.9
185.05213 -14.53957 galactic Tau Second-epoch detections are separated by 1.4" 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 | Gaia DR3 3394944774432402688 | 05:04:44.71 +16:45:40.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.257+/-0.028 (F)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:04:44.76 +16:45:37.9: 12.61 +/- 0.02 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:04:44.76 +16:45:37.9: 12.62 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 04 44.76 +16 45 37.9 11.4 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3394944774432402688,2461258.9235,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3394944774432402688 20260806.4235 11.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 11.39 05:05:25.76 +17:02:41.8
184.90705 -14.24315 galactic Tau Second-epoch detections are separated by 2.8" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3394967241405115008 | 05:05:25.79 +17:02:42.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.679+/-0.031 (K)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:05:25.76 +17:02:41.8: 12.72 +/- 0.02 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:05:25.76 +17:02:41.8: 12.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 05 25.76 +17 02 41.8 11.4 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3394967241405115008,2461258.9235,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3394967241405115008 20260806.4235 11.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 11.46 05:05:39.01 +17:34:55.7
184.48321 -13.89339 galactic Tau Second-epoch detections are separated by 2.7" 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 J076.4128+17.5819 | 05:05:39.08 +17:34:55.0 (Gaia DR3) | LPV (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.988+/-0.032 (M)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:05:39.01 +17:34:55.7: 12.74 +/- 0.02 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:05:39.01 +17:34:55.7: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 05 39.01 +17 34 55.7 11.5 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J076.4128+17.5819,2461258.9235,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J076.4128+17.5819 20260806.4235 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 11.54 05:05:54.99 +18:21:10.6
183.86988 -13.40052 galactic Tau Second-epoch detections are separated by 0.7" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J076.4794+18.3527 | 05:05:55.07 +18:21:09.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.206+/-0.031 (M)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:05:54.99 +18:21:10.6: 12.92 +/- 0.02 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:05:54.99 +18:21:10.6: 12.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 05 54.99 +18 21 10.6 11.5 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J076.4794+18.3527,2461258.9235,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J076.4794+18.3527 20260806.4235 11.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 11.64 05:04:44.43 +17:37:32.2
184.31872 -14.04635 galactic Tau Second-epoch detections are separated by 3.4" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3407030052192677888 | 05:04:44.50 +17:37:35.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:04:44.43 +17:37:32.2: 12.81 +/- 0.02 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:04:44.43 +17:37:32.2: 12.86 +/- 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!
TCP 2026 08 06.4235* 05 04 44.43 +17 37 32.2 11.6 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3407030052192677888,2461258.9235,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3407030052192677888 20260806.4235 11.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 11.61 05:05:10.71 +17:02:33.0
184.87386 -14.29380 galactic Tau Second-epoch detections are separated by 3.7" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:05:10.71 +17:02:33.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:05:10.71 +17:02:33.0: 12.80 +/- 0.02 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:05:10.71 +17:02:33.0: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 05 10.71 +17 02 33.0 11.6 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.9235,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.4235 11.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 11.69 05:06:25.23 +17:37:24.5
184.55611 -13.71906 galactic Tau Second-epoch detections are separated by 1.9" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:06:25.23 +17:37:24.5 (user input) | T | P | (position from user input) J-Ks=0.440+/-0.035 (G)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:06:25.23 +17:37:24.5: 12.78 +/- 0.02 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:06:25.23 +17:37:24.5: 12.89 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 06 25.23 +17 37 24.5 11.7 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.9235,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.4235 11.69CV 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 08 06.4235 2461258.9235 11.55 05:04:25.20 +17:27:34.5
184.41395 -14.20406 galactic Tau Second-epoch detections are separated by 1.1" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:04:25.20 +17:27:34.5 (user input) | T | P | (position from user input) J-Ks=0.462+/-0.028 (G)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:04:25.20 +17:27:34.5: 12.75 +/- 0.02 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:04:25.20 +17:27:34.5: 12.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 04 25.20 +17 27 34.5 11.6 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.9235,11.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.4235 11.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 11.52 05:07:42.11 +17:55:57.8
184.47333 -13.29220 galactic Tau Second-epoch detections are separated by 4.4" and 5.1 pix
The object was found in VSX21" ZTF J050742.14+175618.6
Type: EW
# Max. Min./Amp. JD0 Period
16.175 r Y 0.243 r 2458431.82360 0.342540400000
ATTENTION: measured mag 11.52 is 4.4 mag brighter than the VSX record maximum brightness 15.93 - 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_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:07:42.11 +17:55:57.8: 12.73 +/- 0.02 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:07:42.11 +17:55:57.8: 12.86 +/- 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!
TCP 2026 08 06.4235* 05 07 42.11 +17 55 57.8 11.5 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J050742.14+175618.6,2461258.9235,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J050742.14+175618.6 20260806.4235 11.52CV 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 08 06.4235 2461258.9235 11.43 05:07:23.50 +18:28:28.8
183.97287 -13.04387 galactic Tau Second-epoch detections are separated by 1.1" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3407229995806714880 | 05:07:23.47 +18:28:28.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.487+/-0.028 (K)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:07:23.50 +18:28:28.8: 12.68 +/- 0.02 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:07:23.50 +18:28:28.8: 12.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 07 23.50 +18 28 28.8 11.4 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3407229995806714880,2461258.9235,11.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3407229995806714880 20260806.4235 11.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 11.44 05:07:37.96 +18:28:57.6
183.99960 -12.99238 galactic Tau Second-epoch detections are separated by 3.8" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3407230614281992832 | 05:07:38.08 +18:28:58.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.522+/-0.028 (K)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:07:37.96 +18:28:57.6: 12.67 +/- 0.02 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:07:37.96 +18:28:57.6: 12.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 07 37.96 +18 28 57.6 11.4 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3407230614281992832,2461258.9235,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3407230614281992832 20260806.4235 11.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 11.60 05:05:52.83 +17:35:02.8
184.51383 -13.84720 galactic Tau Second-epoch detections are separated by 1.2" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3407020740703582592 | 05:05:52.85 +17:35:01.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.842+/-0.033 (M)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:05:52.83 +17:35:02.8: 12.65 +/- 0.02 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:05:52.83 +17:35:02.8: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 05 52.83 +17 35 02.8 11.6 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3407020740703582592,2461258.9235,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3407020740703582592 20260806.4235 11.60CV 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 08 06.4235 2461258.9235 11.48 05:05:10.24 +17:41:24.1
184.32474 -13.92545 galactic Tau Second-epoch detections are separated by 6.8" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3407036443104012160 | 05:05:10.34 +17:41:25.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.840+/-0.035 (M)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:05:10.24 +17:41:24.1: 12.66 +/- 0.02 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:05:10.24 +17:41:24.1: 12.71 +/- 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!
TCP 2026 08 06.4235* 05 05 10.24 +17 41 24.1 11.5 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3407036443104012160,2461258.9235,11.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3407036443104012160 20260806.4235 11.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 11.44 05:07:17.86 +18:06:50.3
184.26403 -13.26796 galactic Tau 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 | Gaia DR3 3407167083126073856 | 05:07:17.93 +18:06:48.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.850+/-0.026 (M)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:07:17.86 +18:06:50.3: 12.64 +/- 0.02 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:07:17.86 +18:06:50.3: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 07 17.86 +18 06 50.3 11.4 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3407167083126073856,2461258.9235,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3407167083126073856 20260806.4235 11.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 11.45 05:08:03.36 +18:50:51.6
183.75087 -12.70174 galactic Tau Second-epoch detections are separated by 6.6" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3407621112708804224 | 05:08:03.29 +18:50:49.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.458+/-0.028 (G)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:08:03.36 +18:50:51.6: 12.60 +/- 0.02 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:08:03.36 +18:50:51.6: 12.63 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 08 03.36 +18 50 51.6 11.4 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3407621112708804224,2461258.9235,11.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3407621112708804224 20260806.4235 11.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 11.55 05:05:22.97 +16:57:24.9
184.97516 -14.30245 galactic Tau Second-epoch detections are separated by 1.2" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3394954566957781504 | 05:05:23.00 +16:57:24.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.720+/-0.034 (K)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:05:22.97 +16:57:24.9: 12.57 +/- 0.02 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:05:22.97 +16:57:24.9: 12.62 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.59 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 05 22.97 +16 57 24.9 11.6 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3394954566957781504,2461258.9235,11.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3394954566957781504 20260806.4235 11.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 11.35 05:06:14.68 +17:31:19.2
184.61736 -13.81133 galactic Tau Second-epoch detections are separated by 4.1" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3407019331954312832 | 05:06:14.73 +17:31:20.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.883+/-0.033 (M)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:06:14.68 +17:31:19.2: 12.58 +/- 0.02 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:06:14.68 +17:31:19.2: 12.63 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 06 14.68 +17 31 19.2 11.3 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3407019331954312832,2461258.9235,11.35,0.05,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 3407019331954312832 20260806.4235 11.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 11.44 05:06:42.45 +17:51:46.3
184.39385 -13.52642 galactic Tau Second-epoch detections are separated by 2.1" and 5.0 pix
The object was found in VSX14" ZTF J050643.39+175141.9
Type: BY
# Max. Min./Amp. JD0 Period
16.171 r Y 0.112 r 2458338.97850 0.752099500000
ATTENTION: measured mag 11.44 is 4.6 mag brighter than the VSX record maximum brightness 16.06 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:06:42.45 +17:51:46.3: 12.55 +/- 0.02 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:06:42.45 +17:51:46.3: 12.59 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 06 42.45 +17 51 46.3 11.4 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J050643.39+175141.9,2461258.9235,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J050643.39+175141.9 20260806.4235 11.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 11.18 05:03:21.97 +18:10:46.7
183.65772 -13.99561 galactic Tau Second-epoch detections are separated by 2.1" and 5.4 pix
The object was found in VSX 2" ASASSN-V J050322.06+181044.8
Type: L
# Max. Min./Amp. JD0 Period
12.820 V 13.220 V
The object was not found in astcheck.
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:03:21.97 +18:10:46.7: 12.55 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:03:21.97 +18:10:46.7: 12.56 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 03 21.97 +18 10 46.7 11.2 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J050322.06+181044.8,2461258.9235,11.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J050322.06+181044.8 20260806.4235 11.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 11.46 05:06:06.35 +18:15:50.1
183.97136 -13.41466 galactic Tau Second-epoch detections are separated by 0.3" and 5.4 pix
The object was found in VSX 1" Gaia DR3 3407197250976135168
Type: ROT
# Max. Min./Amp. JD0 Period
12.290 G 12.320 G F
The object was not found in astcheck.
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:06:06.35 +18:15:50.1: 12.53 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:06:06.35 +18:15:50.1: 12.57 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 06 06.35 +18 15 50.1 11.5 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3407197250976135168,2461258.9235,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3407197250976135168 20260806.4235 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 11.39 05:06:39.38 +18:44:55.1
183.63991 -13.03012 galactic Tau Second-epoch detections are separated by 1.1" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3407253222990618240 | 05:06:39.42 +18:44:55.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.633+/-0.028 (K)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:06:39.38 +18:44:55.1: 12.51 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:06:39.38 +18:44:55.1: 12.57 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.54 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 06 39.38 +18 44 55.1 11.4 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3407253222990618240,2461258.9235,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3407253222990618240 20260806.4235 11.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 11.41 05:07:16.09 +17:15:32.3
184.98312 -13.76013 galactic Tau Second-epoch detections are separated by 3.3" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3394986207980680704 | 05:07:16.11 +17:15:31.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.414+/-0.031 (G)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:07:16.09 +17:15:32.3: 12.47 +/- 0.02 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:07:16.09 +17:15:32.3: 12.51 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 07 16.09 +17 15 32.3 11.4 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3394986207980680704,2461258.9235,11.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3394986207980680704 20260806.4235 11.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 11.36 05:08:25.09 +18:28:18.9
184.11757 -12.84546 galactic Tau Second-epoch detections are separated by 1.1" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3407558195731454720 | 05:08:25.13 +18:28:19.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.688+/-0.028 (K)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:08:25.09 +18:28:18.9: 12.47 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:08:25.09 +18:28:18.9: 12.47 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.47 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 08 25.09 +18 28 18.9 11.4 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3407558195731454720,2461258.9235,11.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3407558195731454720 20260806.4235 11.36CV 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 08 06.4235 2461258.9235 11.40 05:07:34.57 +18:24:25.0
184.05559 -13.04659 galactic Tau Second-epoch detections are separated by 3.3" 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 | Gaia DR3 3407181784796895744 | 05:07:34.43 +18:24:23.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.392+/-0.028 (G)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:07:34.57 +18:24:25.0: 12.48 +/- 0.02 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:07:34.57 +18:24:25.0: 12.52 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.50 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 07 34.57 +18 24 25.0 11.4 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3407181784796895744,2461258.9235,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3407181784796895744 20260806.4235 11.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 11.36 05:08:32.93 +17:56:17.4
184.58632 -13.12334 galactic Tau Second-epoch detections are separated by 1.9" 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 | Gaia DR3 3395140517566043008 | 05:08:32.82 +17:56:17.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.392+/-0.028 (G)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:08:32.93 +17:56:17.4: 12.44 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:08:32.93 +17:56:17.4: 12.49 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.46 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 08 32.93 +17 56 17.4 11.4 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3395140517566043008,2461258.9235,11.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3395140517566043008 20260806.4235 11.36CV 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 08 06.4235 2461258.9235 11.40 05:07:36.51 +17:12:16.7
185.07664 -13.72403 galactic Tau Second-epoch detections are separated by 6.3" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1852 Carpenter -546 -215 586 17.3 0 0
ATTENTION: measured mag 11.40 is 5.9 mag brighter than the predicted asteroid brightness 17.3 - the transient may be an unrelated new object!
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:07:36.51 +17:12:16.7: 12.44 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:07:36.51 +17:12:16.7: 12.45 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.44 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 07 36.51 +17 12 16.7 11.4 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461258.9235,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260806.4235 11.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 11.26 05:04:36.57 +17:41:17.5
184.24741 -14.03607 galactic Tau Second-epoch detections are separated by 0.9" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3407033561182447872 | 05:04:36.62 +17:41:16.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.039+/-0.024 (M)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:04:36.57 +17:41:17.5: 12.40 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:04:36.57 +17:41:17.5: 12.46 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.42 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 04 36.57 +17 41 17.5 11.3 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3407033561182447872,2461258.9235,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3407033561182447872 20260806.4235 11.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 11.21 05:05:38.60 +18:03:20.8
184.08221 -13.62389 galactic Tau Second-epoch detections are separated by 2.1" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J076.4193+18.0611 | 05:05:38.61 +18:03:20.7 (Gaia DR3) | MSINE (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.324+/-0.028 (G)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:05:38.60 +18:03:20.8: 12.38 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:05:38.60 +18:03:20.8: 12.41 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.40 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 05 38.60 +18 03 20.8 11.2 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J076.4193+18.0611,2461258.9235,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J076.4193+18.0611 20260806.4235 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 11.28 05:07:30.80 +17:43:25.2
184.62384 -13.44801 galactic Tau Second-epoch detections are separated by 2.1" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3395112827912516992 | 05:07:30.86 +17:43:24.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.873+/-0.031 (M)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:07:30.80 +17:43:25.2: 12.38 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:07:30.80 +17:43:25.2: 12.46 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.41 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 07 30.80 +17 43 25.2 11.3 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3395112827912516992,2461258.9235,11.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3395112827912516992 20260806.4235 11.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 11.28 05:07:44.01 +17:59:50.8
184.42305 -13.24918 galactic Tau Second-epoch detections are separated by 2.4" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J076.9280+17.9983 | 05:07:43.98 +17:59:52.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.399+/-0.028 (G)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:07:44.01 +17:59:50.8: 12.39 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:07:44.01 +17:59:50.8: 12.44 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.41 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 07 44.01 +17 59 50.8 11.3 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J076.9280+17.9983,2461258.9235,11.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J076.9280+17.9983 20260806.4235 11.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 11.36 04:58:47.51 +17:15:40.3
183.78028 -15.41549 galactic Tau Second-epoch detections are separated by 2.6" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3405717441468243840 | 04:58:47.56 +17:15:38.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.005+/-0.027 (M)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:58:47.51 +17:15:40.3: 12.35 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:58:47.51 +17:15:40.3: 12.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 04 58 47.51 +17 15 40.3 11.4 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3405717441468243840,2461258.9235,11.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3405717441468243840 20260806.4235 11.36CV 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 08 06.4235 2461258.9235 11.43 05:07:38.23 +17:41:53.3
184.66267 -13.43826 galactic Tau Second-epoch detections are separated by 2.3" 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 J076.9047+17.6991 | 05:07:38.24 +17:41:54.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.372+/-0.032 (G)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:07:38.23 +17:41:53.3: 12.36 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:07:38.23 +17:41:53.3: 12.46 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.40 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 07 38.23 +17 41 53.3 11.4 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J076.9047+17.6991,2461258.9235,11.43,0.05,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 J076.9047+17.6991 20260806.4235 11.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 11.17 05:07:03.49 +17:50:22.8
184.46236 -13.47108 galactic Tau Second-epoch detections are separated by 2.3" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3407124236532387200 | 05:07:03.53 +17:50:23.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.930+/-0.036 (M)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:07:03.49 +17:50:22.8: 12.35 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:07:03.49 +17:50:22.8: 12.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.37 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 07 03.49 +17 50 22.8 11.2 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3407124236532387200,2461258.9235,11.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3407124236532387200 20260806.4235 11.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 11.25 05:07:04.50 +16:52:06.8
185.28735 -14.01961 galactic Tau Second-epoch detections are separated by 1.0" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3394923673256835584 | 05:07:04.54 +16:52:06.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.692+/-0.035 (K)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:07:04.50 +16:52:06.8: 12.34 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:07:04.50 +16:52:06.8: 12.35 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.34 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 07 04.50 +16 52 06.8 11.2 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3394923673256835584,2461258.9235,11.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3394923673256835584 20260806.4235 11.25CV 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 08 06.4235 2461258.9235 11.37 05:08:15.06 +18:48:06.5
183.81647 -12.69002 galactic Tau Second-epoch detections are separated by 1.1" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3407619940181315456 | 05:08:15.01 +18:48:08.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:08:15.06 +18:48:06.5: 12.37 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:08:15.06 +18:48:06.5: 12.47 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.41 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 08 15.06 +18 48 06.5 11.4 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3407619940181315456,2461258.9235,11.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3407619940181315456 20260806.4235 11.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 11.36 05:00:13.17 +17:02:18.0
184.17356 -15.26670 galactic Tau Second-epoch detections are separated by 0.7" and 5.3 pix
The object was found in VSX 1" Gaia DR3 3405512043247968384
Type: L
# Max. Min./Amp. JD0 Period
11.610 G 11.720 G M
The object was not found in astcheck.
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:00:13.17 +17:02:18.0: 12.34 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:00:13.17 +17:02:18.0: 12.44 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 00 13.17 +17 02 18.0 11.4 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3405512043247968384,2461258.9235,11.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3405512043247968384 20260806.4235 11.36CV 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 08 06.4235 2461258.9235 11.15 04:06:04.77 +26:18:32.1
168.30015 -18.95753 galactic Tau Second-epoch detections are separated by 2.0" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 162622275172299520 | 04:06:04.74 +26:18:33.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.689+/-0.033 (K)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:06:04.77 +26:18:32.1: 12.33 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:06:04.77 +26:18:32.1: 12.26 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.30 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 04 06 04.77 +26 18 32.1 11.2 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 162622275172299520,2461258.9235,11.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 162622275172299520 20260806.4235 11.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 11.30 05:06:49.89 +18:41:49.4
183.70769 -13.02566 galactic Tau Second-epoch detections are separated by 0.5" and 5.2 pix
The object was found in VSX 2" Gaia DR3 3407249340339390464
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.230 G 12.250 G B
The object was not found in astcheck.
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:06:49.89 +18:41:49.4: 12.35 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:06:49.89 +18:41:49.4: 12.41 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 06 49.89 +18 41 49.4 11.3 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3407249340339390464,2461258.9235,11.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3407249340339390464 20260806.4235 11.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 11.27 05:08:40.49 +18:12:30.9
184.37531 -12.94513 galactic Tau Second-epoch detections are separated by 5.9" 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 | Gaia DR3 3407160000722783744 | 05:08:40.60 +18:12:31.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.764+/-0.028 (K)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:08:40.49 +18:12:30.9: 12.33 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:08:40.49 +18:12:30.9: 12.41 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.36 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 08 40.49 +18 12 30.9 11.3 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3407160000722783744,2461258.9235,11.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3407160000722783744 20260806.4235 11.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 11.19 05:06:29.28 +17:36:00.8
184.58522 -13.71909 galactic Tau Second-epoch detections are separated by 3.9" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3407113928610931840 | 05:06:29.40 +17:36:00.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5) J-Ks=0.870+/-0.034 (M)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:06:29.28 +17:36:00.8: 12.27 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:06:29.28 +17:36:00.8: 12.28 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.27 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 06 29.28 +17 36 00.8 11.2 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3407113928610931840,2461258.9235,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3407113928610931840 20260806.4235 11.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 11.25 05:07:27.65 +16:45:16.0
185.43818 -14.00814 galactic Tau Second-epoch detections are separated by 0.3" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3394886152421905664 | 05:07:27.67 +16:45:15.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.802+/-0.030 (K)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:07:27.65 +16:45:16.0: 12.25 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:07:27.65 +16:45:16.0: 12.31 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.28 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 07 27.65 +16 45 16.0 11.2 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3394886152421905664,2461258.9235,11.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3394886152421905664 20260806.4235 11.25CV 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 08 06.4235 2461258.9235 11.24 05:08:03.47 +18:37:56.0
183.93254 -12.82431 galactic Tau Second-epoch detections are separated by 2.5" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3407608223510513536 | 05:08:03.46 +18:37:55.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.726+/-0.026 (K)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:08:03.47 +18:37:56.0: 12.24 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:08:03.47 +18:37:56.0: 12.31 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.27 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 08 03.47 +18 37 56.0 11.2 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3407608223510513536,2461258.9235,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3407608223510513536 20260806.4235 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 11.07 05:08:15.80 +18:23:08.6
184.16882 -12.92472 galactic Tau Second-epoch detections are separated by 0.7" 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 | Gaia DR3 3407179345255472768 | 05:08:15.84 +18:23:08.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.736+/-0.027 (K)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:08:15.80 +18:23:08.6: 12.24 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:08:15.80 +18:23:08.6: 12.27 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.25 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 08 15.80 +18 23 08.6 11.1 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3407179345255472768,2461258.9235,11.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3407179345255472768 20260806.4235 11.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 11.25 05:06:55.48 +19:00:36.6
183.45730 -12.82826 galactic Tau Second-epoch detections are separated by 1.8" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3407821391328101760 | 05:06:55.43 +19:00:36.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.465+/-0.026 (K)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:06:55.48 +19:00:36.6: 12.23 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:06:55.48 +19:00:36.6: 12.26 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.24 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 06 55.48 +19 00 36.6 11.2 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3407821391328101760,2461258.9235,11.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3407821391328101760 20260806.4235 11.25CV 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 08 06.4235 2461258.9235 11.26 05:01:58.83 +17:40:37.9
183.88505 -14.55467 galactic Tau Second-epoch detections are separated by 0.7" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3407074273176889344 | 05:01:58.83 +17:40:38.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.070+/-0.027 (M)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:01:58.83 +17:40:37.9: 12.21 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:01:58.83 +17:40:37.9: 12.26 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.23 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 01 58.83 +17 40 37.9 11.3 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3407074273176889344,2461258.9235,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3407074273176889344 20260806.4235 11.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 10.98 05:06:57.08 +18:23:58.6
183.97489 -13.17246 galactic Tau Second-epoch detections are separated by 1.0" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3407223467456450432 | 05:06:57.10 +18:23:58.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.919+/-0.028 (M)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:06:57.08 +18:23:58.6: 12.19 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:06:57.08 +18:23:58.6: 12.23 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.21 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 06 57.08 +18 23 58.6 11.0 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3407223467456450432,2461258.9235,10.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3407223467456450432 20260806.4235 10.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 11.10 04:06:45.31 +26:35:53.1
168.19726 -18.64608 galactic Tau Second-epoch detections are separated by 3.1" 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 | Gaia DR3 162633098489804032 | 04:06:45.39 +26:35:53.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.426+/-0.034 (G)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:06:45.31 +26:35:53.1: 12.19 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:06:45.31 +26:35:53.1: 12.14 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.17 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 04 06 45.31 +26 35 53.1 11.1 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 162633098489804032,2461258.9235,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 162633098489804032 20260806.4235 11.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 11.06 05:07:08.36 +18:09:25.8
184.20553 -13.27424 galactic Tau Second-epoch detections are separated by 1.0" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3407168178344128896 | 05:07:08.37 +18:09:27.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.728+/-0.027 (K)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:07:08.36 +18:09:25.8: 12.20 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:07:08.36 +18:09:25.8: 12.28 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.23 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 07 08.36 +18 09 25.8 11.1 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3407168178344128896,2461258.9235,11.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3407168178344128896 20260806.4235 11.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 11.08 04:05:19.66 +26:28:43.7
168.04725 -18.95591 galactic Tau Second-epoch detections are separated by 1.4" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 162640039156809088 | 04:05:19.68 +26:28:43.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5) J-Ks=0.484+/-0.033 (K)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:05:19.66 +26:28:43.7: 12.18 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:05:19.66 +26:28:43.7: 12.10 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.14 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 04 05 19.66 +26 28 43.7 11.1 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 162640039156809088,2461258.9235,11.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 162640039156809088 20260806.4235 11.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 11.11 05:08:13.73 +17:55:50.1
184.54835 -13.19030 galactic Tau Second-epoch detections are separated by 0.8" 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 J077.0574+17.9305 | 05:08:13.80 +17:55:49.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: M3 (LAMOST DR5) J-Ks=1.119+/-0.039 (M)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:08:13.73 +17:55:50.1: 12.18 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:08:13.73 +17:55:50.1: 12.26 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.21 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 08 13.73 +17 55 50.1 11.1 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J077.0574+17.9305,2461258.9235,11.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J077.0574+17.9305 20260806.4235 11.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 11.14 05:04:30.88 +17:37:20.3
184.28973 -14.09235 galactic Tau Second-epoch detections are separated by 1.0" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J076.1287+17.6202 | 05:04:30.87 +17:37:22.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.404+/-0.024 (G)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:04:30.88 +17:37:20.3: 12.16 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:04:30.88 +17:37:20.3: 12.17 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.16 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 04 30.88 +17 37 20.3 11.1 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J076.1287+17.6202,2461258.9235,11.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J076.1287+17.6202 20260806.4235 11.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 11.12 05:04:24.07 +17:31:54.4
184.35026 -14.16639 galactic Tau Second-epoch detections are separated by 0.5" 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 | Gaia DR3 3407027612651258752 | 05:04:24.11 +17:31:54.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.819+/-0.024 (M)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:04:24.07 +17:31:54.4: 12.12 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:04:24.07 +17:31:54.4: 12.20 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.15 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 04 24.07 +17 31 54.4 11.1 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3407027612651258752,2461258.9235,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3407027612651258752 20260806.4235 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 11.09 05:07:06.62 +17:37:57.7
184.64464 -13.57870 galactic Tau Second-epoch detections are separated by 0.8" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3395106089108805888 | 05:07:06.61 +17:37:58.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.713+/-0.034 (K)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:07:06.62 +17:37:57.7: 12.12 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:07:06.62 +17:37:57.7: 12.14 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.13 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 07 06.62 +17 37 57.7 11.1 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3395106089108805888,2461258.9235,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3395106089108805888 20260806.4235 11.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 11.04 05:07:37.37 +17:51:29.3
184.52538 -13.35009 galactic Tau Second-epoch detections are separated by 0.5" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J076.9119+17.8582 | 05:07:37.46 +17:51:28.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.777+/-0.032 (K)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:07:37.37 +17:51:29.3: 12.11 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:07:37.37 +17:51:29.3: 12.18 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.14 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 07 37.37 +17 51 29.3 11.0 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J076.9119+17.8582,2461258.9235,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J076.9119+17.8582 20260806.4235 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 11.04 05:06:56.61 +18:01:43.0
184.28677 -13.38579 galactic Tau Second-epoch detections are separated by 1.0" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3407142889573090176 | 05:06:56.63 +18:01:42.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.707+/-0.027 (K)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:06:56.61 +18:01:43.0: 12.11 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:06:56.61 +18:01:43.0: 12.14 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.13 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 06 56.61 +18 01 43.0 11.0 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3407142889573090176,2461258.9235,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3407142889573090176 20260806.4235 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 11.09 04:05:04.24 +25:11:13.8
168.97110 -19.91126 galactic Tau Second-epoch detections are separated by 1.1" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 66142191419537024 | 04:05:04.24 +25:11:13.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5) J-Ks=0.269+/-0.032 (F)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:05:04.24 +25:11:13.8: 12.08 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:05:04.24 +25:11:13.8: 12.01 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.05 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 04 05 04.24 +25 11 13.8 11.1 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 66142191419537024,2461258.9235,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 66142191419537024 20260806.4235 11.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 11.04 05:07:55.39 +18:47:29.2
183.77980 -12.75965 galactic Tau Second-epoch detections are separated by 0.3" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3407614992378990720 | 05:07:55.41 +18:47:29.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.559+/-0.028 (K)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:07:55.39 +18:47:29.2: 12.09 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:07:55.39 +18:47:29.2: 12.12 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.10 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 07 55.39 +18 47 29.2 11.0 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3407614992378990720,2461258.9235,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3407614992378990720 20260806.4235 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 11.13 05:07:06.93 +19:02:14.2
183.46101 -12.77576 galactic Tau Second-epoch detections are separated by 1.3" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3407826687023688064 | 05:07:07.01 +19:02:16.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.022+/-0.043 (M)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:07:06.93 +19:02:14.2: 12.08 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:07:06.93 +19:02:14.2: 12.15 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.11 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 07 06.93 +19 02 14.2 11.1 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3407826687023688064,2461258.9235,11.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3407826687023688064 20260806.4235 11.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 11.02 05:08:15.14 +19:15:50.2
183.42797 -12.42587 galactic Tau Second-epoch detections are separated by 3.4" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3407855205606492032 | 05:08:15.07 +19:15:50.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.953+/-0.038 (M)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:08:15.14 +19:15:50.2: 12.06 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:08:15.14 +19:15:50.2: 12.15 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.10 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 08 15.14 +19 15 50.2 11.0 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3407855205606492032,2461258.9235,11.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3407855205606492032 20260806.4235 11.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 11.10 04:06:21.36 +26:13:04.0
168.41464 -18.97816 galactic Tau Second-epoch detections are separated by 1.2" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 162574068459375744 | 04:06:21.43 +26:13:04.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A1V (LAMOST DR5) J-Ks=0.074+/-0.033 (A)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:06:21.36 +26:13:04.0: 12.06 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:06:21.36 +26:13:04.0: 12.00 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.03 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 04 06 21.36 +26 13 04.0 11.1 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 162574068459375744,2461258.9235,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 162574068459375744 20260806.4235 11.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 11.11 05:05:59.79 +17:27:47.2
184.63244 -13.89352 galactic Tau Second-epoch detections are separated by 1.1" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3407017274666675072 | 05:05:59.77 +17:27:47.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.516+/-0.032 (K)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:05:59.79 +17:27:47.2: 12.06 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:05:59.79 +17:27:47.2: 12.14 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.10 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 05 59.79 +17 27 47.2 11.1 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3407017274666675072,2461258.9235,11.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3407017274666675072 20260806.4235 11.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 10.99 05:03:40.32 +17:07:26.1
184.59242 -14.54268 galactic Tau Second-epoch detections are separated by 2.0" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3406978306427649152 | 05:03:40.32 +17:07:27.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.766+/-0.034 (K)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:03:40.32 +17:07:26.1: 12.05 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:03:40.32 +17:07:26.1: 12.09 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.07 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 03 40.32 +17 07 26.1 11.0 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3406978306427649152,2461258.9235,10.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3406978306427649152 20260806.4235 10.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 10.97 04:05:21.00 +26:49:08.6
167.79791 -18.71075 galactic Tau Second-epoch detections are separated by 0.5" 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 | Gaia DR3 163405333610263680 | 04:05:21.00 +26:49:10.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5) J-Ks=0.456+/-0.032 (G)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:05:21.00 +26:49:08.6: 12.03 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:05:21.00 +26:49:08.6: 11.99 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.02 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 04 05 21.00 +26 49 08.6 11.0 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 163405333610263680,2461258.9235,10.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 163405333610263680 20260806.4235 10.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 10.99 05:04:16.37 +17:10:03.9
184.64016 -14.39990 galactic Tau Second-epoch detections are separated by 1.8" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3406983013710865408 | 05:04:16.41 +17:10:04.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.768+/-0.026 (K)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:04:16.37 +17:10:03.9: 12.03 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:04:16.37 +17:10:03.9: 12.08 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.05 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 04 16.37 +17 10 03.9 11.0 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3406983013710865408,2461258.9235,10.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3406983013710865408 20260806.4235 10.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 11.04 05:07:31.01 +17:47:04.6
184.57279 -13.41266 galactic Tau Second-epoch detections are separated by 2.1" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3395113618187330688 | 05:07:31.01 +17:47:06.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.422+/-0.031 (G)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:07:31.01 +17:47:04.6: 12.04 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:07:31.01 +17:47:04.6: 12.13 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.08 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 07 31.01 +17 47 04.6 11.0 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3395113618187330688,2461258.9235,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3395113618187330688 20260806.4235 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 10.96 05:08:11.64 +17:52:51.1
184.58555 -13.22536 galactic Tau Second-epoch detections are separated by 3.0" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J077.0489+17.8806 | 05:08:11.73 +17:52:50.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.248+/-0.030 (M)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:08:11.64 +17:52:51.1: 12.02 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:08:11.64 +17:52:51.1: 12.13 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.07 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 08 11.64 +17 52 51.1 11.0 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J077.0489+17.8806,2461258.9235,10.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J077.0489+17.8806 20260806.4235 10.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 10.91 05:05:19.72 +17:06:12.6
184.84327 -14.22954 galactic Tau Second-epoch detections are separated by 1.2" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3394969852745226880 | 05:05:19.75 +17:06:11.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.898+/-0.044 (M)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:05:19.72 +17:06:12.6: 11.99 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:05:19.72 +17:06:12.6: 12.06 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.02 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 05 19.72 +17 06 12.6 10.9 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3394969852745226880,2461258.9235,10.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3394969852745226880 20260806.4235 10.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 11.03 04:08:50.05 +24:28:47.0
170.14396 -19.79876 galactic Tau Second-epoch detections are separated by 1.4" and 5.1 pix
The object was found in VSX 1" ASASSN-V J040850.08+242847.8
Type: SR
# Max. Min./Amp. JD0 Period
12.180 V 12.270 V 2457265.06000 36.590000000000
The object was not found in astcheck.
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:08:50.05 +24:28:47.0: 12.00 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:08:50.05 +24:28:47.0: 11.92 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.96 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 04 08 50.05 +24 28 47.0 11.0 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J040850.08+242847.8,2461258.9235,11.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J040850.08+242847.8 20260806.4235 11.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 10.86 05:05:22.38 +16:41:53.4
185.19338 -14.45169 galactic Tau Second-epoch detections are separated by 1.1" and 5.2 pix
The object was found in VSX 2" ASASSN-V J050522.49+164151.7
Type: SRS
# Max. Min./Amp. JD0 Period
12.370 V 12.490 V 2458371.04000 22.220000000000
The object was not found in astcheck.
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:05:22.38 +16:41:53.4: 11.97 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:05:22.38 +16:41:53.4: 12.05 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.00 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 05 22.38 +16 41 53.4 10.9 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J050522.49+164151.7,2461258.9235,10.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J050522.49+164151.7 20260806.4235 10.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 10.94 04:04:28.11 +26:35:24.9
167.81991 -19.01188 galactic Tau Second-epoch detections are separated by 1.1" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 163302288754300416 | 04:04:28.01 +26:35:25.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=1.081+/-0.041 (M)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:04:28.11 +26:35:24.9: 11.97 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:04:28.11 +26:35:24.9: 11.90 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.94 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 04 04 28.11 +26 35 24.9 10.9 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 163302288754300416,2461258.9235,10.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 163302288754300416 20260806.4235 10.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 10.92 04:06:30.89 +26:18:21.2
168.37535 -18.89070 galactic Tau Second-epoch detections are separated by 2.0" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 162575580287845120 | 04:06:30.95 +26:18:21.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.418+/-0.030 (G)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:06:30.89 +26:18:21.2: 11.96 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:06:30.89 +26:18:21.2: 11.88 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.92 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 04 06 30.89 +26 18 21.2 10.9 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 162575580287845120,2461258.9235,10.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 162575580287845120 20260806.4235 10.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 10.92 05:07:45.17 +17:38:43.5
184.72338 -13.44554 galactic Tau Second-epoch detections are separated by 0.5" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J076.9369+17.6428 | 05:07:45.29 +17:38:43.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.958+/-0.040 (M)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:07:45.17 +17:38:43.5: 11.95 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:07:45.17 +17:38:43.5: 11.94 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.94 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 07 45.17 +17 38 43.5 10.9 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J076.9369+17.6428,2461258.9235,10.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J076.9369+17.6428 20260806.4235 10.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 10.95 05:07:11.85 +18:01:35.3
184.32396 -13.33740 galactic Tau Second-epoch detections are separated by 2.3" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3407131275981521920 | 05:07:11.89 +18:01:36.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.404+/-0.028 (G)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:07:11.85 +18:01:35.3: 11.96 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:07:11.85 +18:01:35.3: 12.02 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.99 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 07 11.85 +18 01 35.3 10.9 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3407131275981521920,2461258.9235,10.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3407131275981521920 20260806.4235 10.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 10.98 04:04:17.62 +25:51:03.2
168.34131 -19.56505 galactic Tau Second-epoch detections are separated by 0.5" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 162443982490607360 | 04:04:17.56 +25:51:03.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K7 (LAMOST DR5) J-Ks=1.083+/-0.028 (M)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:04:17.62 +25:51:03.2: 11.94 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:04:17.62 +25:51:03.2: 11.86 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.90 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 04 04 17.62 +25 51 03.2 11.0 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 162443982490607360,2461258.9235,10.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 162443982490607360 20260806.4235 10.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 10.93 05:05:10.52 +17:51:42.4
184.18033 -13.82622 galactic Tau Second-epoch detections are separated by 1.2" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3407043349411008000 | 05:05:10.52 +17:51:43.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.390+/-0.033 (G)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:05:10.52 +17:51:42.4: 11.94 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:05:10.52 +17:51:42.4: 11.98 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.96 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 05 10.52 +17 51 42.4 10.9 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3407043349411008000,2461258.9235,10.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3407043349411008000 20260806.4235 10.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 10.88 04:04:55.89 +26:40:29.4
167.83489 -18.87899 galactic Tau Second-epoch detections are separated by 0.4" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 163396812392615424 | 04:04:55.86 +26:40:28.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.676+/-0.031 (K)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:04:55.89 +26:40:29.4: 11.91 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:04:55.89 +26:40:29.4: 11.82 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.87 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 04 04 55.89 +26 40 29.4 10.9 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 163396812392615424,2461258.9235,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 163396812392615424 20260806.4235 10.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 10.87 05:07:25.56 +18:15:53.7
184.15450 -13.15686 galactic Tau Second-epoch detections are separated by 1.1" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3407173783275019904 | 05:07:25.60 +18:15:53.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.355+/-0.028 (G)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:07:25.56 +18:15:53.7: 11.89 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:07:25.56 +18:15:53.7: 11.92 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.90 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 07 25.56 +18 15 53.7 10.9 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3407173783275019904,2461258.9235,10.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3407173783275019904 20260806.4235 10.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 10.90 04:05:52.14 +24:54:11.3
169.32100 -19.98327 galactic Tau Second-epoch detections are separated by 1.8" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 66122606368699008 | 04:05:52.06 +24:54:11.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.205+/-0.030 (M)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:05:52.14 +24:54:11.3: 11.86 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:05:52.14 +24:54:11.3: 11.78 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.82 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 04 05 52.14 +24 54 11.3 10.9 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 66122606368699008,2461258.9235,10.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 66122606368699008 20260806.4235 10.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 10.84 05:06:30.71 +18:29:07.2
183.84144 -13.20895 galactic Tau Second-epoch detections are separated by 0.7" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3407227968582176768 | 05:06:30.71 +18:29:08.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.562+/-0.031 (K)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:06:30.71 +18:29:07.2: 11.83 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:06:30.71 +18:29:07.2: 11.86 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.84 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 06 30.71 +18 29 07.2 10.8 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3407227968582176768,2461258.9235,10.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3407227968582176768 20260806.4235 10.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 10.84 05:07:56.62 +18:19:21.2
184.17778 -13.02305 galactic Tau Second-epoch detections are separated by 0.9" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3407177386750389120 | 05:07:56.64 +18:19:20.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.817+/-0.026 (M)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:07:56.62 +18:19:21.2: 11.82 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:07:56.62 +18:19:21.2: 11.85 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.83 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 07 56.62 +18 19 21.2 10.8 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3407177386750389120,2461258.9235,10.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3407177386750389120 20260806.4235 10.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 10.89 04:06:22.20 +23:59:27.9
170.09892 -20.54209 galactic Tau Second-epoch detections are separated by 1.5" 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 | Gaia DR3 53987743208185728 | 04:06:22.17 +23:59:27.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.861+/-0.031 (M)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:06:22.20 +23:59:27.9: 11.80 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:06:22.20 +23:59:27.9: 11.78 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.79 +/- 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!
TCP 2026 08 06.4235* 04 06 22.20 +23 59 27.9 10.9 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 53987743208185728,2461258.9235,10.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 53987743208185728 20260806.4235 10.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 10.72 05:07:23.67 +18:55:20.5
183.59635 -12.78746 galactic Tau Second-epoch detections are separated by 0.6" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3407631489349621248 | 05:07:23.72 +18:55:21.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.887+/-0.032 (M)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:07:23.67 +18:55:20.5: 11.79 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:07:23.67 +18:55:20.5: 11.88 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.83 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 07 23.67 +18 55 20.5 10.7 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3407631489349621248,2461258.9235,10.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3407631489349621248 20260806.4235 10.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 10.76 04:07:27.66 +26:45:50.0
168.19105 -18.41735 galactic Tau Second-epoch detections are separated by 1.3" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 162659486768814848 | 04:07:27.68 +26:45:49.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0V 1968AbaOB..38...93M [M69] +26 12 J-Ks=0.378+/-0.033 (G)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:07:27.66 +26:45:50.0: 11.73 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:07:27.66 +26:45:50.0: 11.66 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.70 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 04 07 27.66 +26 45 50.0 10.8 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 162659486768814848,2461258.9235,10.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 162659486768814848 20260806.4235 10.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.4235 2461258.9235 10.49 05:07:49.33 +17:58:51.1
184.44938 -13.24128 galactic Tau Second-epoch detections are separated by 1.3" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3407150556091924736 | 05:07:49.34 +17:58:53.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M2V 1986AJ.....92..139S StKM 2- 404
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:07:49.33 +17:58:51.1: 11.48 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:07:49.33 +17:58:51.1: 11.51 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.50 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.4235* 05 07 49.33 +17 58 51.1 10.5 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3407150556091924736,2461258.9235,10.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3407150556091924736 20260806.4235 10.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.68987713 09.01.2026 04:33:15.384 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
First image: 2461049.68987713 09.01.2026 04:33:15.384 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
Last image: 2461258.92372359 06.08.2026 10:09:59.718 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Tau-03-Q1b1x1_051136_TTUQ1b1x1_635740_EPMM3l3i/fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.50
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: 2 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): 10669
Objects passed selection criteria: 10594
Measurements per detected object (mean, median, min, max): 2.1 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.1 2.0 2 4
Average stars detected per image: 6031
Average stars matched: 5933.5 (98.3834 %)
Memory usage VmPeak: 236892 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Aug 5 15:05:04 CDT 2026
VaST build number 1.0rc89-189-g49d3cdfd
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-05)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Aug 6 05:13:49 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: 2461049.68987713 09.01.2026 04:33:15.384 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
First image: 2461049.68987713 09.01.2026 04:33:15.384 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
Last image: 2461258.92372359 06.08.2026 10:09:59.718 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Tau-03-Q1b1x1_051136_TTUQ1b1x1_635740_EPMM3l3i/fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 131
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.21
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: 10 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): 75357
Objects passed selection criteria: 75113
Measurements per detected object (mean, median, min, max): 2.1 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.1 2.0 2 4
Average stars detected per image: 43836.5
Average stars matched: 42578 (97.1291 %)
Memory usage VmPeak: 296520 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Aug 5 15:05:04 CDT 2026
VaST build number 1.0rc89-189-g49d3cdfd
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-05)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Aug 6 05:14:34 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/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Tau-03-Q1b1x1_051136_TTUQ1b1x1_635740_EPMM3l3i/fd_Tau-03-Q1b1x1_2026-08-06_05-09-16_20.00sec_-0.00C_LIGHTs_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Tau-03-Q1b1x1_051136_TTUQ1b1x1_635740_EPMM3l3i/fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417.fits
SExtractor catalog cache: saved Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.cat to cache
SExtractor catalog cache: saved Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.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/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Tau-03-Q1b1x1_051136_TTUQ1b1x1_635740_EPMM3l3i/fd_Tau-03-Q1b1x1_2026-08-06_05-09-16_20.00sec_-0.00C_LIGHTs_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Tau-03-Q1b1x1_051136_TTUQ1b1x1_635740_EPMM3l3i/fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417.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: 2461258.92322010
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_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits exists and is non-empty
Saving wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits to local_wcs_cache/
'wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits' -> 'local_wcs_cache/wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits'
wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits exists and is non-empty
Saving wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits to local_wcs_cache/
'wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits' -> 'local_wcs_cache/wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits'
wcs_fd_Tau-03-Q1b1x1_2026-08-06_05-09-16_20.00sec_-0.00C_LIGHTs_0416.fits exists and is non-empty
Saving wcs_fd_Tau-03-Q1b1x1_2026-08-06_05-09-16_20.00sec_-0.00C_LIGHTs_0416.fits to local_wcs_cache/
'wcs_fd_Tau-03-Q1b1x1_2026-08-06_05-09-16_20.00sec_-0.00C_LIGHTs_0416.fits' -> 'local_wcs_cache/wcs_fd_Tau-03-Q1b1x1_2026-08-06_05-09-16_20.00sec_-0.00C_LIGHTs_0416.fits'
wcs_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417.fits exists and is non-empty
Saving wcs_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417.fits to local_wcs_cache/
'wcs_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417.fits' -> 'local_wcs_cache/wcs_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits (1st reference image)
verification OK: wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
Image size: 941.5'x627.0' 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: 04:36:56.045 +21:59:37.33 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_Tau-03-Q1b1x1_2026-08-06_05-09-16_20.00sec_-0.00C_LIGHTs_0416.fits (1st new image)
verification OK: wcs_fd_Tau-03-Q1b1x1_2026-08-06_05-09-16_20.00sec_-0.00C_LIGHTs_0416.fits
Image size: 941.5'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: 04:37:13.319 +21:59:23.87 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 04:36:56.045 +21:59:37.33
Second-epoch image center 04:37:13.319 +21:59:23.87
Angular distance between the image centers 0.0668 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417.fits (2nd new image)
verification OK: wcs_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417.fits
Image size: 941.5'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: 04:37:15.293 +21:59:09.20 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 04:36:56.045 +21:59:37.33
Second-epoch image center 04:37:15.293 +21:59:09.20
Angular distance between the image centers 0.0748 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 04:37:13.319 +21:59:23.87
Second-epoch second image center 04:37:15.293 +21:59:09.20
Angular distance between the image centers 0.00865 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/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits &> /tmp/tmp.dugaGBsm6T
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits &> /tmp/tmp.6KUcEvbb9Q
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Tau-03-Q1b1x1_051136_TTUQ1b1x1_635740_EPMM3l3i/fd_Tau-03-Q1b1x1_2026-08-06_05-09-16_20.00sec_-0.00C_LIGHTs_0416.fits &> /tmp/tmp.IzDC1Xdv7V
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Tau-03-Q1b1x1_051136_TTUQ1b1x1_635740_EPMM3l3i/fd_Tau-03-Q1b1x1_2026-08-06_05-09-16_20.00sec_-0.00C_LIGHTs_0416.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Tau-03-Q1b1x1_051136_TTUQ1b1x1_635740_EPMM3l3i/fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417.fits &> /tmp/tmp.S02nOpFTyG
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Tau-03-Q1b1x1_051136_TTUQ1b1x1_635740_EPMM3l3i/fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.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_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits and wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.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_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits and wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat
Found non-empty wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits and wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat
The reference image (wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits) and catalog (wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat) found
'wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat' -> 'wcsmag.cat'
Read 11927 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 60.5112 to 78.0902 deg, Dec +16.4856 to +27.2829 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 60.5112 to 78.0902 deg, Dec 16.4856 to 27.2829 deg
Loaded 5180 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): 3947 out of 4318 total matches.
Matched with Tycho-2 4318 out of 11927 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.997400
a=0.000000 b=1.000000 c=22.997400
From vast_summary.log: estimated ref. image limiting mag.: -7.50
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.50
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.50
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 11927 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 60.5112 to 78.0902 deg, Dec +16.4856 to +27.2829 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 60.5112 to 78.0902 deg, Dec 16.4856 to 27.2829 deg
Loaded 5180 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): 3947 out of 4318 total matches.
Matched with Tycho-2 4318 out of 11927 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
Forced-photometry filter: calibrated wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits -> calib.txt_param_ref_wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits (aperture=6.0)
Read 11076 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 60.5314 to 78.0905 deg, Dec +16.4856 to +27.2796 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 60.5314 to 78.0905 deg, Dec 16.4856 to 27.2796 deg
Loaded 5169 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): 3956 out of 4300 total matches.
Matched with Tycho-2 4300 out of 11076 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
Forced-photometry filter: calibrated wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits -> calib.txt_param_ref_wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits (aperture=6.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
2.1 pix Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
3.0 pix fd_Tau-03-Q1b1x1_2026-08-06_05-09-16_20.00sec_-0.00C_LIGHTs_0416.fits
2.9 pix fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417.fits
Limiting magnitude estimates:
15.5 mag. Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
15.4 mag. Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
11.2 mag. fd_Tau-03-Q1b1x1_2026-08-06_05-09-16_20.00sec_-0.00C_LIGHTs_0416.fits
11.1 mag. fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417.fits
All-image limiting magnitude estimate: 11.1 (SNR ) 9.4 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.dugaGBsm6T (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_2026-08-06_CI_Tau-03-Q1b1x1_051136_TTUQ1b1x1_635740_EPMM3l3i/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits' -> 'wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.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/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
WCS_IMAGE_NAME=wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
WCS-calibrated image found: wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
Checking if the catalog wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat corresponding to the image wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits alredy exist and is non-empty...
Catalog wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat corresponding to the image wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
WCS catalog name: wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.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=967, bad_region=0, passed=11927
Got 11927 stars (including 10942 good ones) from the SExtractor catalog wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat
util/solve_plate_with_UCAC5 got 11927 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4866 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4844 matched stars entering correct_measured_positions(), 4844 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4844 matched stars entering correct_measured_positions(), 11927 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4866 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4844 matched stars entering correct_measured_positions(), 11927 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4844 matched stars entering correct_measured_positions(), 11927 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4844 stars left (next iteration limit 5328)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits N_match=4844 sigma_overall_arcsec=0.304 sigma_q1_arcsec=0.380 sigma_q2_arcsec=0.308 sigma_q3_arcsec=0.262 sigma_q4_arcsec=0.246 n_q1=1283 n_q2=1077 n_q3=1448 n_q4=1036 worst_quadrant_to_overall_ratio=1.251
The image catalog is written to wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits -region wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.6KUcEvbb9Q (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_2026-08-06_CI_Tau-03-Q1b1x1_051136_TTUQ1b1x1_635740_EPMM3l3i/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits' -> 'wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.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/Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
WCS_IMAGE_NAME=wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
WCS-calibrated image found: wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
Checking if the catalog wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits.wcscat corresponding to the image wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits alredy exist and is non-empty...
Catalog wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits.wcscat corresponding to the image wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
WCS catalog name: wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.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=897, bad_region=0, passed=11076
Got 11076 stars (including 10166 good ones) from the SExtractor catalog wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits.wcscat
util/solve_plate_with_UCAC5 got 11076 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4864 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4844 matched stars entering correct_measured_positions(), 4844 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4844 matched stars entering correct_measured_positions(), 11076 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4864 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4844 matched stars entering correct_measured_positions(), 11076 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4844 matched stars entering correct_measured_positions(), 11076 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 4844 stars left (next iteration limit 5328)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits N_match=4844 sigma_overall_arcsec=0.351 sigma_q1_arcsec=0.456 sigma_q2_arcsec=0.338 sigma_q3_arcsec=0.326 sigma_q4_arcsec=0.285 n_q1=1273 n_q2=1107 n_q3=1409 n_q4=1055 worst_quadrant_to_overall_ratio=1.297
The image catalog is written to wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits -region wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.IzDC1Xdv7V (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_2026-08-06_CI_Tau-03-Q1b1x1_051136_TTUQ1b1x1_635740_EPMM3l3i/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Tau-03-Q1b1x1_051136_TTUQ1b1x1_635740_EPMM3l3i/fd_Tau-03-Q1b1x1_2026-08-06_05-09-16_20.00sec_-0.00C_LIGHTs_0416.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Tau-03-Q1b1x1_051136_TTUQ1b1x1_635740_EPMM3l3i/fd_Tau-03-Q1b1x1_2026-08-06_05-09-16_20.00sec_-0.00C_LIGHTs_0416.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Tau-03-Q1b1x1_051136_TTUQ1b1x1_635740_EPMM3l3i/fd_Tau-03-Q1b1x1_2026-08-06_05-09-16_20.00sec_-0.00C_LIGHTs_0416.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Tau-03-Q1b1x1_051136_TTUQ1b1x1_635740_EPMM3l3i/fd_Tau-03-Q1b1x1_2026-08-06_05-09-16_20.00sec_-0.00C_LIGHTs_0416.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Tau-03-Q1b1x1_051136_TTUQ1b1x1_635740_EPMM3l3i/fd_Tau-03-Q1b1x1_2026-08-06_05-09-16_20.00sec_-0.00C_LIGHTs_0416.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_2026-08-06_CI_Tau-03-Q1b1x1_051136_TTUQ1b1x1_635740_EPMM3l3i/fd_Tau-03-Q1b1x1_2026-08-06_05-09-16_20.00sec_-0.00C_LIGHTs_0416.fits
WCS_IMAGE_NAME=wcs_fd_Tau-03-Q1b1x1_2026-08-06_05-09-16_20.00sec_-0.00C_LIGHTs_0416.fits
WCS-calibrated image found: wcs_fd_Tau-03-Q1b1x1_2026-08-06_05-09-16_20.00sec_-0.00C_LIGHTs_0416.fits
Checking if the catalog wcs_fd_Tau-03-Q1b1x1_2026-08-06_05-09-16_20.00sec_-0.00C_LIGHTs_0416.fits.wcscat corresponding to the image wcs_fd_Tau-03-Q1b1x1_2026-08-06_05-09-16_20.00sec_-0.00C_LIGHTs_0416.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-03-Q1b1x1_2026-08-06_05-09-16_20.00sec_-0.00C_LIGHTs_0416.fits.wcscat corresponding to the image wcs_fd_Tau-03-Q1b1x1_2026-08-06_05-09-16_20.00sec_-0.00C_LIGHTs_0416.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-03-Q1b1x1_2026-08-06_05-09-16_20.00sec_-0.00C_LIGHTs_0416.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Tau-03-Q1b1x1_051136_TTUQ1b1x1_635740_EPMM3l3i/fd_Tau-03-Q1b1x1_2026-08-06_05-09-16_20.00sec_-0.00C_LIGHTs_0416.fits
WCS catalog name: wcs_fd_Tau-03-Q1b1x1_2026-08-06_05-09-16_20.00sec_-0.00C_LIGHTs_0416.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=56, bad_region=0, passed=708
Got 708 stars (including 650 good ones) from the SExtractor catalog wcs_fd_Tau-03-Q1b1x1_2026-08-06_05-09-16_20.00sec_-0.00C_LIGHTs_0416.fits.wcscat
util/solve_plate_with_UCAC5 got 708 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 530 to 589 (Dec 16.2 to 27.4)
Done reading UCAC5 zone files...
Matched 621 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 617 matched stars entering correct_measured_positions(), 566 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 617 matched stars entering correct_measured_positions(), 645 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
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 530 to 589 (Dec 16.2 to 27.4)
Done reading UCAC5 zone files...
Matched 622 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 615 matched stars entering correct_measured_positions(), 644 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 615 matched stars entering correct_measured_positions(), 644 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 615 stars left (next iteration limit 678)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=615 robust_rms=14.665 arcsec worst_quadrant_rms=18.492 arcsec
SIP_REFIT: SIP order 3 trial: matched=615 robust_rms=0.522 arcsec worst_quadrant_rms=0.612 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=615 robust_rms_before=1.024 arcsec robust_rms_before_corrected=0.514 arcsec robust_rms_after=0.522 arcsec worst_quadrant_rms_before=0.768 worst_quadrant_rms_after=0.612
verification OK: wcs_fd_Tau-03-Q1b1x1_2026-08-06_05-09-16_20.00sec_-0.00C_LIGHTs_0416.fits
verification OK: wcs_fd_Tau-03-Q1b1x1_2026-08-06_05-09-16_20.00sec_-0.00C_LIGHTs_0416.fits
Image size: 941.5'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: 04:37:13.361 +21:59:23.00 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 708 stars ###
'wcs_fd_Tau-03-Q1b1x1_2026-08-06_05-09-16_20.00sec_-0.00C_LIGHTs_0416.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Tau-03-Q1b1x1_051136_TTUQ1b1x1_635740_EPMM3l3i/correct_sextractor_wcs_catalog_usingxy2sky643553.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 3, robust RMS 1.024 -> 0.522 arcsec)
WCS_QUALITY_DIAG: file=fd_Tau-03-Q1b1x1_2026-08-06_05-09-16_20.00sec_-0.00C_LIGHTs_0416.fits N_match=615 sigma_overall_arcsec=0.551 sigma_q1_arcsec=0.477 sigma_q2_arcsec=0.650 sigma_q3_arcsec=0.688 sigma_q4_arcsec=0.375 n_q1=183 n_q2=226 n_q3=127 n_q4=79 worst_quadrant_to_overall_ratio=1.250
The image catalog is written to wcs_fd_Tau-03-Q1b1x1_2026-08-06_05-09-16_20.00sec_-0.00C_LIGHTs_0416.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-03-Q1b1x1_2026-08-06_05-09-16_20.00sec_-0.00C_LIGHTs_0416.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Tau-03-Q1b1x1_051136_TTUQ1b1x1_635740_EPMM3l3i/fd_Tau-03-Q1b1x1_2026-08-06_05-09-16_20.00sec_-0.00C_LIGHTs_0416.fits -region wcs_fd_Tau-03-Q1b1x1_2026-08-06_05-09-16_20.00sec_-0.00C_LIGHTs_0416.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-03-Q1b1x1_2026-08-06_05-09-16_20.00sec_-0.00C_LIGHTs_0416.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.S02nOpFTyG (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_2026-08-06_CI_Tau-03-Q1b1x1_051136_TTUQ1b1x1_635740_EPMM3l3i/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Tau-03-Q1b1x1_051136_TTUQ1b1x1_635740_EPMM3l3i/fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Tau-03-Q1b1x1_051136_TTUQ1b1x1_635740_EPMM3l3i/fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Tau-03-Q1b1x1_051136_TTUQ1b1x1_635740_EPMM3l3i/fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Tau-03-Q1b1x1_051136_TTUQ1b1x1_635740_EPMM3l3i/fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Tau-03-Q1b1x1_051136_TTUQ1b1x1_635740_EPMM3l3i/fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417.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_2026-08-06_CI_Tau-03-Q1b1x1_051136_TTUQ1b1x1_635740_EPMM3l3i/fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417.fits
WCS_IMAGE_NAME=wcs_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417.fits
WCS-calibrated image found: wcs_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417.fits
Checking if the catalog wcs_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417.fits.wcscat corresponding to the image wcs_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417.fits.wcscat corresponding to the image wcs_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Tau-03-Q1b1x1_051136_TTUQ1b1x1_635740_EPMM3l3i/fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417.fits
WCS catalog name: wcs_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417.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=53, bad_region=0, passed=570
Got 570 stars (including 516 good ones) from the SExtractor catalog wcs_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417.fits.wcscat
util/solve_plate_with_UCAC5 got 570 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 530 to 589 (Dec 16.2 to 27.4)
Done reading UCAC5 zone files...
Matched 493 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 491 matched stars entering correct_measured_positions(), 420 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 491 matched stars entering correct_measured_positions(), 483 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
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 530 to 589 (Dec 16.2 to 27.4)
Done reading UCAC5 zone files...
Matched 494 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 489 matched stars entering correct_measured_positions(), 482 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Accuracy estimation diagnostic: 489 matched stars entering correct_measured_positions(), 481 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Excluding outliers - 489 stars left (next iteration limit 540)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=489 robust_rms=15.783 arcsec worst_quadrant_rms=18.444 arcsec
SIP_REFIT: SIP order 3 trial: matched=489 robust_rms=0.471 arcsec worst_quadrant_rms=0.610 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=489 robust_rms_before=1.018 arcsec robust_rms_before_corrected=0.526 arcsec robust_rms_after=0.471 arcsec worst_quadrant_rms_before=0.854 worst_quadrant_rms_after=0.610
verification OK: wcs_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417.fits
verification OK: wcs_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417.fits
Image size: 941.5'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: 04:37:15.328 +21:59:08.33 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 570 stars ###
'wcs_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Tau-03-Q1b1x1_051136_TTUQ1b1x1_635740_EPMM3l3i/correct_sextractor_wcs_catalog_usingxy2sky643544.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 3, robust RMS 1.018 -> 0.471 arcsec)
WCS_QUALITY_DIAG: file=fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417.fits N_match=489 sigma_overall_arcsec=0.507 sigma_q1_arcsec=0.460 sigma_q2_arcsec=0.722 sigma_q3_arcsec=0.553 sigma_q4_arcsec=0.373 n_q1=149 n_q2=158 n_q3=121 n_q4=61 worst_quadrant_to_overall_ratio=1.425
The image catalog is written to wcs_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Tau-03-Q1b1x1_051136_TTUQ1b1x1_635740_EPMM3l3i/fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417.fits -region wcs_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits sigma_overall=0.304 worst_q_ratio=1.251
ref2=Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits sigma_overall=0.351 worst_q_ratio=1.297
new1=fd_Tau-03-Q1b1x1_2026-08-06_05-09-16_20.00sec_-0.00C_LIGHTs_0416.fits sigma_overall=0.551 worst_q_ratio=1.250
new2=fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417.fits sigma_overall=0.507 worst_q_ratio=1.425
reference average sigma_overall=0.3275 worst_q_ratio=1.274
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161_astrometric_residuals.png (4844 matched stars from wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202_astrometric_residuals.png (4844 matched stars from wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Tau-03-Q1b1x1_2026-08-06_05-09-16_20.00sec_-0.00C_LIGHTs_0416_astrometric_residuals.png (615 matched stars from wcs_fd_Tau-03-Q1b1x1_2026-08-06_05-09-16_20.00sec_-0.00C_LIGHTs_0416.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.43 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417_astrometric_residuals.png (489 matched stars from wcs_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.40 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Tau-03-Q1b1x1_2026-08-06_05-09-16_20.00sec_-0.00C_LIGHTs_0416.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-03-Q1b1x1_2026-08-06_05-09-16_20.00sec_-0.00C_LIGHTs_0416.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Tau-03-Q1b1x1_051136_TTUQ1b1x1_635740_EPMM3l3i/wcs_fd_Tau-03-Q1b1x1_2026-08-06_05-09-16_20.00sec_-0.00C_LIGHTs_0416.fits'
Saving fully-calibrated image wcs_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Tau-03-Q1b1x1_051136_TTUQ1b1x1_635740_EPMM3l3i/wcs_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417.fits'
Preparing the HTML report for the field Tau-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20364_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
The candidate 20364_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 04:23:57.80 +24:18:13.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101182_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 101182_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101273_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
The candidate 101273_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 04:28:23.66 +19:10:45.2 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13764_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
The candidate 13764_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01675_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 01675_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55839_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 55839_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02319_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 02319_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06472_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 06472_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58434_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 58434_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55877_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 55877_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57697_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 57697_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 66802_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 66802_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10046_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
The candidate 10046_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 04:04:05.09 +25:42:46.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72730_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 72730_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 67046_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 67046_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57675_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 57675_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 67078_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 67078_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 65543_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 65543_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55409_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
The candidate 55409_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:03:28.01 +16:42:01.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 69775_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 69775_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 73593_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 73593_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 78047_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 78047_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 66859_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 66859_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 67898_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 67898_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71064_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 71064_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55795_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
The candidate 55795_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:03:21.28 +16:45:50.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 76732_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 76732_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57120_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 57120_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 66350_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 66350_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 69104_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 69104_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71185_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 71185_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 80339_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 80339_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 75714_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 75714_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 59332_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 59332_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 73752_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 73752_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 73046_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 73046_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55440_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
The candidate 55440_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:00:34.77 +16:44:08.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 84205_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 84205_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58988_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 58988_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 67601_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 67601_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70545_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 70545_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86339_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 86339_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70339_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 70339_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58720_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 58720_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 67975_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 67975_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 85277_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 85277_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56688_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 56688_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 75830_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 75830_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57305_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 57305_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05989_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 05989_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 75095_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 75095_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 82943_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 82943_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56902_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
The candidate 56902_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:01:09.50 +16:58:07.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 67082_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 67082_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56020_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 56020_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 76478_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 76478_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 79215_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 79215_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 45849_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
The candidate 45849_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 04:04:12.85 +21:43:49.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 76955_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 76955_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 67260_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 67260_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 73071_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 73071_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03938_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 03938_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71308_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 71308_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04684_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 04684_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 69879_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 69879_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 67018_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 67018_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 66142_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 66142_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 67386_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 67386_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 65673_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
The candidate 65673_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:01:02.72 +17:30:38.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 69150_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 69150_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70472_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 70472_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58662_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
The candidate 58662_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:03:18.97 +17:12:22.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13576_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 13576_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 75741_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 75741_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 77161_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 77161_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70860_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 70860_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06659_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 06659_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 65717_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 65717_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58054_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 58054_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 84461_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
The candidate 84461_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:07:19.21 +17:57:08.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02152_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 02152_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58461_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 58461_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 85526_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 85526_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 84831_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 84831_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58080_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 58080_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19127_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 19127_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55512_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 55512_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03738_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 03738_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06017_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 06017_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 67343_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 67343_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 83717_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 83717_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09156_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 09156_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 85040_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 85040_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03184_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 03184_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12112_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
The candidate 12112_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 04:28:18.55 +25:31:40.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72228_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 72228_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15635_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 15635_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 73642_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 73642_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 79654_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 79654_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23360_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 23360_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 76400_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 76400_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02740_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 02740_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30889_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
The candidate 30889_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 04:03:55.27 +23:12:24.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70148_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
Preparing report for the candidate 70148_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34769_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
The candidate 34769_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 04:26:18.95 +22:48:44.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39892_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
The candidate 39892_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 04:25:22.63 +22:17:34.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 40794_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417
The candidate 40794_fd_Tau-03-Q1b1x1_2026-08-06_05-09-59_20.00sec_0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 04:04:42.10 +22:04:53.2 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 5s
make_report_in_HTML.sh TOTAL: 145s
Prepared the HTML report for the field Tau-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
04:08:24.73 +26:55:28.9
04:05:21.00 +26:49:08.6
04:07:26.43 +26:48:49.6
04:07:27.66 +26:45:50.0
04:04:55.89 +26:40:29.4
04:04:28.11 +26:35:24.9
04:06:45.31 +26:35:53.1
04:05:19.66 +26:28:43.7
04:06:04.77 +26:18:32.1
04:06:30.89 +26:18:21.2
04:05:57.40 +26:14:11.4
04:06:21.36 +26:13:04.0
04:04:17.62 +25:51:03.2
04:05:04.24 +25:11:13.8
04:05:52.14 +24:54:11.3
04:08:50.05 +24:28:47.0
04:06:22.20 +23:59:27.9
05:05:22.38 +16:41:53.4
04:57:05.43 +16:49:52.6
05:04:44.76 +16:45:37.9
05:07:27.65 +16:45:16.0
05:07:04.50 +16:52:06.8
05:05:22.97 +16:57:24.9
05:00:13.17 +17:02:18.0
05:05:10.71 +17:02:33.0
05:05:25.76 +17:02:41.8
05:03:40.32 +17:07:26.1
05:05:19.72 +17:06:12.6
04:59:49.11 +17:12:39.3
05:04:16.37 +17:10:03.9
04:58:47.51 +17:15:40.3
05:07:36.51 +17:12:16.7
05:07:16.09 +17:15:32.3
05:04:25.20 +17:27:34.5
05:05:59.79 +17:27:47.2
05:04:24.07 +17:31:54.4
05:06:14.68 +17:31:19.2
05:05:39.01 +17:34:55.7
05:05:52.83 +17:35:02.8
05:04:30.88 +17:37:20.3
05:04:44.43 +17:37:32.2
05:06:25.23 +17:37:24.5
05:06:29.28 +17:36:00.8
05:01:58.83 +17:40:37.9
05:07:45.17 +17:38:43.5
05:07:06.62 +17:37:57.7
05:04:36.57 +17:41:17.5
05:05:10.24 +17:41:24.1
05:07:38.23 +17:41:53.3
05:06:42.45 +17:51:46.3
05:07:37.37 +17:51:29.3
05:07:42.11 +17:55:57.8
05:08:13.73 +17:55:50.1
05:07:49.33 +17:58:51.1
05:07:44.01 +17:59:50.8
05:06:56.61 +18:01:43.0
05:05:38.60 +18:03:20.8
05:08:15.14 +19:15:50.2
05:07:17.86 +18:06:50.3
05:03:21.97 +18:10:46.7
05:07:08.36 +18:09:25.8
05:07:25.56 +18:15:53.7
05:05:54.99 +18:21:10.6
05:07:34.57 +18:24:25.0
05:06:57.08 +18:23:58.6
05:07:23.50 +18:28:28.8
05:06:30.71 +18:29:07.2
05:08:25.09 +18:28:18.9
05:06:49.89 +18:41:49.4
05:06:39.38 +18:44:55.1
05:07:55.39 +18:47:29.2
05:08:15.06 +18:48:06.5
05:07:23.67 +18:55:20.5
05:08:03.47 +18:37:56.0
05:08:03.36 +18:50:51.6
05:06:55.48 +19:00:36.6
05:07:06.93 +19:02:14.2
05:07:37.96 +18:28:57.6
05:08:15.80 +18:23:08.6
05:07:56.62 +18:19:21.2
05:06:06.35 +18:15:50.1
05:08:40.49 +18:12:30.9
05:07:11.85 +18:01:35.3
05:08:32.93 +17:56:17.4
05:08:11.64 +17:52:51.1
05:05:10.52 +17:51:42.4
05:07:03.49 +17:50:22.8
05:07:31.01 +17:47:04.6
05:07:30.80 +17:43:25.2
########### Completed Tau-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 ####
04:11:31.68 +20:56:25.5
04:11:31.70 +20:56:26.3
04:08:24.73 +26:55:28.9
04:57:05.43 +16:49:52.6
04:07:26.43 +26:48:49.6
04:05:57.40 +26:14:11.4
04:59:49.11 +17:12:39.3
05:04:44.76 +16:45:37.9
05:05:25.76 +17:02:41.8
05:05:39.01 +17:34:55.7
05:05:54.99 +18:21:10.6
05:04:44.43 +17:37:32.2
05:05:10.71 +17:02:33.0
05:06:25.23 +17:37:24.5
05:04:25.20 +17:27:34.5
05:07:42.11 +17:55:57.8
05:07:23.50 +18:28:28.8
05:07:37.96 +18:28:57.6
05:05:52.83 +17:35:02.8
05:05:10.24 +17:41:24.1
05:07:17.86 +18:06:50.3
05:08:03.36 +18:50:51.6
05:05:22.97 +16:57:24.9
05:06:14.68 +17:31:19.2
05:06:42.45 +17:51:46.3
05:03:21.97 +18:10:46.7
05:06:06.35 +18:15:50.1
05:06:39.38 +18:44:55.1
05:07:16.09 +17:15:32.3
05:08:25.09 +18:28:18.9
05:07:34.57 +18:24:25.0
05:08:32.93 +17:56:17.4
05:07:36.51 +17:12:16.7
05:04:36.57 +17:41:17.5
05:05:38.60 +18:03:20.8
05:07:30.80 +17:43:25.2
05:07:44.01 +17:59:50.8
04:58:47.51 +17:15:40.3
05:07:38.23 +17:41:53.3
05:07:03.49 +17:50:22.8
05:07:04.50 +16:52:06.8
05:08:15.06 +18:48:06.5
05:00:13.17 +17:02:18.0
04:06:04.77 +26:18:32.1
05:06:49.89 +18:41:49.4
05:08:40.49 +18:12:30.9
05:06:29.28 +17:36:00.8
05:07:27.65 +16:45:16.0
05:08:03.47 +18:37:56.0
05:08:15.80 +18:23:08.6
05:06:55.48 +19:00:36.6
05:01:58.83 +17:40:37.9
05:06:57.08 +18:23:58.6
04:06:45.31 +26:35:53.1
05:07:08.36 +18:09:25.8
04:05:19.66 +26:28:43.7
05:08:13.73 +17:55:50.1
05:04:30.88 +17:37:20.3
05:04:24.07 +17:31:54.4
05:07:06.62 +17:37:57.7
05:07:37.37 +17:51:29.3
05:06:56.61 +18:01:43.0
04:05:04.24 +25:11:13.8
05:07:55.39 +18:47:29.2
05:07:06.93 +19:02:14.2
05:08:15.14 +19:15:50.2
04:06:21.36 +26:13:04.0
05:05:59.79 +17:27:47.2
05:03:40.32 +17:07:26.1
04:05:21.00 +26:49:08.6
05:04:16.37 +17:10:03.9
05:07:31.01 +17:47:04.6
05:08:11.64 +17:52:51.1
05:05:19.72 +17:06:12.6
04:08:50.05 +24:28:47.0
05:05:22.38 +16:41:53.4
04:04:28.11 +26:35:24.9
04:06:30.89 +26:18:21.2
05:07:45.17 +17:38:43.5
05:07:11.85 +18:01:35.3
04:04:17.62 +25:51:03.2
05:05:10.52 +17:51:42.4
04:04:55.89 +26:40:29.4
05:07:25.56 +18:15:53.7
04:05:52.14 +24:54:11.3
05:06:30.71 +18:29:07.2
05:07:56.62 +18:19:21.2
04:06:22.20 +23:59:27.9
05:07:23.67 +18:55:20.5
04:07:27.66 +26:45:50.0
05:07:49.33 +17:58:51.1
###################################################################################
04:11:31.68 +20:56:25.5 -- asteroid (will NOT add it to exclusion list)
04:11:31.70 +20:56:26.3 -- asteroid (will NOT add it to exclusion list)
04:08:24.73 +26:55:28.9 -- not an asteroid (will add it to exclusion list)
04:57:05.43 +16:49:52.6 -- not an asteroid (will add it to exclusion list)
04:07:26.43 +26:48:49.6 -- not an asteroid (will add it to exclusion list)
04:05:57.40 +26:14:11.4 -- not an asteroid (will add it to exclusion list)
04:59:49.11 +17:12:39.3 -- not an asteroid (will add it to exclusion list)
05:04:44.76 +16:45:37.9 -- not an asteroid (will add it to exclusion list)
05:05:25.76 +17:02:41.8 -- not an asteroid (will add it to exclusion list)
05:05:39.01 +17:34:55.7 -- not an asteroid (will add it to exclusion list)
05:05:54.99 +18:21:10.6 -- not an asteroid (will add it to exclusion list)
05:04:44.43 +17:37:32.2 -- not an asteroid (will add it to exclusion list)
05:05:10.71 +17:02:33.0 -- not an asteroid (will add it to exclusion list)
05:06:25.23 +17:37:24.5 -- not an asteroid (will add it to exclusion list)
05:04:25.20 +17:27:34.5 -- not an asteroid (will add it to exclusion list)
05:07:42.11 +17:55:57.8 -- not an asteroid (will add it to exclusion list)
05:07:23.50 +18:28:28.8 -- not an asteroid (will add it to exclusion list)
05:07:37.96 +18:28:57.6 -- not an asteroid (will add it to exclusion list)
05:05:52.83 +17:35:02.8 -- not an asteroid (will add it to exclusion list)
05:05:10.24 +17:41:24.1 -- not an asteroid (will add it to exclusion list)
05:07:17.86 +18:06:50.3 -- not an asteroid (will add it to exclusion list)
05:08:03.36 +18:50:51.6 -- not an asteroid (will add it to exclusion list)
05:05:22.97 +16:57:24.9 -- not an asteroid (will add it to exclusion list)
05:06:14.68 +17:31:19.2 -- not an asteroid (will add it to exclusion list)
05:06:42.45 +17:51:46.3 -- not an asteroid (will add it to exclusion list)
05:03:21.97 +18:10:46.7 -- not an asteroid (will add it to exclusion list)
05:06:06.35 +18:15:50.1 -- not an asteroid (will add it to exclusion list)
05:06:39.38 +18:44:55.1 -- not an asteroid (will add it to exclusion list)
05:07:16.09 +17:15:32.3 -- not an asteroid (will add it to exclusion list)
05:08:25.09 +18:28:18.9 -- not an asteroid (will add it to exclusion list)
05:07:34.57 +18:24:25.0 -- not an asteroid (will add it to exclusion list)
05:08:32.93 +17:56:17.4 -- not an asteroid (will add it to exclusion list)
05:07:36.51 +17:12:16.7 -- asteroid (will NOT add it to exclusion list)
05:04:36.57 +17:41:17.5 -- not an asteroid (will add it to exclusion list)
05:05:38.60 +18:03:20.8 -- not an asteroid (will add it to exclusion list)
05:07:30.80 +17:43:25.2 -- not an asteroid (will add it to exclusion list)
05:07:44.01 +17:59:50.8 -- not an asteroid (will add it to exclusion list)
04:58:47.51 +17:15:40.3 -- not an asteroid (will add it to exclusion list)
05:07:38.23 +17:41:53.3 -- not an asteroid (will add it to exclusion list)
05:07:03.49 +17:50:22.8 -- not an asteroid (will add it to exclusion list)
05:07:04.50 +16:52:06.8 -- not an asteroid (will add it to exclusion list)
05:08:15.06 +18:48:06.5 -- not an asteroid (will add it to exclusion list)
05:00:13.17 +17:02:18.0 -- not an asteroid (will add it to exclusion list)
04:06:04.77 +26:18:32.1 -- not an asteroid (will add it to exclusion list)
05:06:49.89 +18:41:49.4 -- not an asteroid (will add it to exclusion list)
05:08:40.49 +18:12:30.9 -- not an asteroid (will add it to exclusion list)
05:06:29.28 +17:36:00.8 -- not an asteroid (will add it to exclusion list)
05:07:27.65 +16:45:16.0 -- not an asteroid (will add it to exclusion list)
05:08:03.47 +18:37:56.0 -- not an asteroid (will add it to exclusion list)
05:08:15.80 +18:23:08.6 -- not an asteroid (will add it to exclusion list)
05:06:55.48 +19:00:36.6 -- not an asteroid (will add it to exclusion list)
05:01:58.83 +17:40:37.9 -- not an asteroid (will add it to exclusion list)
05:06:57.08 +18:23:58.6 -- not an asteroid (will add it to exclusion list)
04:06:45.31 +26:35:53.1 -- not an asteroid (will add it to exclusion list)
05:07:08.36 +18:09:25.8 -- not an asteroid (will add it to exclusion list)
04:05:19.66 +26:28:43.7 -- not an asteroid (will add it to exclusion list)
05:08:13.73 +17:55:50.1 -- not an asteroid (will add it to exclusion list)
05:04:30.88 +17:37:20.3 -- not an asteroid (will add it to exclusion list)
05:04:24.07 +17:31:54.4 -- not an asteroid (will add it to exclusion list)
05:07:06.62 +17:37:57.7 -- not an asteroid (will add it to exclusion list)
05:07:37.37 +17:51:29.3 -- not an asteroid (will add it to exclusion list)
05:06:56.61 +18:01:43.0 -- not an asteroid (will add it to exclusion list)
04:05:04.24 +25:11:13.8 -- not an asteroid (will add it to exclusion list)
05:07:55.39 +18:47:29.2 -- not an asteroid (will add it to exclusion list)
05:07:06.93 +19:02:14.2 -- not an asteroid (will add it to exclusion list)
05:08:15.14 +19:15:50.2 -- not an asteroid (will add it to exclusion list)
04:06:21.36 +26:13:04.0 -- not an asteroid (will add it to exclusion list)
05:05:59.79 +17:27:47.2 -- not an asteroid (will add it to exclusion list)
05:03:40.32 +17:07:26.1 -- not an asteroid (will add it to exclusion list)
04:05:21.00 +26:49:08.6 -- not an asteroid (will add it to exclusion list)
05:04:16.37 +17:10:03.9 -- not an asteroid (will add it to exclusion list)
05:07:31.01 +17:47:04.6 -- not an asteroid (will add it to exclusion list)
05:08:11.64 +17:52:51.1 -- not an asteroid (will add it to exclusion list)
05:05:19.72 +17:06:12.6 -- not an asteroid (will add it to exclusion list)
04:08:50.05 +24:28:47.0 -- not an asteroid (will add it to exclusion list)
05:05:22.38 +16:41:53.4 -- not an asteroid (will add it to exclusion list)
04:04:28.11 +26:35:24.9 -- not an asteroid (will add it to exclusion list)
04:06:30.89 +26:18:21.2 -- not an asteroid (will add it to exclusion list)
05:07:45.17 +17:38:43.5 -- not an asteroid (will add it to exclusion list)
05:07:11.85 +18:01:35.3 -- not an asteroid (will add it to exclusion list)
04:04:17.62 +25:51:03.2 -- not an asteroid (will add it to exclusion list)
05:05:10.52 +17:51:42.4 -- not an asteroid (will add it to exclusion list)
04:04:55.89 +26:40:29.4 -- not an asteroid (will add it to exclusion list)
05:07:25.56 +18:15:53.7 -- not an asteroid (will add it to exclusion list)
04:05:52.14 +24:54:11.3 -- not an asteroid (will add it to exclusion list)
05:06:30.71 +18:29:07.2 -- not an asteroid (will add it to exclusion list)
05:07:56.62 +18:19:21.2 -- not an asteroid (will add it to exclusion list)
04:06:22.20 +23:59:27.9 -- not an asteroid (will add it to exclusion list)
05:07:23.67 +18:55:20.5 -- not an asteroid (will add it to exclusion list)
04:07:27.66 +26:45:50.0 -- not an asteroid (will add it to exclusion list)
05:07:49.33 +17:58:51.1 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
04:04:17.62 +25:51:03.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:04:28.11 +26:35:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:04:55.89 +26:40:29.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:05:04.24 +25:11:13.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:05:19.66 +26:28:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:05:21.00 +26:49:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:05:52.14 +24:54:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:05:57.40 +26:14:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:06:04.77 +26:18:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:06:21.36 +26:13:04.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:06:22.20 +23:59:27.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:06:30.89 +26:18:21.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:06:45.31 +26:35:53.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:07:26.43 +26:48:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:07:27.66 +26:45:50.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:08:24.73 +26:55:28.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:08:50.05 +24:28:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:05.43 +16:49:52.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:47.51 +17:15:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:49.11 +17:12:39.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:00:13.17 +17:02:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:01:58.83 +17:40:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:03:21.97 +18:10:46.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:03:40.32 +17:07:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:04:16.37 +17:10:03.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:04:24.07 +17:31:54.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:04:25.20 +17:27:34.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:04:30.88 +17:37:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:04:36.57 +17:41:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:04:44.43 +17:37:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:04:44.76 +16:45:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:05:10.24 +17:41:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:05:10.52 +17:51:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:05:10.71 +17:02:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:05:19.72 +17:06:12.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:05:22.38 +16:41:53.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:05:22.97 +16:57:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:05:25.76 +17:02:41.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:05:38.60 +18:03:20.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:05:39.01 +17:34:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:05:52.83 +17:35:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:05:54.99 +18:21:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:05:59.79 +17:27:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:06:06.35 +18:15:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:06:14.68 +17:31:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:06:25.23 +17:37:24.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:06:29.28 +17:36:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:06:30.71 +18:29:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:06:39.38 +18:44:55.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:06:42.45 +17:51:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:06:49.89 +18:41:49.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:06:55.48 +19:00:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:06:56.61 +18:01:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:06:57.08 +18:23:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:03.49 +17:50:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:04.50 +16:52:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:06.62 +17:37:57.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:06.93 +19:02:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:08.36 +18:09:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:11.85 +18:01:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:16.09 +17:15:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:17.86 +18:06:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:23.50 +18:28:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:23.67 +18:55:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:25.56 +18:15:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:27.65 +16:45:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:30.80 +17:43:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:31.01 +17:47:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:34.57 +18:24:25.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:37.37 +17:51:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:37.96 +18:28:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:38.23 +17:41:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:42.11 +17:55:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:44.01 +17:59:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:45.17 +17:38:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:49.33 +17:58:51.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:55.39 +18:47:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:56.62 +18:19:21.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:08:03.36 +18:50:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:08:03.47 +18:37:56.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:08:11.64 +17:52:51.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:08:13.73 +17:55:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:08:15.06 +18:48:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:08:15.14 +19:15:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:08:15.80 +18:23:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:08:25.09 +18:28:18.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:08:32.93 +17:56:17.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:08:40.49 +18:12:30.9 -- 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)
04:04:17.62 +25:51:03.2 -- not a known variable star
04:04:28.11 +26:35:24.9 -- not a known variable star
04:04:55.89 +26:40:29.4 -- not a known variable star
04:05:04.24 +25:11:13.8 -- not a known variable star
04:05:19.66 +26:28:43.7 -- not a known variable star
04:05:21.00 +26:49:08.6 -- not a known variable star
04:05:52.14 +24:54:11.3 -- not a known variable star
04:05:57.40 +26:14:11.4 -- not a known variable star
04:06:04.77 +26:18:32.1 -- not a known variable star
04:06:21.36 +26:13:04.0 -- not a known variable star
04:06:22.20 +23:59:27.9 -- not a known variable star
04:06:30.89 +26:18:21.2 -- not a known variable star
04:06:45.31 +26:35:53.1 -- not a known variable star
04:07:26.43 +26:48:49.6 -- not a known variable star
04:07:27.66 +26:45:50.0 -- not a known variable star
04:08:24.73 +26:55:28.9 -- not a known variable star
04:08:50.05 +24:28:47.0 -- a known variable star
04:57:05.43 +16:49:52.6 -- not a known variable star
04:58:47.51 +17:15:40.3 -- not a known variable star
04:59:49.11 +17:12:39.3 -- a known variable star
05:00:13.17 +17:02:18.0 -- a known variable star
05:01:58.83 +17:40:37.9 -- not a known variable star
05:03:21.97 +18:10:46.7 -- a known variable star
05:03:40.32 +17:07:26.1 -- not a known variable star
05:04:16.37 +17:10:03.9 -- not a known variable star
05:04:24.07 +17:31:54.4 -- not a known variable star
05:04:25.20 +17:27:34.5 -- not a known variable star
05:04:30.88 +17:37:20.3 -- not a known variable star
05:04:36.57 +17:41:17.5 -- not a known variable star
05:04:44.43 +17:37:32.2 -- not a known variable star
05:04:44.76 +16:45:37.9 -- not a known variable star
05:05:10.24 +17:41:24.1 -- not a known variable star
05:05:10.52 +17:51:42.4 -- not a known variable star
05:05:10.71 +17:02:33.0 -- not a known variable star
05:05:19.72 +17:06:12.6 -- not a known variable star
05:05:22.38 +16:41:53.4 -- a known variable star
05:05:22.97 +16:57:24.9 -- not a known variable star
05:05:25.76 +17:02:41.8 -- not a known variable star
05:05:38.60 +18:03:20.8 -- not a known variable star
05:05:39.01 +17:34:55.7 -- not a known variable star
05:05:52.83 +17:35:02.8 -- not a known variable star
05:05:54.99 +18:21:10.6 -- not a known variable star
05:05:59.79 +17:27:47.2 -- not a known variable star
05:06:06.35 +18:15:50.1 -- a known variable star
05:06:14.68 +17:31:19.2 -- not a known variable star
05:06:25.23 +17:37:24.5 -- not a known variable star
05:06:29.28 +17:36:00.8 -- not a known variable star
05:06:30.71 +18:29:07.2 -- not a known variable star
05:06:39.38 +18:44:55.1 -- not a known variable star
05:06:42.45 +17:51:46.3 -- a known variable star
05:06:49.89 +18:41:49.4 -- a known variable star
05:06:55.48 +19:00:36.6 -- not a known variable star
05:06:56.61 +18:01:43.0 -- not a known variable star
05:06:57.08 +18:23:58.6 -- not a known variable star
05:07:03.49 +17:50:22.8 -- not a known variable star
05:07:04.50 +16:52:06.8 -- not a known variable star
05:07:06.62 +17:37:57.7 -- not a known variable star
05:07:06.93 +19:02:14.2 -- not a known variable star
05:07:08.36 +18:09:25.8 -- not a known variable star
05:07:11.85 +18:01:35.3 -- not a known variable star
05:07:16.09 +17:15:32.3 -- not a known variable star
05:07:17.86 +18:06:50.3 -- not a known variable star
05:07:23.50 +18:28:28.8 -- not a known variable star
05:07:23.67 +18:55:20.5 -- not a known variable star
05:07:25.56 +18:15:53.7 -- not a known variable star
05:07:27.65 +16:45:16.0 -- not a known variable star
05:07:30.80 +17:43:25.2 -- not a known variable star
05:07:31.01 +17:47:04.6 -- not a known variable star
05:07:34.57 +18:24:25.0 -- not a known variable star
05:07:37.37 +17:51:29.3 -- not a known variable star
05:07:37.96 +18:28:57.6 -- not a known variable star
05:07:38.23 +17:41:53.3 -- not a known variable star
05:07:42.11 +17:55:57.8 -- a known variable star
05:07:44.01 +17:59:50.8 -- not a known variable star
05:07:45.17 +17:38:43.5 -- not a known variable star
05:07:49.33 +17:58:51.1 -- not a known variable star
05:07:55.39 +18:47:29.2 -- not a known variable star
05:07:56.62 +18:19:21.2 -- not a known variable star
05:08:03.36 +18:50:51.6 -- not a known variable star
05:08:03.47 +18:37:56.0 -- not a known variable star
05:08:11.64 +17:52:51.1 -- not a known variable star
05:08:13.73 +17:55:50.1 -- not a known variable star
05:08:15.06 +18:48:06.5 -- not a known variable star
05:08:15.14 +19:15:50.2 -- not a known variable star
05:08:15.80 +18:23:08.6 -- not a known variable star
05:08:25.09 +18:28:18.9 -- not a known variable star
05:08:32.93 +17:56:17.4 -- not a known variable star
05:08:40.49 +18:12:30.9 -- not a known variable star
Found 79 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
88 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 88 (excluding asteroids and hot pixels, 79 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)2461258.92322010 -observatory V36
07:46:47.51 +20:23:24.2 Mercury (-0.4mag)
11:56:25.30 -00:09:58.9 Venus (-4.3mag)
05:44:02.23 +23:33:05.0 Mars (1.3mag)
08:41:19.27 +18:47:17.6 Jupiter (-1.8mag)
00:56:32.22 +03:16:39.1 Saturn (0.6mag)
04:11:31.22 +20:56:24.6 Uranus (5.8mag)
00:16:12.12 +00:13:53.9 Neptune (7.7mag)
20:28:18.80 -23:29:29.1 Pluto (14.4mag)
02:57:42.01 +21:50:04.7 Moon (-10.3mag)
-rw-r--r-- 1 apache apache 363 Aug 6 05:13 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461258.92322010:
08:41:22.88 +18:47:01.9 Io (6.0mag)
08:41:13.20 +18:47:44.4 Europa (6.3mag)
08:41:18.52 +18:47:24.8 Ganymede (5.6mag)
08:41:07.32 +18:48:12.1 Callisto (6.7mag)
08:38:54.91 +18:45:35.0 Himalia (15.7mag)
08:41:20.82 +18:47:11.4 Thebe (16.6mag)
08:38:25.68 +18:44:27.8 Elara (17.7mag)
08:45:25.28 +18:27:36.6 Pasiphae (17.9mag)
08:44:37.27 +18:57:10.7 Carme (19.0mag)
00:56:28.99 +03:17:06.1 Titan (8.4mag)
00:56:26.18 +03:16:39.5 Rhea (9.7mag)
00:56:36.43 +03:15:03.4 Iapetus (11.1mag)
00:56:18.40 +03:16:51.5 Hyperion (14.4mag)
00:55:56.98 +03:10:04.1 Phoebe (16.5mag)
-rw-r--r-- 1 apache apache 568 Aug 6 05:13 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461258.92322010:
18:55:35.82 -23:53:46.8 JWST
17:29:20.14 +36:18:19.0 Chandra
11:23:38.98 -60:31:46.7 XMM-Newton
-rw-r--r-- 1 apache apache 96 Aug 6 05:13 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461258.92322010 -observatory V36
03:11:37.37 +17:13:31.0 17.7mag P/1996 R2 (Lagerkvist)
18:02:20.44 -34:38:19.0 14.0mag P/2010 H2 (Vales)
06:52:06.48 -68:50:05.8 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:09:20.38 +32:57:20.7 17.7mag C/2017 K2 (PANSTARRS)
03:38:20.20 +36:50:01.8 16.7mag P/2021 N1 (ZTF)
22:40:06.76 +31:33:15.8 17.3mag C/2022 E2 (ATLAS)
06:41:41.19 +26:34:19.7 16.8mag C/2022 N2 (PANSTARRS)
10:19:54.24 +28:33:02.1 17.0mag C/2022 QE78 (ATLAS)
09:27:39.27 +05:17:45.9 17.9mag C/2022 R6 (PANSTARRS)
15:12:10.97 -12:12:55.8 17.9mag P/2023 B1 (PANSTARRS)
21:13:08.50 +66:12:39.9 17.9mag C/2023 H5 (Lemmon)
15:49:41.42 -12:46:04.1 14.3mag C/2023 R1 (PANSTARRS)
08:06:04.09 +31:15:53.7 15.3mag C/2024 E1 (Wierzchos)
15:07:15.57 +15:36:56.6 17.7mag C/2024 G6 (ATLAS)
19:05:24.70 +42:58:29.4 13.7mag C/2024 J3 (ATLAS)
21:13:22.33 +49:05:32.6 17.6mag C/2024 R4 (PANSTARRS)
05:13:41.25 -12:59:28.4 15.5mag C/2024 T5 (ATLAS)
06:55:03.06 +24:28:22.9 17.9mag C/2025 J1 (Borisov)
07:30:02.48 -15:53:38.6 17.7mag C/2025 R3 (PANSTARRS)
10:30:24.22 +21:01:07.4 17.3mag C/2025 V2 (Rankin)
12:57:03.50 +02:28:08.5 17.0mag C/2025 Y1 (ATLAS)
16:03:36.89 +77:59:58.8 16.8mag C/2026 A2 (Bok)
03:06:48.02 +46:09:00.8 17.1mag C/2026 B2 (Sun-Gao)
11:45:18.74 +08:21:16.3 17.3mag A/2026 E1
21:56:19.14 -26:32:32.2 6.9mag 10P/Tempel
11:27:53.19 -03:17:18.7 16.2mag 29P/Schwassmann-Wachmann
04:37:00.53 +32:16:51.8 18.0mag 47P/Ashbrook-Jackson
11:04:01.18 +05:13:52.3 17.2mag 63P/Wild
00:54:17.55 -05:23:07.0 15.4mag 65P/Gunn
05:31:27.59 +20:43:38.6 13.7mag 78P/Gehrels
20:39:36.21 -23:18:55.7 17.8mag 84P/Giclas
02:58:55.89 +13:33:20.6 16.7mag 88P/Howell
07:51:16.99 +27:54:08.8 16.1mag 93P/Lovas
04:01:17.21 +16:10:27.1 17.6mag 112P/Urata-Niijima
05:50:31.96 +30:29:46.7 16.3mag 114P/Wiseman-Skiff
09:14:13.53 +26:57:11.0 15.0mag 123P/West-Hartley
11:40:08.01 -09:34:31.1 17.1mag 124P/Mrkos
05:33:53.75 +21:11:10.3 16.1mag 128P/Shoemaker-Holt
06:25:25.85 +18:59:13.9 17.9mag 131P/Mueller
00:03:40.12 +03:25:17.7 17.6mag 139P/Vaisala-Oterma
03:21:31.14 -19:44:28.5 14.0mag 161P/Hartley-IRAS
07:09:56.26 +37:42:10.0 15.8mag 162P/SidingSpring
15:46:28.97 +39:39:06.1 12.3mag 169P/NEAT
02:39:40.80 +09:28:49.2 17.6mag 220P/McNaught
16:40:40.95 -09:57:30.7 17.7mag 235P/LINEAR
20:23:34.57 -52:50:55.7 17.8mag 259P/Garradd
03:16:51.91 +24:24:21.6 15.4mag 260P/McNaught
06:59:56.64 +37:45:07.5 17.3mag 295P/LINEAR
15:09:54.55 +03:20:13.5 17.7mag 391P/Kowalski
08:59:14.69 +18:27:51.7 17.9mag 450P/LONEOS
-rw-r--r-- 1 apache apache 2.5K Aug 6 05:13 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
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
02:02:26.67 +32:04:22.70 AT2026ovz 2026-06-14.6 15.52
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:33.11 -68:48:32.90 ASASSN-26no 2026-05-24.03 8.35
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.72 -58:37:47.60 ASASSN-26dn 2026-05-20.01 14.64
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.28 +22:02:03.40 AT2026lxf 2026-05-8.07 13.88
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:49.13 -61:36:14.60 ASASSN-26dd 2026-05-5.15 15.93
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
-rw-r--r-- 1 apache apache 5.7K Aug 6 05:13 asassn_transients_list.txt
############################################################
Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
12:24:25.10 +28:47:12.0 TCP J12242510+2847120 2026-05-31.6015 14.8mag
00:56:07.13 +43:01:40.6 TCP J00560713+4301406 2026-06-01.4135 12.2mag
00:42:41.64 +41:15:16.2 PNV J00424164+4115162 2026-06-02.029 17.4mag
00:42:38.68 +41:15:58.2 PNV J00423868+4115582 2026-06-05.1224 19.97Umag
19:00:42.95 -48:31:01.7 PNV J19004295-4831017 2026-05-25.0752 14.2mag
09:55:21.28 +69:02:52.6 PNV J09552128+6902526 2026-06-13.933 18.9mag
19:51:21.42 +37:06:40.0 TCP J19512142+3706400 2026-06-17.2942 16.8mag
19:57:03.87 +37:41:46.4 TCP J19570387+3741464 2026-06-18.2638 17.5mag
00:42:32.04 +41:10:28.3 PNV J00423204+4110283 2026-06-26.059 16.6mag
02:19:17.36 +28:57:15.8 TCP J02191736+2857158 2026-07-12.3549 12.5mag
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
-rw-r--r-- 1 apache apache 189K Aug 6 05:13 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
12:00:47.340 +09:31:50.99 AT 2026vlb 2026-05-21.37 20.73
09:39:31.292 -08:28:35.35 AT 2026vla 2026-02-21.40 20.65
17:07:24.157 +32:28:59.94 AT 2026vkz 2026-06-16.33 21.89
18:55:34.805 +34:42:05.78 AT 2026vky 2026-06-22.39 21.01
15:27:13.875 -10:50:21.14 AT 2026vkx 2026-06-14.35 20.55
13:36:43.476 +25:28:01.16 AT 2026vkw 2026-06-25.38 20.6
04:43:04.292 -16:08:54.64 AT 2026vkv 2026-01-12.30 21.72
04:48:25.928 -18:19:58.05 AT 2026vku 2026-01-26.25 21.35
12:55:24.686 +13:58:33.13 AT 2026vkt 2026-06-05.34 21.42
11:39:28.884 +47:23:59.43 AT 2026vks 2026-01-14.61 21.82
10:26:55.799 -14:09:20.42 AT 2026vkr 2026-01-13.55 21.98
12:26:22.284 +20:06:25.68 AT 2026vkq 2026-02-13.60 20.86
12:08:12.778 +41:30:56.83 AT 2026vkp 2026-06-15.27 20.88
05:11:50.298 -12:02:24.75 AT 2026vko 2026-02-15.23 20.49
00:35:37.087 -45:29:22.45 AT 2026vkn 2026-06-26.42 23.13
04:11:06.535 -49:23:35.67 AT 2026vkm 2026-07-09.42 22.31
23:40:19.411 -26:01:53.34 AT 2026vkl 2026-07-20.59 21.47
22:23:27.160 +00:54:32.97 AT 2026vkk 2026-07-14.55 21.17
21:14:05.875 -09:55:36.50 AT 2026vkj 2026-07-20.46 21.9
17:17:56.970 +19:09:32.22 AT 2026vki 2026-07-19.39 21.8
-rw-r--r-- 1 apache apache 87K Aug 6 05:13 tns_transients_list.txt
