This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 08 24.3495 2461276.8495 10.74 03:42:40.46 +13:08:33.4
174.34014 -32.14972 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 38052997925811072 | 03:42:40.50 +13:08:33.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F6 (LAMOST DR5) J-Ks=0.381+/-0.028 (G)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:42:40.46 +13:08:33.4: 11.64 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:42:40.46 +13:08:33.4: 11.62 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.63 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 24.3495* 03 42 40.46 +13 08 33.4 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 38052997925811072,2461276.8495,10.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 38052997925811072 20260824.3495 10.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 24.3495 2461276.8495 10.81 03:36:30.64 +14:41:35.9
171.79681 -32.10064 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 41489452798983168 | 03:36:30.62 +14:41:35.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.379+/-0.028 (G)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:36:30.64 +14:41:35.9: 11.80 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:36:30.64 +14:41:35.9: 11.81 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.80 +/- 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 24.3495* 03 36 30.64 +14 41 35.9 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 41489452798983168,2461276.8495,10.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 41489452798983168 20260824.3495 10.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 24.3495 2461276.8495 11.14 03:43:16.67 +17:34:21.6
170.84186 -28.89837 galactic Tau Second-epoch detections are separated by 0.8" and 5.4 pix
The object was found in VSX 1" HAT 307-0002013
Type: ROT
# Max. Min./Amp. JD0 Period
10.960 J Y 0.002 r 5.114391940000
The object was not found in astcheck.
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:43:16.67 +17:34:21.6: 12.02 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:43:16.67 +17:34:21.6: 12.07 +/- 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 24.3495* 03 43 16.67 +17 34 21.6 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
HAT 307-0002013,2461276.8495,11.14,0.05,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
HAT 307-0002013 20260824.3495 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 24.3495 2461276.8495 10.88 03:38:15.64 +11:29:00.0
174.85539 -34.08080 galactic Tau Second-epoch detections are separated by 0.6" 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 37252145438898048 | 03:38:15.66 +11:28:59.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5) J-Ks=0.535+/-0.031 (K)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:38:15.64 +11:29:00.0: 12.09 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:38:15.64 +11:29:00.0: 12.07 +/- 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 24.3495* 03 38 15.64 +11 29 00.0 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 37252145438898048,2461276.8495,10.88,0.05,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 37252145438898048 20260824.3495 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 24.3495 2461276.8495 10.63 03:38:07.41 +11:06:21.3
175.15376 -34.36839 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 37177894046235904 | 03:38:07.41 +11:06:21.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=1.057+/-0.035 (M)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:38:07.41 +11:06:21.3: 12.11 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:38:07.41 +11:06:21.3: 12.13 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.12 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 24.3495* 03 38 07.41 +11 06 21.3 10.6 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 37177894046235904,2461276.8495,10.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 37177894046235904 20260824.3495 10.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 24.3495 2461276.8495 11.29 03:42:17.82 +13:30:49.1
173.95210 -31.95499 galactic Tau Second-epoch detections are separated by 0.6" 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 38113097405266944 | 03:42:17.81 +13:30:49.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G4 (LAMOST DR5) J-Ks=0.579+/-0.028 (K)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:42:17.82 +13:30:49.1: 12.37 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:42:17.82 +13:30:49.1: 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 24.3495* 03 42 17.82 +13 30 49.1 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 38113097405266944,2461276.8495,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 38113097405266944 20260824.3495 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 24.3495 2461276.8495 11.22 03:41:11.96 +12:31:30.5
174.56506 -32.83859 galactic Tau Second-epoch detections are separated by 0.2" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 37616152509305088 | 03:41:12.00 +12:31:30.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5) J-Ks=0.398+/-0.026 (G)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:41:11.96 +12:31:30.5: 12.48 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:41:11.96 +12:31:30.5: 12.46 +/- 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 24.3495* 03 41 11.96 +12 31 30.5 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 37616152509305088,2461276.8495,11.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 37616152509305088 20260824.3495 11.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 24.3495 2461276.8495 11.02 03:33:45.06 +09:19:38.8
175.80123 -36.37875 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 | Gaia DR3 11813256008042624 | 03:33:45.09 +09:19:39.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.796+/-0.031 (K)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:33:45.06 +09:19:38.8: 12.53 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:33:45.06 +09:19:38.8: 12.54 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.53 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 24.3495* 03 33 45.06 +09 19 38.8 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 11813256008042624,2461276.8495,11.02,0.05,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 11813256008042624 20260824.3495 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 24.3495 2461276.8495 11.55 03:39:06.56 +15:36:07.4
171.58772 -31.01100 galactic Tau Second-epoch detections are separated by 1.2" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 41655788292864384 | 03:39:06.60 +15:36:07.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.690+/-0.028 (K)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:39:06.56 +15:36:07.4: 12.55 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:39:06.56 +15:36:07.4: 12.51 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.53 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 24.3495* 03 39 06.56 +15 36 07.4 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 41655788292864384,2461276.8495,11.55,0.05,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 41655788292864384 20260824.3495 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 24.3495 2461276.8495 11.39 03:30:43.05 +09:00:26.2
175.43634 -37.13874 galactic Tau Second-epoch detections are separated by 2.1" and 5.3 pix
The object was found in VSX 1" Gaia DR3 12432113551592448
Type: ROT
# Max. Min./Amp. JD0 Period
12.350 G 12.370 G K
The object was not found in astcheck.
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:30:43.05 +09:00:26.2: 12.63 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:30:43.05 +09:00:26.2: 12.63 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 24.3495* 03 30 43.05 +09 00 26.2 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 12432113551592448,2461276.8495,11.39,0.05,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 12432113551592448 20260824.3495 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 24.3495 2461276.8495 11.61 03:36:04.07 +14:27:48.8
171.89375 -32.34051 galactic Tau Second-epoch detections are separated by 0.2" 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 | target | 03:36:04.07 +14:27:48.8 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.461+/-0.028 (G)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:36:04.07 +14:27:48.8: 12.85 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:36:04.07 +14:27:48.8: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.87 +/- 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 24.3495* 03 36 04.07 +14 27 48.8 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
target,2461276.8495,11.61,0.05,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 20260824.3495 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 24.3495 2461276.8495 11.59 03:42:24.28 +13:03:27.1
174.35766 -32.25617 galactic Tau Second-epoch detections are separated by 2.5" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:42:24.28 +13:03:27.1 (user input) | T | P | (position from user input) SpType: F6 (LAMOST DR5) J-Ks=0.410+/-0.030 (G)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:42:24.28 +13:03:27.1: 12.93 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:42:24.28 +13:03:27.1: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 24.3495* 03 42 24.28 +13 03 27.1 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,2461276.8495,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260824.3495 11.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 24.3495 2461276.8495 11.46 03:37:14.30 +10:39:56.1
175.35353 -34.83108 galactic Tau Second-epoch detections are separated by 2.1" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:37:14.30 +10:39:56.1 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.725+/-0.033 (K)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:37:14.30 +10:39:56.1: 13.05 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:37:14.30 +10:39:56.1: 13.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 24.3495* 03 37 14.30 +10 39 56.1 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
target,2461276.8495,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260824.3495 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 24.3495 2461276.8495 11.85 03:37:38.51 +10:57:57.9
175.17537 -34.55061 galactic Tau Second-epoch detections are separated by 2.7" 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 J054.4122+10.9670 | 03:37:38.51 +10:57:57.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A7V (LAMOST DR5) J-Ks=0.365+/-0.033 (G)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:37:38.51 +10:57:57.9: 13.63 +/- 0.03 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:37:38.51 +10:57:57.9: 13.63 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 24.3495* 03 37 38.51 +10 57 57.9 11.8 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
ATO J054.4122+10.9670,2461276.8495,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J054.4122+10.9670 20260824.3495 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 24.3495 2461276.8495 11.67 03:37:50.14 +11:12:45.2
175.00156 -34.34454 galactic Tau Second-epoch detections are separated by 3.2" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:37:50.14 +11:12:45.2 (user input) | T | P | (position from user input) J-Ks=0.445+/-0.034 (G)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:37:50.14 +11:12:45.2: 13.47 +/- 0.03 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:37:50.14 +11:12:45.2: 13.48 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 24.3495* 03 37 50.14 +11 12 45.2 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,2461276.8495,11.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260824.3495 11.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 24.3495 2461276.8495 11.55 03:38:03.25 +10:46:22.9
175.42929 -34.61239 galactic Tau Second-epoch detections are separated by 1.6" 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 | target | 03:38:03.25 +10:46:22.9 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.479+/-0.031 (K)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:38:03.25 +10:46:22.9: 13.46 +/- 0.03 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:38:03.25 +10:46:22.9: 13.48 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 24.3495* 03 38 03.25 +10 46 22.9 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
target,2461276.8495,11.55,0.05,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 20260824.3495 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 24.3495 2461276.8495 11.52 03:37:45.14 +11:03:45.5
175.11437 -34.46383 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 | target | 03:37:45.14 +11:03:45.5 (user input) | T | P | (position from user input) J-Ks=0.470+/-0.035 (K)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:37:45.14 +11:03:45.5: 13.39 +/- 0.03 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:37:45.14 +11:03:45.5: 13.41 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.40 +/- 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 24.3495* 03 37 45.14 +11 03 45.5 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
target,2461276.8495,11.52,0.05,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
target 20260824.3495 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 24.3495 2461276.8495 11.56 03:40:22.93 +12:11:01.6
174.68974 -33.21994 galactic Tau Second-epoch detections are separated by 2.3" 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 | target | 03:40:22.93 +12:11:01.6 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.425+/-0.028 (G)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:40:22.93 +12:11:01.6: 13.34 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:40:22.93 +12:11:01.6: 13.24 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.29 +/- 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 24.3495* 03 40 22.93 +12 11 01.6 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,2461276.8495,11.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260824.3495 11.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 24.3495 2461276.8495 11.72 03:39:51.61 +12:08:08.8
174.62404 -33.34469 galactic Tau Second-epoch detections are separated by 1.2" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:39:51.61 +12:08:08.8 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.544+/-0.028 (K)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:39:51.61 +12:08:08.8: 13.34 +/- 0.03 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:39:51.61 +12:08:08.8: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 24.3495* 03 39 51.61 +12 08 08.8 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,2461276.8495,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260824.3495 11.72CV 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 24.3495 2461276.8495 11.69 03:42:28.33 +17:37:28.4
170.64242 -28.99372 galactic Tau Second-epoch detections are separated by 1.3" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:42:28.33 +17:37:28.4 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.758+/-0.030 (K)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:42:28.33 +17:37:28.4: 13.27 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:42:28.33 +17:37:28.4: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 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 24.3495* 03 42 28.33 +17 37 28.4 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,2461276.8495,11.69,0.05,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 20260824.3495 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 24.3495 2461276.8495 11.54 03:42:19.11 +13:12:25.1
174.21422 -32.16647 galactic Tau Second-epoch detections are separated by 1.0" 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 | target | 03:42:19.11 +13:12:25.1 (user input) | T | P | (position from user input) SpType: K5 (LAMOST DR5) J-Ks=0.822+/-0.028 (M)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:42:19.11 +13:12:25.1: 13.27 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:42:19.11 +13:12:25.1: 13.26 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 24.3495* 03 42 19.11 +13 12 25.1 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
target,2461276.8495,11.54,0.05,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
target 20260824.3495 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 24.3495 2461276.8495 11.38 03:38:05.85 +10:47:26.7
175.42280 -34.59241 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 | target | 03:38:05.85 +10:47:26.7 (user input) | T | P | (position from user input) J-Ks=0.494+/-0.032 (K)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:38:05.85 +10:47:26.7: 13.26 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:38:05.85 +10:47:26.7: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 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 24.3495* 03 38 05.85 +10 47 26.7 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
target,2461276.8495,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260824.3495 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 24.3495 2461276.8495 11.80 03:37:58.82 +11:25:22.3
174.84958 -34.17218 galactic Tau Second-epoch detections are separated by 2.9" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:37:58.82 +11:25:22.3 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.309+/-0.031 (F)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:37:58.82 +11:25:22.3: 13.25 +/- 0.03 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:37:58.82 +11:25:22.3: 13.26 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.25 +/- 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 24.3495* 03 37 58.82 +11 25 22.3 11.8 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
target,2461276.8495,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260824.3495 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 24.3495 2461276.8495 11.26 03:36:52.87 +10:20:00.7
175.57012 -35.12514 galactic Tau Second-epoch detections are separated by 1.7" 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 | target | 03:36:52.87 +10:20:00.7 (user input) | T | P | (position from user input) J-Ks=0.655+/-0.032 (K)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:36:52.87 +10:20:00.7: 13.24 +/- 0.03 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:36:52.87 +10:20:00.7: 13.17 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.20 +/- 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 24.3495* 03 36 52.87 +10 20 00.7 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
target,2461276.8495,11.26,0.05,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
target 20260824.3495 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 24.3495 2461276.8495 11.79 03:42:07.85 +13:20:14.1
174.06674 -32.10763 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 | target | 03:42:07.85 +13:20:14.1 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.375+/-0.029 (G)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:42:07.85 +13:20:14.1: 13.23 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:42:07.85 +13:20:14.1: 13.18 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.21 +/- 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 24.3495* 03 42 07.85 +13 20 14.1 11.8 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
target,2461276.8495,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260824.3495 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 24.3495 2461276.8495 11.51 03:37:48.94 +11:11:08.7
175.02065 -34.36677 galactic Tau Second-epoch detections are separated by 0.6" and 5.4 pix
The object was found in VSX 1" Gaia DR3 37226375636963584
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.990 G 13.020 G A
The object was not found in astcheck.
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:37:48.94 +11:11:08.7: 13.18 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:37:48.94 +11:11:08.7: 13.15 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 24.3495* 03 37 48.94 +11 11 08.7 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
Gaia DR3 37226375636963584,2461276.8495,11.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 37226375636963584 20260824.3495 11.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 24.3495 2461276.8495 11.64 03:36:51.45 +10:40:53.1
175.26024 -34.88716 galactic Tau Second-epoch detections are separated by 3.7" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:36:51.45 +10:40:53.1 (user input) | T | P | (position from user input) SpType: G6 (LAMOST DR5) J-Ks=0.685+/-0.032 (K)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:36:51.45 +10:40:53.1: 13.16 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:36:51.45 +10:40:53.1: 13.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.14 +/- 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 24.3495* 03 36 51.45 +10 40 53.1 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,2461276.8495,11.64,0.05,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
target 20260824.3495 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 24.3495 2461276.8495 11.72 03:40:26.08 +12:14:34.7
174.64988 -33.16938 galactic Tau Second-epoch detections are separated by 1.5" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:40:26.08 +12:14:34.7 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.718+/-0.028 (K)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:40:26.08 +12:14:34.7: 13.14 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:40:26.08 +12:14:34.7: 13.22 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 24.3495* 03 40 26.08 +12 14 34.7 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,2461276.8495,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260824.3495 11.72CV 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 24.3495 2461276.8495 11.47 03:38:54.30 +11:40:32.5
174.82259 -33.83348 galactic Tau Second-epoch detections are separated by 3.9" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:38:54.30 +11:40:32.5 (user input) | T | P | (position from user input) SpType: F3 (LAMOST DR5) J-Ks=0.396+/-0.035 (G)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:38:54.30 +11:40:32.5: 13.12 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:38:54.30 +11:40:32.5: 13.13 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 24.3495* 03 38 54.30 +11 40 32.5 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
target,2461276.8495,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260824.3495 11.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 24.3495 2461276.8495 11.56 03:33:35.49 +09:19:19.0
175.77216 -36.41086 galactic Tau Second-epoch detections are separated by 0.1" 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 | target | 03:33:35.49 +09:19:19.0 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.396+/-0.031 (G)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:33:35.49 +09:19:19.0: 13.12 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:33:35.49 +09:19:19.0: 13.15 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 24.3495* 03 33 35.49 +09 19 19.0 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,2461276.8495,11.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260824.3495 11.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 24.3495 2461276.8495 11.61 03:38:41.89 +11:48:18.3
174.66870 -33.77913 galactic Tau Second-epoch detections are separated by 0.2" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:38:41.89 +11:48:18.3 (user input) | T | P | (position from user input) SpType: A1IV (LAMOST DR5) J-Ks=0.220+/-0.033 (F)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:38:41.89 +11:48:18.3: 13.07 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:38:41.89 +11:48:18.3: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.07 +/- 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 24.3495* 03 38 41.89 +11 48 18.3 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,2461276.8495,11.61,0.05,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 20260824.3495 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 24.3495 2461276.8495 11.59 03:38:18.91 +15:14:42.4
171.71612 -31.40084 galactic Tau Second-epoch detections are separated by 0.7" 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 | 03:38:18.91 +15:14:42.4 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=0.366+/-0.030 (G)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:38:18.91 +15:14:42.4: 13.05 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:38:18.91 +15:14:42.4: 13.04 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.05 +/- 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 24.3495* 03 38 18.91 +15 14 42.4 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,2461276.8495,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260824.3495 11.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 24.3495 2461276.8495 11.46 03:40:33.82 +12:11:44.4
174.71662 -33.17991 galactic Tau Second-epoch detections are separated by 1.6" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:40:33.82 +12:11:44.4 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.554+/-0.027 (K)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:40:33.82 +12:11:44.4: 13.00 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:40:33.82 +12:11:44.4: 13.03 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.02 +/- 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 24.3495* 03 40 33.82 +12 11 44.4 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
target,2461276.8495,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260824.3495 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 24.3495 2461276.8495 11.43 03:36:48.29 +10:33:09.3
175.36195 -34.98622 galactic Tau Second-epoch detections are separated by 2.2" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:36:48.29 +10:33:09.3 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.651+/-0.030 (K)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:36:48.29 +10:33:09.3: 12.95 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:36:48.29 +10:33:09.3: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.96 +/- 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 24.3495* 03 36 48.29 +10 33 09.3 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
target,2461276.8495,11.43,0.05,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
target 20260824.3495 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 24.3495 2461276.8495 11.45 03:39:47.83 +12:12:26.3
174.55002 -33.30561 galactic Tau Second-epoch detections are separated by 3.2" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:39:47.83 +12:12:26.3 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=0.428+/-0.027 (G)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:39:47.83 +12:12:26.3: 12.92 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:39:47.83 +12:12:26.3: 12.95 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 24.3495* 03 39 47.83 +12 12 26.3 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
target,2461276.8495,11.45,0.05,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
target 20260824.3495 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 24.3495 2461276.8495 11.27 03:31:38.88 +08:57:21.1
175.68351 -37.01010 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 11771238343796352 | 03:31:38.94 +08:57:22.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G4 (LAMOST DR5) J-Ks=0.504+/-0.034 (K)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:31:38.88 +08:57:21.1: 12.85 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:31:38.88 +08:57:21.1: 12.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 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 24.3495* 03 31 38.88 +08 57 21.1 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 11771238343796352,2461276.8495,11.27,0.05,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 11771238343796352 20260824.3495 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 24.3495 2461276.8495 11.47 03:38:04.64 +11:36:25.7
174.71072 -34.02624 galactic Tau Second-epoch detections are separated by 1.2" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 37258227114404480 | 03:38:04.64 +11:36:25.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.766+/-0.030 (K)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:38:04.64 +11:36:25.7: 12.84 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:38:04.64 +11:36:25.7: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 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 24.3495* 03 38 04.64 +11 36 25.7 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
Gaia DR3 37258227114404480,2461276.8495,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 37258227114404480 20260824.3495 11.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 24.3495 2461276.8495 11.54 03:39:42.94 +12:17:37.8
174.45948 -33.25919 galactic Tau Second-epoch detections are separated by 2.7" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 37590412768055040 | 03:39:42.96 +12:17:37.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.781+/-0.028 (K)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:39:42.94 +12:17:37.8: 12.83 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:39:42.94 +12:17:37.8: 12.82 +/- 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 24.3495* 03 39 42.94 +12 17 37.8 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
Gaia DR3 37590412768055040,2461276.8495,11.54,0.05,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
Gaia DR3 37590412768055040 20260824.3495 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 24.3495 2461276.8495 11.40 03:42:05.19 +13:14:11.0
174.14266 -32.18610 galactic Tau Second-epoch detections are separated by 1.6" and 5.6 pix
The object was found in VSX 0" EPIC 210390215
Type: DSCT
# Max. Min./Amp. JD0 Period
12.689 Kp Y 0.006 Kp 0.056197000000
The object was not found in astcheck.
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:42:05.19 +13:14:11.0: 12.81 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:42:05.19 +13:14:11.0: 12.84 +/- 0.01 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 24.3495* 03 42 05.19 +13 14 11.0 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
EPIC 210390215,2461276.8495,11.40,0.05,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
EPIC 210390215 20260824.3495 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 24.3495 2461276.8495 11.38 03:35:19.86 +09:44:17.9
175.77035 -35.81313 galactic Tau Second-epoch detections are separated by 1.7" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:35:19.86 +09:44:17.9 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.506+/-0.033 (K)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:35:19.86 +09:44:17.9: 12.78 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:35:19.86 +09:44:17.9: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 24.3495* 03 35 19.86 +09 44 17.9 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
target,2461276.8495,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260824.3495 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 24.3495 2461276.8495 11.47 03:37:09.95 +10:48:11.3
175.21828 -34.74800 galactic Tau Second-epoch detections are separated by 1.8" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 13146452512422912 | 03:37:09.97 +10:48:11.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.870+/-0.028 (M)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:37:09.95 +10:48:11.3: 12.76 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:37:09.95 +10:48:11.3: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 24.3495* 03 37 09.95 +10 48 11.3 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 13146452512422912,2461276.8495,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 13146452512422912 20260824.3495 11.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 24.3495 2461276.8495 11.09 03:36:55.15 +10:18:02.7
175.60688 -35.14120 galactic Tau Second-epoch detections are separated by 0.6" 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 | target | 03:36:55.15 +10:18:02.7 (user input) | T | P | (position from user input) J-Ks=0.448+/-0.030 (G)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:36:55.15 +10:18:02.7: 12.77 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:36:55.15 +10:18:02.7: 12.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 24.3495* 03 36 55.15 +10 18 02.7 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
target,2461276.8495,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260824.3495 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 24.3495 2461276.8495 11.18 03:32:53.25 +09:03:59.5
175.85040 -36.71331 galactic Tau Second-epoch detections are separated by 0.8" and 5.5 pix
The object was found in VSX 2" Gaia DR3 11768279110707840
Type: ROT
# Max. Min./Amp. JD0 Period
12.170 G 12.200 G K
The object was not found in astcheck.
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:32:53.25 +09:03:59.5: 12.72 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:32:53.25 +09:03:59.5: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 24.3495* 03 32 53.25 +09 03 59.5 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 11768279110707840,2461276.8495,11.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 11768279110707840 20260824.3495 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 24.3495 2461276.8495 11.54 03:36:28.64 +14:34:35.4
171.88559 -32.19041 galactic Tau Second-epoch detections are separated by 2.9" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 41484303135271040 | 03:36:28.62 +14:34:36.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K1 (LAMOST DR5) J-Ks=0.655+/-0.028 (K)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:36:28.64 +14:34:35.4: 12.69 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:36:28.64 +14:34:35.4: 12.68 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.69 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 24.3495* 03 36 28.64 +14 34 35.4 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 41484303135271040,2461276.8495,11.54,0.05,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
Gaia DR3 41484303135271040 20260824.3495 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 24.3495 2461276.8495 11.36 03:34:39.24 +09:53:46.3
175.48740 -35.82312 galactic Tau Second-epoch detections are separated by 4.0" 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 12960149715040768 | 03:34:39.25 +09:53:46.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.772+/-0.030 (K)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:34:39.24 +09:53:46.3: 12.66 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:34:39.24 +09:53:46.3: 12.68 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.67 +/- 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 24.3495* 03 34 39.24 +09 53 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
Gaia DR3 12960149715040768,2461276.8495,11.36,0.05,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 12960149715040768 20260824.3495 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 24.3495 2461276.8495 11.09 03:37:21.04 +10:43:52.6
175.31952 -34.76552 galactic Tau Second-epoch detections are separated by 0.7" and 5.5 pix
The object was found in VSX 1" ASASSN-V J033721.01+104351.9
Type: ROT
# Max. Min./Amp. JD0 Period
13.200 g Y 0.210 g 2459205.59200 2.722000000000
The object was not found in astcheck.
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:37:21.04 +10:43:52.6: 12.63 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:37:21.04 +10:43:52.6: 12.68 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 24.3495* 03 37 21.04 +10 43 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
ASASSN-V J033721.01+104351.9,2461276.8495,11.09,0.05,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
ASASSN-V J033721.01+104351.9 20260824.3495 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 24.3495 2461276.8495 11.35 03:38:44.47 +15:24:01.4
171.67656 -31.21776 galactic Tau Second-epoch detections are separated by 1.2" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 41644346499992448 | 03:38:44.48 +15:24:00.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 (LAMOST DR5) J-Ks=0.460+/-0.029 (G)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:38:44.47 +15:24:01.4: 12.64 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:38:44.47 +15:24:01.4: 12.61 +/- 0.01 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 24.3495* 03 38 44.47 +15 24 01.4 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 41644346499992448,2461276.8495,11.35,0.05,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 41644346499992448 20260824.3495 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 24.3495 2461276.8495 11.22 03:40:19.44 +12:20:15.2
174.54658 -33.12252 galactic Tau Second-epoch detections are separated by 1.9" and 5.4 pix
The object was found in VSX 2" ASAS J034019+1220.4
Type: ROT
# Max. Min./Amp. JD0 Period
12.624 V Y 0.080 Ic 0.554720000000 K0V
The object was not found in astcheck.
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:40:19.44 +12:20:15.2: 12.64 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:40:19.44 +12:20:15.2: 12.60 +/- 0.01 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 24.3495* 03 40 19.44 +12 20 15.2 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
ASAS J034019+1220.4,2461276.8495,11.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J034019+1220.4 20260824.3495 11.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 24.3495 2461276.8495 11.29 03:40:08.92 +12:10:21.6
174.65153 -33.26850 galactic Tau Second-epoch detections are separated by 2.2" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 37397968170526848 | 03:40:08.95 +12:10:22.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.463+/-0.028 (G)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:40:08.92 +12:10:21.6: 12.62 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:40:08.92 +12:10:21.6: 12.64 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 24.3495* 03 40 08.92 +12 10 21.6 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 37397968170526848,2461276.8495,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 37397968170526848 20260824.3495 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 24.3495 2461276.8495 11.38 03:30:44.60 +08:57:32.6
175.48520 -37.16789 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 12431632515257216 | 03:30:44.65 +08:57:33.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5) J-Ks=0.711+/-0.035 (K)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:30:44.60 +08:57:32.6: 12.61 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:30:44.60 +08:57:32.6: 12.61 +/- 0.01 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 24.3495* 03 30 44.60 +08 57 32.6 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 12431632515257216,2461276.8495,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 12431632515257216 20260824.3495 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 24.3495 2461276.8495 11.31 03:38:30.66 +15:12:47.0
171.78202 -31.39112 galactic Tau Second-epoch detections are separated by 1.8" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 41605313836622976 | 03:38:30.70 +15:12:47.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.661+/-0.028 (K)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:38:30.66 +15:12:47.0: 12.57 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:38:30.66 +15:12:47.0: 12.58 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.58 +/- 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 24.3495* 03 38 30.66 +15 12 47.0 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 41605313836622976,2461276.8495,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 41605313836622976 20260824.3495 11.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 24.3495 2461276.8495 11.21 03:33:11.85 +09:18:13.7
175.70430 -36.49331 galactic Tau Second-epoch detections are separated by 2.4" 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 11808067687549568 | 03:33:11.75 +09:18:13.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5) J-Ks=0.741+/-0.035 (K)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:33:11.85 +09:18:13.7: 12.56 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:33:11.85 +09:18:13.7: 12.55 +/- 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 24.3495* 03 33 11.85 +09 18 13.7 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
Gaia DR3 11808067687549568,2461276.8495,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 11808067687549568 20260824.3495 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 24.3495 2461276.8495 11.18 03:38:10.35 +11:30:23.6
174.81711 -34.07999 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 | Gaia DR3 37252450381467392 | 03:38:10.33 +11:30:23.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 (LAMOST DR5) J-Ks=0.429+/-0.033 (G)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:38:10.35 +11:30:23.6: 12.52 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:38:10.35 +11:30:23.6: 12.47 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 24.3495* 03 38 10.35 +11 30 23.6 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 37252450381467392,2461276.8495,11.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 37252450381467392 20260824.3495 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 24.3495 2461276.8495 11.12 03:40:45.52 +12:21:21.7
174.61946 -33.03375 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 37612196842179200 | 03:40:45.54 +12:21:21.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:40:45.52 +12:21:21.7: 12.46 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:40:45.52 +12:21:21.7: 12.50 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.48 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 24.3495* 03 40 45.52 +12 21 21.7 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 37612196842179200,2461276.8495,11.12,0.05,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 37612196842179200 20260824.3495 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 24.3495 2461276.8495 11.23 03:37:58.54 +11:27:04.8
174.82402 -34.15308 galactic Tau Second-epoch detections are separated by 0.3" 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 37251561325170688 | 03:37:58.50 +11:27:05.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.444+/-0.032 (G)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:37:58.54 +11:27:04.8: 12.46 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:37:58.54 +11:27:04.8: 12.44 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.45 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 24.3495* 03 37 58.54 +11 27 04.8 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 37251561325170688,2461276.8495,11.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 37251561325170688 20260824.3495 11.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 24.3495 2461276.8495 11.33 03:42:06.19 +13:27:27.9
173.95994 -32.02779 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 38111649999196416 | 03:42:06.17 +13:27:27.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5) J-Ks=0.489+/-0.026 (K)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:42:06.19 +13:27:27.9: 12.43 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:42:06.19 +13:27:27.9: 12.43 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.43 +/- 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 24.3495* 03 42 06.19 +13 27 27.9 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 38111649999196416,2461276.8495,11.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 38111649999196416 20260824.3495 11.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 24.3495 2461276.8495 11.33 03:42:03.35 +17:02:31.2
171.02203 -29.48313 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 44157696938555520 | 03:42:03.33 +17:02:30.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.419+/-0.027 (G)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:42:03.35 +17:02:31.2: 12.38 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:42:03.35 +17:02:31.2: 12.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.39 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 24.3495* 03 42 03.35 +17 02 31.2 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 44157696938555520,2461276.8495,11.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 44157696938555520 20260824.3495 11.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 24.3495 2461276.8495 11.37 03:41:32.79 +17:17:41.6
170.72032 -29.38460 galactic Tau Second-epoch detections are separated by 1.2" and 5.4 pix
The object was found in VSX 1" EPIC 210623357
Type: VAR
# Max. Min./Amp. JD0 Period
11.922 Kp Y 0.004 Kp 8.762909000000
The object was not found in astcheck.
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:41:32.79 +17:17:41.6: 12.33 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:41:32.79 +17:17:41.6: 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 24.3495* 03 41 32.79 +17 17 41.6 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
EPIC 210623357,2461276.8495,11.37,0.05,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
EPIC 210623357 20260824.3495 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 24.3495 2461276.8495 11.01 03:36:47.49 +10:36:56.5
175.30392 -34.94460 galactic Tau Second-epoch detections are separated by 1.9" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:36:47.49 +10:36:56.5 (user input) | T | P | (position from user input) J-Ks=0.448+/-0.033 (G)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:36:47.49 +10:36:56.5: 12.31 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:36:47.49 +10:36:56.5: 12.32 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.31 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 24.3495* 03 36 47.49 +10 36 56.5 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
target,2461276.8495,11.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260824.3495 11.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 24.3495 2461276.8495 11.17 03:36:46.49 +10:38:01.4
175.28467 -34.93497 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 13118307591084800 | 03:36:46.47 +10:38:01.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F6 (LAMOST DR5) J-Ks=0.424+/-0.031 (G)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:36:46.49 +10:38:01.4: 12.30 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:36:46.49 +10:38:01.4: 12.31 +/- 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 24.3495* 03 36 46.49 +10 38 01.4 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 13118307591084800,2461276.8495,11.17,0.05,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 13118307591084800 20260824.3495 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 24.3495 2461276.8495 11.18 03:40:54.91 +12:34:20.7
174.46710 -32.85505 galactic Tau Second-epoch detections are separated by 0.8" and 5.6 pix
The object was found in VSX 1" EPIC 210363145
Type: VAR
# Max. Min./Amp. JD0 Period
11.896 Kp Y 0.029 Kp 19.716550000000
The object was not found in astcheck.
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:40:54.91 +12:34:20.7: 12.18 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:40:54.91 +12:34:20.7: 12.19 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.19 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 24.3495* 03 40 54.91 +12 34 20.7 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
EPIC 210363145,2461276.8495,11.18,0.05,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
EPIC 210363145 20260824.3495 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 24.3495 2461276.8495 11.14 03:36:28.91 +10:41:33.8
175.17185 -34.94539 galactic Tau Second-epoch detections are separated by 1.6" 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 13121881003778560 | 03:36:28.91 +10:41:34.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5) J-Ks=0.387+/-0.033 (G)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:36:28.91 +10:41:33.8: 12.15 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:36:28.91 +10:41:33.8: 12.13 +/- 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 24.3495* 03 36 28.91 +10 41 33.8 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 13121881003778560,2461276.8495,11.14,0.05,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
Gaia DR3 13121881003778560 20260824.3495 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 24.3495 2461276.8495 10.99 03:38:44.68 +15:22:30.4
171.69779 -31.23537 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 41642598449980800 | 03:38:44.69 +15:22:31.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.777+/-0.029 (K)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:38:44.68 +15:22:30.4: 12.15 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:38:44.68 +15:22:30.4: 12.12 +/- 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 24.3495* 03 38 44.68 +15 22 30.4 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 41642598449980800,2461276.8495,10.99,0.05,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 41642598449980800 20260824.3495 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 24.3495 2461276.8495 11.07 03:38:15.43 +11:43:54.2
174.64071 -33.90754 galactic Tau Second-epoch detections are separated by 1.1" and 5.5 pix
The object was found in VSX 2" Gaia DR3 37283584601313536
Type: ROT
# Max. Min./Amp. JD0 Period
11.780 G 11.820 G K
The object was not found in astcheck.
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:38:15.43 +11:43:54.2: 12.04 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:38:15.43 +11:43:54.2: 12.06 +/- 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 24.3495* 03 38 15.43 +11 43 54.2 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 37283584601313536,2461276.8495,11.07,0.05,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 37283584601313536 20260824.3495 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 24.3495 2461276.8495 10.54 03:37:55.28 +10:46:30.7
175.39983 -34.63432 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 | Gaia DR3 13132330659997056 | 03:37:55.29 +10:46:31.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.448+/-0.030 (G)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:37:55.28 +10:46:30.7: 11.97 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:37:55.28 +10:46:30.7: 11.98 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.97 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 24.3495* 03 37 55.28 +10 46 30.7 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 13132330659997056,2461276.8495,10.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 13132330659997056 20260824.3495 10.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 24.3495 2461276.8495 10.92 03:38:14.69 +15:20:43.1
171.62042 -31.34043 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 41645171133715072 | 03:38:14.68 +15:20:43.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5) J-Ks=0.417+/-0.028 (G)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:38:14.69 +15:20:43.1: 11.95 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:38:14.69 +15:20:43.1: 11.95 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.95 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 24.3495* 03 38 14.69 +15 20 43.1 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 41645171133715072,2461276.8495,10.92,0.05,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 41645171133715072 20260824.3495 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 24.3495 2461276.8495 10.96 03:38:29.52 +15:36:50.6
171.45292 -31.10536 galactic Tau Second-epoch detections are separated by 0.8" and 5.4 pix
The object was found in VSX 1" EPIC 210512162
Type: EA
# Max. Min./Amp. JD0 Period
11.600 Kp Y 0.100 Kp 2457064.40350 4.110298280000
The object was not found in astcheck.
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:38:29.52 +15:36:50.6: 11.90 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:38:29.52 +15:36:50.6: 11.91 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.91 +/- 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 24.3495* 03 38 29.52 +15 36 50.6 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
EPIC 210512162,2461276.8495,10.96,0.05,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
EPIC 210512162 20260824.3495 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 24.3495 2461276.8495 10.83 03:34:50.40 +09:49:04.0
175.59617 -35.84485 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 | Gaia DR3 12208221200583552 | 03:34:50.42 +09:49:03.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.894+/-0.034 (M)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:34:50.40 +09:49:04.0: 11.83 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:34:50.40 +09:49:04.0: 11.84 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.83 +/- 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 24.3495* 03 34 50.40 +09 49 04.0 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 12208221200583552,2461276.8495,10.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 12208221200583552 20260824.3495 10.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 24.3495 2461276.8495 10.70 03:40:18.68 +12:06:18.1
174.74263 -33.28736 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 37390752625470336 | 03:40:18.69 +12:06:18.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.819+/-0.028 (M)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:40:18.68 +12:06:18.1: 11.80 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:40:18.68 +12:06:18.1: 11.82 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.81 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 24.3495* 03 40 18.68 +12 06 18.1 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 37390752625470336,2461276.8495,10.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 37390752625470336 20260824.3495 10.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 24.3495 2461276.8495 10.66 03:38:06.35 +11:32:01.4
174.77988 -34.07265 galactic Tau Second-epoch detections are separated by 1.2" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 37253279310249600 | 03:38:06.37 +11:32:02.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.429+/-0.029 (G)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:38:06.35 +11:32:01.4: 11.69 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:38:06.35 +11:32:01.4: 11.70 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.69 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 24.3495* 03 38 06.35 +11 32 01.4 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 37253279310249600,2461276.8495,10.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 37253279310249600 20260824.3495 10.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 24.3495 2461276.8495 10.48 03:35:08.70 +09:46:03.4
175.70509 -35.82574 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 12206885466392192 | 03:35:08.67 +09:46:03.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5) J-Ks=0.366+/-0.034 (G)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:35:08.70 +09:46:03.4: 11.45 +/- 0.00 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:35:08.70 +09:46:03.4: 11.43 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.44 +/- 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 24.3495* 03 35 08.70 +09 46 03.4 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 12206885466392192,2461276.8495,10.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 12206885466392192 20260824.3495 10.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 24.3495 2461276.8495 10.36 03:38:19.02 +11:09:07.0
175.15387 -34.30227 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 37178753039655552 | 03:38:19.06 +11:09:07.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.471+/-0.031 (K)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:38:19.02 +11:09:07.0: 11.43 +/- 0.00 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:38:19.02 +11:09:07.0: 11.44 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.43 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 24.3495* 03 38 19.02 +11 09 07.0 10.4 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 37178753039655552,2461276.8495,10.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 37178753039655552 20260824.3495 10.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 24.3495 2461276.8495 10.29 03:37:43.95 +11:13:37.7
174.96752 -34.35245 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 | Gaia DR3 37229639812106624 | 03:37:43.95 +11:13:37.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.850+/-0.031 (M)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:37:43.95 +11:13:37.7: 11.24 +/- 0.00 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:37:43.95 +11:13:37.7: 11.24 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.24 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 24.3495* 03 37 43.95 +11 13 37.7 10.3 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 37229639812106624,2461276.8495,10.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 37229639812106624 20260824.3495 10.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 24.3495 2461276.8495 10.22 03:33:44.01 +09:13:09.4
175.89420 -36.45699 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 11794637325648896 | 03:33:43.99 +09:13:09.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.589+/-0.033 (K)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:33:44.01 +09:13:09.4: 11.17 +/- 0.00 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:33:44.01 +09:13:09.4: 11.17 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.17 +/- 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 24.3495* 03 33 44.01 +09 13 09.4 10.2 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 11794637325648896,2461276.8495,10.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 11794637325648896 20260824.3495 10.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 24.3495 2461276.8495 10.23 03:36:36.14 +10:10:18.3
175.65420 -35.28687 galactic Tau Second-epoch detections are separated by 0.2" 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 12244028343542656 | 03:36:36.15 +10:10:18.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.404+/-0.030 (G)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:36:36.14 +10:10:18.3: 11.09 +/- 0.00 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:36:36.14 +10:10:18.3: 11.13 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.11 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 24.3495* 03 36 36.14 +10 10 18.3 10.2 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 12244028343542656,2461276.8495,10.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 12244028343542656 20260824.3495 10.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 24.3495 2461276.8495 9.99 03:37:45.28 +10:46:49.0
175.36077 -34.66018 galactic Tau Second-epoch detections are separated by 1.5" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 13144184769735168 | 03:37:45.30 +10:46:49.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A5 1958PMcCO..13b....V AG+10 365 J-Ks=0.264+/-0.030 (F)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:37:45.28 +10:46:49.0: 11.03 +/- 0.00 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:37:45.28 +10:46:49.0: 11.04 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.03 +/- 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 24.3495* 03 37 45.28 +10 46 49.0 10.0 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 13144184769735168,2461276.8495,9.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 13144184769735168 20260824.3495 9.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 24.3495 2461276.8495 9.96 03:38:29.79 +11:27:00.7
174.93276 -34.06263 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 37239324961411712 | 03:38:29.79 +11:27:00.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.861+/-0.024 (M)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:38:29.79 +11:27:00.7: 10.86 +/- 0.00 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:38:29.79 +11:27:00.7: 10.87 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.87 +/- 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 24.3495* 03 38 29.79 +11 27 00.7 10.0 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 37239324961411712,2461276.8495,9.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 37239324961411712 20260824.3495 9.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 24.3495 2461276.8495 11.69 03:36:40.89 +10:23:33.8
175.47636 -35.11927 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 | target | 03:36:40.89 +10:23:33.8 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.816+/-0.031 (M)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:36:40.89 +10:23:33.8: 13.87 +/- 0.04 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:36:40.89 +10:23:33.8: 13.86 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.87 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 24.3495* 03 36 40.89 +10 23 33.8 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,2461276.8495,11.69,0.05,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 20260824.3495 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.67169814 09.01.2026 04:07:04.719 /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
First image: 2461049.67169814 09.01.2026 04:07:04.719 /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
Last image: 2461276.84978968 24.08.2026 08:23:31.828 /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.54
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: 4 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): 7290
Objects passed selection criteria: 7232
Measurements per detected object (mean, median, min, max): 2.0 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.0 2.0 2 4
Average stars detected per image: 3895
Average stars matched: 3796.25 (97.4647 %)
Memory usage VmPeak: 238900 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Aug 20 15:05:04 CDT 2026
VaST build number 1.0rc89-192-g23359006
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-20)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Aug 24 03:34:21 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: 2461049.67169814 09.01.2026 04:07:04.719 /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
First image: 2461049.67169814 09.01.2026 04:07:04.719 /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
Last image: 2461276.84978968 24.08.2026 08:23:31.828 /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 85
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.25
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: 13 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): 44751
Objects passed selection criteria: 44564
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: 24755.8
Average stars matched: 23861 (96.3857 %)
Memory usage VmPeak: 267440 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Aug 20 15:05:04 CDT 2026
VaST build number 1.0rc89-192-g23359006
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-20)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Aug 24 03:36:19 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-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits
SExtractor catalog cache: saved Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.cat to cache
SExtractor catalog cache: saved Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.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-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.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: 2461276.84922612
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-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits exists and is non-empty
wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits exists and is non-empty
wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits exists and is non-empty
wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits (1st reference image)
verification OK: wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.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: 03:33:20.383 +13:59:53.59 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-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits (1st new image)
verification OK: wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.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: 03:33:05.894 +13:58:18.17 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 03:33:20.383 +13:59:53.59
Second-epoch image center 03:33:05.894 +13:58:18.17
Angular distance between the image centers 0.0643 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits (2nd new image)
verification OK: wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits
Image size: 941.4'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: 03:33:05.606 +13:57:46.30 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 03:33:20.383 +13:59:53.59
Second-epoch image center 03:33:05.606 +13:57:46.30
Angular distance between the image centers 0.0694 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 03:33:05.894 +13:58:18.17
Second-epoch second image center 03:33:05.606 +13:57:46.30
Angular distance between the image centers 0.00893 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits &> /tmp/tmp.qd14yeHnuP
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits &> /tmp/tmp.Q0oh0vEMw1
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits &> /tmp/tmp.QKRG2glDjR
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits &> /tmp/tmp.S3FbLanfP6
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.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-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits and wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.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-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits and wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat
Found non-empty wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits and wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat
The reference image (wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits) and catalog (wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat) found
'wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat' -> 'wcsmag.cat'
Read 7716 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 45.0636 to 61.6428 deg, Dec +8.6205 to +19.2872 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 45.0636 to 61.6428 deg, Dec 8.6205 to 19.2872 deg
Loaded 4361 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): 3534 out of 3742 total matches.
Matched with Tycho-2 3742 out of 7716 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.950750
a=0.000000 b=1.000000 c=22.950750
From vast_summary.log: estimated ref. image limiting mag.: -7.54
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.41
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.41
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 7716 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 45.0636 to 61.6428 deg, Dec +8.6205 to +19.2872 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 45.0636 to 61.6428 deg, Dec 8.6205 to 19.2872 deg
Loaded 4361 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): 3534 out of 3742 total matches.
Matched with Tycho-2 3742 out of 7716 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
Forced-photometry filter: calibrated wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits -> calib.txt_param_ref_wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits (aperture=6.0)
Read 7722 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 45.0650 to 61.6427 deg, Dec +8.6182 to +19.2791 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 45.0650 to 61.6427 deg, Dec 8.6182 to 19.2791 deg
Loaded 4354 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): 3534 out of 3736 total matches.
Matched with Tycho-2 3736 out of 7722 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
Forced-photometry filter: calibrated wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits -> calib.txt_param_ref_wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits (aperture=6.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
2.0 pix Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
2.4 pix fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits
2.4 pix fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits
Limiting magnitude estimates:
15.4 mag. Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
15.4 mag. Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
11.5 mag. fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits
10.6 mag. fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits
All-image limiting magnitude estimate: 10.6 (SNR ) 9.2 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.qd14yeHnuP (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_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.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-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits' -> 'wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.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-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
WCS_IMAGE_NAME=wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
WCS-calibrated image found: wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
Checking if the catalog wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat corresponding to the image wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits alredy exist and is non-empty...
Catalog wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat corresponding to the image wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
WCS catalog name: wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.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=551, bad_region=0, passed=7716
Got 7716 stars (including 7157 good ones) from the SExtractor catalog wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat
util/solve_plate_with_UCAC5 got 7716 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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4903 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4895 matched stars entering correct_measured_positions(), 4895 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4895 matched stars entering correct_measured_positions(), 7716 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4903 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4895 matched stars entering correct_measured_positions(), 7716 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 4895 matched stars entering correct_measured_positions(), 7716 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 4895 stars left (next iteration limit 5384)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits N_match=4895 sigma_overall_arcsec=0.305 sigma_q1_arcsec=0.404 sigma_q2_arcsec=0.301 sigma_q3_arcsec=0.272 sigma_q4_arcsec=0.248 n_q1=1380 n_q2=1359 n_q3=1203 n_q4=953 worst_quadrant_to_overall_ratio=1.327
The image catalog is written to wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits -region wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.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.Q0oh0vEMw1 (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_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.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-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits' -> 'wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.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-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
WCS_IMAGE_NAME=wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
WCS-calibrated image found: wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
Checking if the catalog wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat corresponding to the image wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits alredy exist and is non-empty...
Catalog wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat corresponding to the image wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
WCS catalog name: wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.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=536, bad_region=0, passed=7722
Got 7722 stars (including 7177 good ones) from the SExtractor catalog wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat
util/solve_plate_with_UCAC5 got 7722 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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4908 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4900 matched stars entering correct_measured_positions(), 4900 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4900 matched stars entering correct_measured_positions(), 7722 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4908 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4900 matched stars entering correct_measured_positions(), 7722 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 4900 matched stars entering correct_measured_positions(), 7722 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 4900 stars left (next iteration limit 5390)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits N_match=4900 sigma_overall_arcsec=0.307 sigma_q1_arcsec=0.403 sigma_q2_arcsec=0.295 sigma_q3_arcsec=0.260 sigma_q4_arcsec=0.260 n_q1=1378 n_q2=1355 n_q3=1207 n_q4=960 worst_quadrant_to_overall_ratio=1.311
The image catalog is written to wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits -region wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.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.QKRG2glDjR (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_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.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_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits
WCS_IMAGE_NAME=wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits
WCS-calibrated image found: wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits
Checking if the catalog wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits.wcscat corresponding to the image wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits.wcscat corresponding to the image wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits
WCS catalog name: wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.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=5, bad_region=0, passed=143
Got 143 stars (including 137 good ones) from the SExtractor catalog wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits.wcscat
util/solve_plate_with_UCAC5 got 143 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 493 to 548 (Dec 8.7 to 19.4)
Done reading UCAC5 zone files...
Matched 120 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 120 matched stars entering correct_measured_positions(), 59 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.95"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 120 matched stars entering correct_measured_positions(), 61 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.95"
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 493 to 548 (Dec 8.7 to 19.4)
Done reading UCAC5 zone files...
Matched 119 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 119 matched stars entering correct_measured_positions(), 63 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.15"
Accuracy estimation diagnostic: 119 matched stars entering correct_measured_positions(), 63 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.17"
Excluding outliers - 119 stars left (next iteration limit 132)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=119 robust_rms=5.231 arcsec worst_quadrant_rms=8.735 arcsec
SIP_REFIT: SIP order 3 trial: matched=119 robust_rms=0.343 arcsec worst_quadrant_rms=0.364 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=119 robust_rms_before=1.147 arcsec robust_rms_before_corrected=1.067 arcsec robust_rms_after=0.343 arcsec worst_quadrant_rms_before=1.265 worst_quadrant_rms_after=0.364
verification OK: wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits
verification OK: wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits
Image size: 941.3'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: 03:33:05.908 +13:58:17.28 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 143 stars ###
'wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/correct_sextractor_wcs_catalog_usingxy2sky1074499.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 3, robust RMS 1.147 -> 0.343 arcsec)
WCS_QUALITY_DIAG: file=fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits N_match=119 sigma_overall_arcsec=0.368 sigma_q1_arcsec=0.445 sigma_q2_arcsec=0.286 sigma_q3_arcsec=0.387 sigma_q4_arcsec=0.424 n_q1=17 n_q2=36 n_q3=27 n_q4=39 worst_quadrant_to_overall_ratio=1.210
The image catalog is written to wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits -region wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.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.S3FbLanfP6 (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_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.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_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits
WCS_IMAGE_NAME=wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits
WCS-calibrated image found: wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits
Checking if the catalog wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits.wcscat corresponding to the image wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits.wcscat corresponding to the image wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits found.
The catalog seems suspiciously small (only 87 lines), re-generating the catalog with SExtractor...
ok
Catalog wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits.wcscat corresponding to the image wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits created.
verification OK: wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits
verification OK: wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits
Image size: 941.4'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: 03:33:05.606 +13:57:46.30 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 87 stars ###
'wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/correct_sextractor_wcs_catalog_usingxy2sky1088765.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits
WCS catalog name: wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.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=3, bad_region=0, passed=87
Got 87 stars (including 84 good ones) from the SExtractor catalog wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits.wcscat
util/solve_plate_with_UCAC5 got 87 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 493 to 548 (Dec 8.8 to 19.4)
Done reading UCAC5 zone files...
Matched 71 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 71 matched stars entering correct_measured_positions(), 36 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 71 matched stars entering correct_measured_positions(), 37 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
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 493 to 548 (Dec 8.8 to 19.4)
Done reading UCAC5 zone files...
Matched 71 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 71 matched stars entering correct_measured_positions(), 37 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Accuracy estimation diagnostic: 71 matched stars entering correct_measured_positions(), 37 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Excluding outliers - 71 stars left (next iteration limit 78)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: only 71 catalog matches (<100) - keeping the original solution
WCS_QUALITY_DIAG: file=fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits N_match=71 sigma_overall_arcsec=0.582 sigma_q1_arcsec=0.440 sigma_q2_arcsec=0.370 sigma_q3_arcsec=0.473 sigma_q4_arcsec=0.765 n_q1=11 n_q2=19 n_q3=16 n_q4=25 worst_quadrant_to_overall_ratio=1.315
The image catalog is written to wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits -region wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Saving the final (post-refit) wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits to local_wcs_cache/
'wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits' -> 'local_wcs_cache/wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits'
Saving the final (post-refit) wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits to local_wcs_cache/
'wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits' -> 'local_wcs_cache/wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits'
Saving the final (post-refit) wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits to local_wcs_cache/
'wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits' -> 'local_wcs_cache/wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits'
Saving the final (post-refit) wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits to local_wcs_cache/
'wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits' -> 'local_wcs_cache/wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits sigma_overall=0.305 worst_q_ratio=1.327
ref2=Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits sigma_overall=0.307 worst_q_ratio=1.311
new1=fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits sigma_overall=0.368 worst_q_ratio=1.210
new2=fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits sigma_overall=0.582 worst_q_ratio=1.315
reference average sigma_overall=0.306 worst_q_ratio=1.319
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_astrometric_residuals.png (4895 matched stars from wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_astrometric_residuals.png (4900 matched stars from wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374_astrometric_residuals.png (119 matched stars from wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.29 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375_astrometric_residuals.png (71 matched stars from wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.42 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits'
Saving fully-calibrated image wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits'
Preparing the HTML report for the field Tau-05-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Tau-05-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits
SExtractor catalog cache: saved Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.cat to cache
SExtractor catalog cache: saved Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
Creating symlink local_wcs_cache/wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits
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
Plate-solving the images
wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits exists and is non-empty
wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits exists and is non-empty
wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits exists and is non-empty
wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits (1st reference image)
verification OK: wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.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: 03:33:20.383 +13:59:53.59 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-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits (1st new image)
verification OK: wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits
Image size: 941.3'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: 03:33:05.908 +13:58:17.28 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 03:33:20.383 +13:59:53.59
Second-epoch image center 03:33:05.908 +13:58:17.28
Angular distance between the image centers 0.0644 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits (2nd new image)
verification OK: wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits
Image size: 941.4'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: 03:33:05.606 +13:57:46.30 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 03:33:20.383 +13:59:53.59
Second-epoch image center 03:33:05.606 +13:57:46.30
Angular distance between the image centers 0.0694 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 03:33:05.908 +13:58:17.28
Second-epoch second image center 03:33:05.606 +13:57:46.30
Angular distance between the image centers 0.00869 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-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits &> /tmp/tmp.0ymh92q2kP
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits &> /tmp/tmp.XRlvD0Cskv
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits &> /tmp/tmp.wjjlfPKrBi
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits &> /tmp/tmp.0mCKABs7QO
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.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-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits and wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.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-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits and wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat
Found non-empty wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits and wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat
The reference image (wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits) and catalog (wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat) found
'wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat' -> 'wcsmag.cat'
Read 48584 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 45.0636 to 61.6458 deg, Dec +8.6191 to +19.2871 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 45.0636 to 61.6458 deg, Dec 8.6191 to 19.2871 deg
Loaded 4361 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): 3309 out of 3760 total matches.
Matched with Tycho-2 3760 out of 48584 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.830300
a=0.000000 b=1.000000 c=22.830300
From vast_summary.log: estimated ref. image limiting mag.: -7.25
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.58
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.58
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 48584 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 45.0636 to 61.6458 deg, Dec +8.6191 to +19.2871 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 45.0636 to 61.6458 deg, Dec 8.6191 to 19.2871 deg
Loaded 4361 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): 3309 out of 3760 total matches.
Matched with Tycho-2 3760 out of 48584 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
Forced-photometry filter: calibrated wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits -> calib.txt_param_ref_wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits (aperture=4.6)
Read 48560 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 45.0650 to 61.6548 deg, Dec +8.6183 to +19.2794 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 45.0650 to 61.6548 deg, Dec 8.6183 to 19.2794 deg
Loaded 4358 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): 3320 out of 3753 total matches.
Matched with Tycho-2 3753 out of 48560 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
Forced-photometry filter: calibrated wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits -> calib.txt_param_ref_wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits (aperture=4.6)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 81 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.9 pix Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
1.9 pix Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
2.3 pix fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits
2.3 pix fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits
Limiting magnitude estimates:
15.6 mag. Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
15.6 mag. Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
11.9 mag. fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits
11.6 mag. fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits
All-image limiting magnitude estimate: 11.6 (SNR ) 11.6 (80% of stars) with default.sex.telephoto_lens_vSTL
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.0ymh92q2kP (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_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.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-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits' -> 'wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.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-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
WCS_IMAGE_NAME=wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
WCS-calibrated image found: wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
Checking if the catalog wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat corresponding to the image wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits alredy exist and is non-empty...
Catalog wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat corresponding to the image wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
WCS catalog name: wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.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=16, blended=2222, bad_region=4, passed=48568
Got 48568 stars (including 46270 good ones) from the SExtractor catalog wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat
util/solve_plate_with_UCAC5 got 48568 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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4904 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4898 matched stars entering correct_measured_positions(), 4898 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4898 matched stars entering correct_measured_positions(), 48568 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4904 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4898 matched stars entering correct_measured_positions(), 48568 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 4898 matched stars entering correct_measured_positions(), 48568 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 4898 stars left (next iteration limit 5387)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits N_match=4898 sigma_overall_arcsec=0.295 sigma_q1_arcsec=0.387 sigma_q2_arcsec=0.289 sigma_q3_arcsec=0.266 sigma_q4_arcsec=0.252 n_q1=1362 n_q2=1350 n_q3=1192 n_q4=994 worst_quadrant_to_overall_ratio=1.312
The image catalog is written to wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits -region wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.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.XRlvD0Cskv (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_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.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-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits' -> 'wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.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-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
WCS_IMAGE_NAME=wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
WCS-calibrated image found: wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
Checking if the catalog wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat corresponding to the image wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits alredy exist and is non-empty...
Catalog wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat corresponding to the image wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
WCS catalog name: wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.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=16, blended=2192, bad_region=5, passed=48544
Got 48544 stars (including 46257 good ones) from the SExtractor catalog wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat
util/solve_plate_with_UCAC5 got 48544 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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4905 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4898 matched stars entering correct_measured_positions(), 4898 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4898 matched stars entering correct_measured_positions(), 48544 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4905 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4899 matched stars entering correct_measured_positions(), 48544 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 4899 matched stars entering correct_measured_positions(), 48544 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 4899 stars left (next iteration limit 5387)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits N_match=4899 sigma_overall_arcsec=0.297 sigma_q1_arcsec=0.379 sigma_q2_arcsec=0.293 sigma_q3_arcsec=0.255 sigma_q4_arcsec=0.256 n_q1=1361 n_q2=1351 n_q3=1201 n_q4=986 worst_quadrant_to_overall_ratio=1.274
The image catalog is written to wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits -region wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.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.wjjlfPKrBi (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_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.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_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits
WCS_IMAGE_NAME=wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits
WCS-calibrated image found: wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits
Checking if the catalog wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits.wcscat corresponding to the image wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits.wcscat corresponding to the image wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits
WCS catalog name: wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.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=17, bad_region=0, passed=1528
Got 1528 stars (including 1507 good ones) from the SExtractor catalog wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits.wcscat
util/solve_plate_with_UCAC5 got 1528 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 493 to 549 (Dec 8.6 to 19.5)
Done reading UCAC5 zone files...
Matched 1431 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1426 matched stars entering correct_measured_positions(), 1395 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.93"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1426 matched stars entering correct_measured_positions(), 1486 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.93"
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 493 to 549 (Dec 8.6 to 19.5)
Done reading UCAC5 zone files...
Matched 1431 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1426 matched stars entering correct_measured_positions(), 1486 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.95"
Accuracy estimation diagnostic: 1426 matched stars entering correct_measured_positions(), 1486 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.95"
Excluding outliers - 1426 stars left (next iteration limit 1568)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=1426 robust_rms=5.006 arcsec worst_quadrant_rms=8.699 arcsec
SIP_REFIT: SIP order 3 trial: matched=1426 robust_rms=0.959 arcsec worst_quadrant_rms=1.116 arcsec
SIP_REFIT: SIP order 5 trial: matched=1426 robust_rms=0.934 arcsec worst_quadrant_rms=0.988 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=1426 robust_rms_before=1.004 arcsec robust_rms_before_corrected=0.980 arcsec robust_rms_after=0.934 arcsec worst_quadrant_rms_before=1.078 worst_quadrant_rms_after=0.988
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 1.078 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits N_match=1426 sigma_overall_arcsec=0.911 sigma_q1_arcsec=1.004 sigma_q2_arcsec=0.897 sigma_q3_arcsec=0.896 sigma_q4_arcsec=0.862 n_q1=208 n_q2=408 n_q3=280 n_q4=530 worst_quadrant_to_overall_ratio=1.102
The image catalog is written to wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits -region wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.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.0mCKABs7QO (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_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.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_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits
WCS_IMAGE_NAME=wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits
WCS-calibrated image found: wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits
Checking if the catalog wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits.wcscat corresponding to the image wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits.wcscat corresponding to the image wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits
WCS catalog name: wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.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=8, bad_region=0, passed=945
Got 945 stars (including 934 good ones) from the SExtractor catalog wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits.wcscat
util/solve_plate_with_UCAC5 got 945 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 493 to 549 (Dec 8.6 to 19.5)
Done reading UCAC5 zone files...
Matched 875 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 871 matched stars entering correct_measured_positions(), 832 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.89"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 871 matched stars entering correct_measured_positions(), 896 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.89"
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 493 to 549 (Dec 8.6 to 19.5)
Done reading UCAC5 zone files...
Matched 875 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 871 matched stars entering correct_measured_positions(), 897 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.94"
Accuracy estimation diagnostic: 871 matched stars entering correct_measured_positions(), 897 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.94"
Excluding outliers - 871 stars left (next iteration limit 958)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=871 robust_rms=4.662 arcsec worst_quadrant_rms=6.377 arcsec
SIP_REFIT: SIP order 3 trial: matched=871 robust_rms=0.950 arcsec worst_quadrant_rms=0.993 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=871 robust_rms_before=1.410 arcsec robust_rms_before_corrected=0.966 arcsec robust_rms_after=0.950 arcsec worst_quadrant_rms_before=1.124 worst_quadrant_rms_after=0.993
SIP_REFIT: applied the refit solution to the output catalog positions only (order 3, robust RMS 1.410 -> 0.950 arcsec); the image header was NOT rewritten as wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits is a symbolic link
WCS_QUALITY_DIAG: file=fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits N_match=871 sigma_overall_arcsec=0.870 sigma_q1_arcsec=0.816 sigma_q2_arcsec=0.843 sigma_q3_arcsec=0.928 sigma_q4_arcsec=0.885 n_q1=158 n_q2=227 n_q3=217 n_q4=269 worst_quadrant_to_overall_ratio=1.067
The image catalog is written to wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits -region wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-22-43_20.00sec_-0.00C_LIGHTs_0374.fits
Saving fully-calibrated image wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Tau-05-Q1b1x1_033136_TTUQ1b1x1_963336_Tik0JLRo/wcs_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375.fits
Preparing the HTML report for the field Tau-05-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:36:30.64 +14:41:35.9: 11.80 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:41:11.96 +12:31:30.5: 12.48 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:38:15.64 +11:29:00.0: 12.09 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:33:45.06 +09:19:38.8: 12.53 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:43:16.67 +17:34:21.6: 12.02 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:38:07.41 +11:06:21.3: 12.11 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:39:06.56 +15:36:07.4: 12.55 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:42:17.82 +13:30:49.1: 12.37 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:30:43.05 +09:00:26.2: 12.63 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:42:40.46 +13:08:33.4: 11.64 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:36:30.64 +14:41:35.9: 11.81 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:38:15.64 +11:29:00.0: 12.07 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:38:07.41 +11:06:21.3: 12.13 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.80 +/- 0.00
Forced photometry reference-image weighted average: 12.08 +/- 0.01
Forced photometry reference-image weighted average: 12.12 +/- 0.01
Forced photometry filter KEPT candidate at 03:36:30.64 +14:41:35.9: ref_mag=11.80 +/- 0.00 new_mean_mag=10.8229 delta=0.98 (need > 0.90)
Forced photometry filter KEPT candidate at 03:38:15.64 +11:29:00.0: ref_mag=12.08 +/- 0.01 new_mean_mag=10.8555 delta=1.22 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:41:11.96 +12:31:30.5: 12.46 +/- 0.01 detection
Forced photometry filter KEPT candidate at 03:38:07.41 +11:06:21.3: ref_mag=12.12 +/- 0.01 new_mean_mag=10.6355 delta=1.48 (need > 0.90)
Forced photometry reference-image weighted average: 12.47 +/- 0.01
Forced photometry filter KEPT candidate at 03:41:11.96 +12:31:30.5: ref_mag=12.47 +/- 0.01 new_mean_mag=11.1347 delta=1.33 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:42:17.82 +13:30:49.1: 12.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.01
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:30:43.05 +09:00:26.2: 12.63 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:42:40.46 +13:08:33.4: 11.62 +/- 0.01 detection
Forced photometry filter KEPT candidate at 03:42:17.82 +13:30:49.1: ref_mag=12.38 +/- 0.01 new_mean_mag=11.2226 delta=1.16 (need > 0.90)
Forced photometry reference-image weighted average: 11.63 +/- 0.00
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Forced photometry filter KEPT candidate at 03:42:40.46 +13:08:33.4: ref_mag=11.63 +/- 0.00 new_mean_mag=10.6097 delta=1.02 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:39:06.56 +15:36:07.4: 12.51 +/- 0.01 detection
Forced photometry filter KEPT candidate at 03:30:43.05 +09:00:26.2: ref_mag=12.63 +/- 0.01 new_mean_mag=11.3757 delta=1.25 (need > 0.90)
Forced photometry reference-image weighted average: 12.53 +/- 0.01
Forced photometry filter KEPT candidate at 03:39:06.56 +15:36:07.4: ref_mag=12.53 +/- 0.01 new_mean_mag=11.5570 delta=0.97 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:33:45.06 +09:19:38.8: 12.54 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:43:16.67 +17:34:21.6: 12.07 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.53 +/- 0.01
Forced photometry filter KEPT candidate at 03:33:45.06 +09:19:38.8: ref_mag=12.53 +/- 0.01 new_mean_mag=10.9481 delta=1.58 (need > 0.90)
Forced photometry reference-image weighted average: 12.05 +/- 0.01
Forced photometry filter KEPT candidate at 03:43:16.67 +17:34:21.6: ref_mag=12.05 +/- 0.01 new_mean_mag=11.1209 delta=0.93 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:36:04.07 +14:27:48.8: 12.85 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:36:04.07 +14:27:48.8: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.01
Forced photometry filter KEPT candidate at 03:36:04.07 +14:27:48.8: ref_mag=12.87 +/- 0.01 new_mean_mag=11.6220 delta=1.25 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:42:24.28 +13:03:27.1: 12.93 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:42:24.28 +13:03:27.1: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.01
Forced photometry filter KEPT candidate at 03:42:24.28 +13:03:27.1: ref_mag=12.93 +/- 0.01 new_mean_mag=11.5243 delta=1.40 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:37:14.30 +10:39:56.1: 13.05 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:37:38.51 +10:57:57.9: 13.63 +/- 0.03 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:37:14.30 +10:39:56.1: 13.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.01
Forced photometry filter KEPT candidate at 03:37:14.30 +10:39:56.1: ref_mag=13.09 +/- 0.01 new_mean_mag=11.4577 delta=1.63 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:37:38.51 +10:57:57.9: 13.63 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.02
Forced photometry filter KEPT candidate at 03:37:38.51 +10:57:57.9: ref_mag=13.63 +/- 0.02 new_mean_mag=11.8548 delta=1.77 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:37:50.14 +11:12:45.2: 13.47 +/- 0.03 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:37:50.14 +11:12:45.2: 13.48 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.02
Forced photometry filter KEPT candidate at 03:37:50.14 +11:12:45.2: ref_mag=13.48 +/- 0.02 new_mean_mag=11.6789 delta=1.80 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:38:03.25 +10:46:22.9: 13.46 +/- 0.03 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:38:03.25 +10:46:22.9: 13.48 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.02
Forced photometry filter KEPT candidate at 03:38:03.25 +10:46:22.9: ref_mag=13.47 +/- 0.02 new_mean_mag=11.5286 delta=1.94 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:37:45.14 +11:03:45.5: 13.39 +/- 0.03 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:40:22.93 +12:11:01.6: 13.34 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:37:45.14 +11:03:45.5: 13.41 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.02
Forced photometry filter KEPT candidate at 03:37:45.14 +11:03:45.5: ref_mag=13.40 +/- 0.02 new_mean_mag=11.5084 delta=1.89 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:40:22.93 +12:11:01.6: 13.24 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Forced photometry filter KEPT candidate at 03:40:22.93 +12:11:01.6: ref_mag=13.29 +/- 0.02 new_mean_mag=11.6274 delta=1.66 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:39:51.61 +12:08:08.8: 13.34 +/- 0.03 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:39:51.61 +12:08:08.8: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.02
Forced photometry filter KEPT candidate at 03:39:51.61 +12:08:08.8: ref_mag=13.34 +/- 0.02 new_mean_mag=11.7420 delta=1.60 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:42:28.33 +17:37:28.4: 13.27 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:42:19.11 +13:12:25.1: 13.27 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:42:28.33 +17:37:28.4: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Forced photometry filter KEPT candidate at 03:42:28.33 +17:37:28.4: ref_mag=13.28 +/- 0.02 new_mean_mag=11.6844 delta=1.60 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:38:05.85 +10:47:26.7: 13.26 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:42:19.11 +13:12:25.1: 13.26 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Forced photometry filter KEPT candidate at 03:42:19.11 +13:12:25.1: ref_mag=13.26 +/- 0.02 new_mean_mag=11.5788 delta=1.69 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:38:05.85 +10:47:26.7: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Forced photometry filter KEPT candidate at 03:38:05.85 +10:47:26.7: ref_mag=13.27 +/- 0.02 new_mean_mag=11.3939 delta=1.88 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:37:58.82 +11:25:22.3: 13.25 +/- 0.03 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:37:58.82 +11:25:22.3: 13.26 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.02
Forced photometry filter KEPT candidate at 03:37:58.82 +11:25:22.3: ref_mag=13.25 +/- 0.02 new_mean_mag=11.7970 delta=1.46 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:36:52.87 +10:20:00.7: 13.24 +/- 0.03 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:42:07.85 +13:20:14.1: 13.23 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:36:52.87 +10:20:00.7: 13.17 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.02
Forced photometry filter KEPT candidate at 03:36:52.87 +10:20:00.7: ref_mag=13.20 +/- 0.02 new_mean_mag=11.2597 delta=1.94 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:42:07.85 +13:20:14.1: 13.18 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Forced photometry filter KEPT candidate at 03:42:07.85 +13:20:14.1: ref_mag=13.21 +/- 0.02 new_mean_mag=11.6927 delta=1.51 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:37:48.94 +11:11:08.7: 13.18 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:37:48.94 +11:11:08.7: 13.15 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.02
Forced photometry filter KEPT candidate at 03:37:48.94 +11:11:08.7: ref_mag=13.17 +/- 0.02 new_mean_mag=11.5106 delta=1.66 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:36:51.45 +10:40:53.1: 13.16 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:36:51.45 +10:40:53.1: 13.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.01
Forced photometry filter KEPT candidate at 03:36:51.45 +10:40:53.1: ref_mag=13.14 +/- 0.01 new_mean_mag=11.6439 delta=1.50 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:40:26.08 +12:14:34.7: 13.14 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:40:26.08 +12:14:34.7: 13.22 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.02
Forced photometry filter KEPT candidate at 03:40:26.08 +12:14:34.7: ref_mag=13.18 +/- 0.02 new_mean_mag=11.6915 delta=1.49 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:38:54.30 +11:40:32.5: 13.12 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:38:54.30 +11:40:32.5: 13.13 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.01
Forced photometry filter KEPT candidate at 03:38:54.30 +11:40:32.5: ref_mag=13.12 +/- 0.01 new_mean_mag=11.4474 delta=1.68 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:33:35.49 +09:19:19.0: 13.12 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:33:35.49 +09:19:19.0: 13.15 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Forced photometry filter KEPT candidate at 03:33:35.49 +09:19:19.0: ref_mag=13.13 +/- 0.02 new_mean_mag=11.5394 delta=1.59 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:38:41.89 +11:48:18.3: 13.07 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:38:41.89 +11:48:18.3: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.01
Forced photometry filter KEPT candidate at 03:38:41.89 +11:48:18.3: ref_mag=13.07 +/- 0.01 new_mean_mag=11.6027 delta=1.47 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:40:33.82 +12:11:44.4: 13.00 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:38:18.91 +15:14:42.4: 13.05 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:40:33.82 +12:11:44.4: 13.03 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.01
Forced photometry filter KEPT candidate at 03:40:33.82 +12:11:44.4: ref_mag=13.02 +/- 0.01 new_mean_mag=11.4178 delta=1.60 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:38:18.91 +15:14:42.4: 13.04 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.01
Forced photometry filter KEPT candidate at 03:38:18.91 +15:14:42.4: ref_mag=13.05 +/- 0.01 new_mean_mag=11.5863 delta=1.46 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:36:48.29 +10:33:09.3: 12.95 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:36:48.29 +10:33:09.3: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.01
Forced photometry filter KEPT candidate at 03:36:48.29 +10:33:09.3: ref_mag=12.96 +/- 0.01 new_mean_mag=11.4229 delta=1.54 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:39:47.83 +12:12:26.3: 12.92 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:39:47.83 +12:12:26.3: 12.95 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.01
Forced photometry filter KEPT candidate at 03:39:47.83 +12:12:26.3: ref_mag=12.93 +/- 0.01 new_mean_mag=11.4578 delta=1.48 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:31:38.88 +08:57:21.1: 12.85 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:31:38.88 +08:57:21.1: 12.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.01
Forced photometry filter KEPT candidate at 03:31:38.88 +08:57:21.1: ref_mag=12.86 +/- 0.01 new_mean_mag=11.2760 delta=1.58 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:38:04.64 +11:36:25.7: 12.84 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:38:04.64 +11:36:25.7: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.01
Forced photometry filter KEPT candidate at 03:38:04.64 +11:36:25.7: ref_mag=12.85 +/- 0.01 new_mean_mag=11.4668 delta=1.38 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:39:42.94 +12:17:37.8: 12.83 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:39:42.94 +12:17:37.8: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.01
Forced photometry filter KEPT candidate at 03:39:42.94 +12:17:37.8: ref_mag=12.82 +/- 0.01 new_mean_mag=11.5126 delta=1.31 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:42:05.19 +13:14:11.0: 12.81 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:42:05.19 +13:14:11.0: 12.84 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.01
Forced photometry filter KEPT candidate at 03:42:05.19 +13:14:11.0: ref_mag=12.82 +/- 0.01 new_mean_mag=11.4030 delta=1.42 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:35:19.86 +09:44:17.9: 12.78 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:35:19.86 +09:44:17.9: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.01
Forced photometry filter KEPT candidate at 03:35:19.86 +09:44:17.9: ref_mag=12.78 +/- 0.01 new_mean_mag=11.3598 delta=1.42 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:37:09.95 +10:48:11.3: 12.76 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:37:09.95 +10:48:11.3: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Forced photometry filter KEPT candidate at 03:37:09.95 +10:48:11.3: ref_mag=12.77 +/- 0.01 new_mean_mag=11.4200 delta=1.35 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:36:55.15 +10:18:02.7: 12.77 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:36:55.15 +10:18:02.7: 12.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Forced photometry filter KEPT candidate at 03:36:55.15 +10:18:02.7: ref_mag=12.77 +/- 0.01 new_mean_mag=11.1072 delta=1.66 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:32:53.25 +09:03:59.5: 12.72 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:32:53.25 +09:03:59.5: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.01
Forced photometry filter KEPT candidate at 03:32:53.25 +09:03:59.5: ref_mag=12.72 +/- 0.01 new_mean_mag=11.1519 delta=1.57 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:36:28.64 +14:34:35.4: 12.69 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:36:28.64 +14:34:35.4: 12.68 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.69 +/- 0.01
Forced photometry filter KEPT candidate at 03:36:28.64 +14:34:35.4: ref_mag=12.69 +/- 0.01 new_mean_mag=11.5529 delta=1.14 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:34:39.24 +09:53:46.3: 12.66 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:34:39.24 +09:53:46.3: 12.68 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.01
Forced photometry filter KEPT candidate at 03:34:39.24 +09:53:46.3: ref_mag=12.67 +/- 0.01 new_mean_mag=11.3430 delta=1.33 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:37:21.04 +10:43:52.6: 12.63 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:37:21.04 +10:43:52.6: 12.68 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Forced photometry filter KEPT candidate at 03:37:21.04 +10:43:52.6: ref_mag=12.65 +/- 0.01 new_mean_mag=11.0840 delta=1.57 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:38:44.47 +15:24:01.4: 12.64 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:38:44.47 +15:24:01.4: 12.61 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.01
Forced photometry filter KEPT candidate at 03:38:44.47 +15:24:01.4: ref_mag=12.62 +/- 0.01 new_mean_mag=11.3497 delta=1.27 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:40:19.44 +12:20:15.2: 12.64 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:40:19.44 +12:20:15.2: 12.60 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.01
Forced photometry filter KEPT candidate at 03:40:19.44 +12:20:15.2: ref_mag=12.62 +/- 0.01 new_mean_mag=11.2034 delta=1.42 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:40:08.92 +12:10:21.6: 12.62 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:40:08.92 +12:10:21.6: 12.64 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Forced photometry filter KEPT candidate at 03:40:08.92 +12:10:21.6: ref_mag=12.63 +/- 0.01 new_mean_mag=11.2814 delta=1.35 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:30:44.60 +08:57:32.6: 12.61 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:30:44.60 +08:57:32.6: 12.61 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.01
Forced photometry filter KEPT candidate at 03:30:44.60 +08:57:32.6: ref_mag=12.61 +/- 0.01 new_mean_mag=11.3343 delta=1.28 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:38:30.66 +15:12:47.0: 12.57 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:38:30.66 +15:12:47.0: 12.58 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.58 +/- 0.01
Forced photometry filter KEPT candidate at 03:38:30.66 +15:12:47.0: ref_mag=12.58 +/- 0.01 new_mean_mag=11.3152 delta=1.26 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:33:11.85 +09:18:13.7: 12.56 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:33:11.85 +09:18:13.7: 12.55 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.01
Forced photometry filter KEPT candidate at 03:33:11.85 +09:18:13.7: ref_mag=12.56 +/- 0.01 new_mean_mag=11.1024 delta=1.46 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:38:10.35 +11:30:23.6: 12.52 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:38:10.35 +11:30:23.6: 12.47 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.01
Forced photometry filter KEPT candidate at 03:38:10.35 +11:30:23.6: ref_mag=12.49 +/- 0.01 new_mean_mag=11.1175 delta=1.37 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:40:45.52 +12:21:21.7: 12.46 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:40:45.52 +12:21:21.7: 12.50 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.48 +/- 0.01
Forced photometry filter KEPT candidate at 03:40:45.52 +12:21:21.7: ref_mag=12.48 +/- 0.01 new_mean_mag=11.1219 delta=1.36 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:37:58.54 +11:27:04.8: 12.46 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:37:58.54 +11:27:04.8: 12.44 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.45 +/- 0.01
Forced photometry filter KEPT candidate at 03:37:58.54 +11:27:04.8: ref_mag=12.45 +/- 0.01 new_mean_mag=11.2374 delta=1.21 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:42:06.19 +13:27:27.9: 12.43 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:42:06.19 +13:27:27.9: 12.43 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.43 +/- 0.01
Forced photometry filter KEPT candidate at 03:42:06.19 +13:27:27.9: ref_mag=12.43 +/- 0.01 new_mean_mag=11.2799 delta=1.15 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:42:03.35 +17:02:31.2: 12.38 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:42:03.35 +17:02:31.2: 12.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.39 +/- 0.01
Forced photometry filter KEPT candidate at 03:42:03.35 +17:02:31.2: ref_mag=12.39 +/- 0.01 new_mean_mag=11.3417 delta=1.05 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:41:32.79 +17:17:41.6: 12.33 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:41:32.79 +17:17:41.6: 12.35 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.34 +/- 0.01
Forced photometry filter KEPT candidate at 03:41:32.79 +17:17:41.6: ref_mag=12.34 +/- 0.01 new_mean_mag=11.3696 delta=0.97 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:36:47.49 +10:36:56.5: 12.31 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:36:47.49 +10:36:56.5: 12.32 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.31 +/- 0.01
Forced photometry filter KEPT candidate at 03:36:47.49 +10:36:56.5: ref_mag=12.31 +/- 0.01 new_mean_mag=11.0019 delta=1.31 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:36:46.49 +10:38:01.4: 12.30 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:36:46.49 +10:38:01.4: 12.31 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.30 +/- 0.01
Forced photometry filter KEPT candidate at 03:36:46.49 +10:38:01.4: ref_mag=12.30 +/- 0.01 new_mean_mag=11.1722 delta=1.13 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:40:54.91 +12:34:20.7: 12.18 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:40:54.91 +12:34:20.7: 12.19 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.19 +/- 0.01
Forced photometry filter KEPT candidate at 03:40:54.91 +12:34:20.7: ref_mag=12.19 +/- 0.01 new_mean_mag=11.1673 delta=1.02 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:36:28.91 +10:41:33.8: 12.15 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:36:28.91 +10:41:33.8: 12.13 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.14 +/- 0.01
Forced photometry filter KEPT candidate at 03:36:28.91 +10:41:33.8: ref_mag=12.14 +/- 0.01 new_mean_mag=11.1392 delta=1.00 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:38:44.68 +15:22:30.4: 12.15 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:38:44.68 +15:22:30.4: 12.12 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.13 +/- 0.01
Forced photometry filter KEPT candidate at 03:38:44.68 +15:22:30.4: ref_mag=12.13 +/- 0.01 new_mean_mag=11.0121 delta=1.12 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:38:15.43 +11:43:54.2: 12.04 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:38:15.43 +11:43:54.2: 12.06 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.05 +/- 0.01
Forced photometry filter KEPT candidate at 03:38:15.43 +11:43:54.2: ref_mag=12.05 +/- 0.01 new_mean_mag=11.0728 delta=0.98 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:37:55.28 +10:46:30.7: 11.97 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:37:55.28 +10:46:30.7: 11.98 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.97 +/- 0.01
Forced photometry filter KEPT candidate at 03:37:55.28 +10:46:30.7: ref_mag=11.97 +/- 0.01 new_mean_mag=10.5439 delta=1.43 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:38:14.69 +15:20:43.1: 11.95 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:38:29.52 +15:36:50.6: 11.90 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:38:14.69 +15:20:43.1: 11.95 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.95 +/- 0.00
Forced photometry filter KEPT candidate at 03:38:14.69 +15:20:43.1: ref_mag=11.95 +/- 0.00 new_mean_mag=10.9132 delta=1.04 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:38:29.52 +15:36:50.6: 11.91 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.91 +/- 0.00
Forced photometry filter KEPT candidate at 03:38:29.52 +15:36:50.6: ref_mag=11.91 +/- 0.00 new_mean_mag=10.9094 delta=1.00 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:34:50.40 +09:49:04.0: 11.83 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:34:50.40 +09:49:04.0: 11.84 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.83 +/- 0.00
Forced photometry filter KEPT candidate at 03:34:50.40 +09:49:04.0: ref_mag=11.83 +/- 0.00 new_mean_mag=10.8237 delta=1.01 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:40:18.68 +12:06:18.1: 11.80 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:38:06.35 +11:32:01.4: 11.69 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:40:18.68 +12:06:18.1: 11.82 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.81 +/- 0.00
Forced photometry filter KEPT candidate at 03:40:18.68 +12:06:18.1: ref_mag=11.81 +/- 0.00 new_mean_mag=10.7004 delta=1.11 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:38:06.35 +11:32:01.4: 11.70 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.69 +/- 0.00
Forced photometry filter KEPT candidate at 03:38:06.35 +11:32:01.4: ref_mag=11.69 +/- 0.00 new_mean_mag=10.6513 delta=1.04 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:35:08.70 +09:46:03.4: 11.45 +/- 0.00 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:35:08.70 +09:46:03.4: 11.43 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.44 +/- 0.00
Forced photometry filter KEPT candidate at 03:35:08.70 +09:46:03.4: ref_mag=11.44 +/- 0.00 new_mean_mag=10.4687 delta=0.97 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:38:19.02 +11:09:07.0: 11.43 +/- 0.00 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:38:19.02 +11:09:07.0: 11.44 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.43 +/- 0.00
Forced photometry filter KEPT candidate at 03:38:19.02 +11:09:07.0: ref_mag=11.43 +/- 0.00 new_mean_mag=10.3131 delta=1.12 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:37:43.95 +11:13:37.7: 11.24 +/- 0.00 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:37:43.95 +11:13:37.7: 11.24 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.24 +/- 0.00
Forced photometry filter KEPT candidate at 03:37:43.95 +11:13:37.7: ref_mag=11.24 +/- 0.00 new_mean_mag=10.2842 delta=0.96 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:33:44.01 +09:13:09.4: 11.17 +/- 0.00 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:33:44.01 +09:13:09.4: 11.17 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.17 +/- 0.00
Forced photometry filter KEPT candidate at 03:33:44.01 +09:13:09.4: ref_mag=11.17 +/- 0.00 new_mean_mag=10.1323 delta=1.04 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:36:36.14 +10:10:18.3: 11.09 +/- 0.00 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:37:45.28 +10:46:49.0: 11.03 +/- 0.00 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:36:36.14 +10:10:18.3: 11.13 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.11 +/- 0.00
Forced photometry filter KEPT candidate at 03:36:36.14 +10:10:18.3: ref_mag=11.11 +/- 0.00 new_mean_mag=10.1704 delta=0.94 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:37:45.28 +10:46:49.0: 11.04 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.03 +/- 0.00
Forced photometry filter KEPT candidate at 03:37:45.28 +10:46:49.0: ref_mag=11.03 +/- 0.00 new_mean_mag=9.9872 delta=1.04 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:38:29.79 +11:27:00.7: 10.86 +/- 0.00 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:38:29.79 +11:27:00.7: 10.87 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.87 +/- 0.00
Forced photometry filter KEPT candidate at 03:38:29.79 +11:27:00.7: ref_mag=10.87 +/- 0.00 new_mean_mag=9.9547 delta=0.91 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:36:40.89 +10:23:33.8: 13.87 +/- 0.04 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:36:40.89 +10:23:33.8: 13.86 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.87 +/- 0.03
Forced photometry filter KEPT candidate at 03:36:40.89 +10:23:33.8: ref_mag=13.87 +/- 0.03 new_mean_mag=11.6926 delta=2.17 (need > 0.90)
Adding exclusion_list_local.txt__out08895.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09078.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10602.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11980.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19649.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19728.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20791.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20927.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21043.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21624.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21761.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24241.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24847.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25412.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29694.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29998.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out30562.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out30975.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31122.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31328.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31763.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33215.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33226.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33410.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33625.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34183.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34497.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34563.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34581.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35806.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36460.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36688.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36937.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37590.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37717.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38105.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38466.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38485.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38515.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38814.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38921.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38941.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39059.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39091.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39142.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39296.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40511.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40772.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41016.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41107.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41113.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41327.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41386.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out42413.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out42529.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out42638.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out42720.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out42953.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out42994.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43434.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43808.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44092.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44352.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44461.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44756.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45264.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45902.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45997.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46104.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46171.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46621.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46635.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46651.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46830.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47043.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47524.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47551.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out48532.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 873s
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: 42s
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Considering the candidate 53523_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
The candidate 53523_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375 did not pass the final checks
Rejecting candidate due to large distance (32.3") between the two second-epoch detections
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Considering the candidate 53531_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
The candidate 53531_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375 did not pass the final checks
Rejecting candidate due to large distance (32.3") between the two second-epoch detections
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Considering the candidate 31328_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 31328_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 24241_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 24241_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 09078_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 09078_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 42720_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 42720_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 40772_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 40772_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 29694_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 29694_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 48532_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 48532_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 34581_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 34581_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 19728_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 19728_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 33410_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 33410_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 25412_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 25412_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 31763_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 31763_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 38485_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 38485_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 39296_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 39296_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 41113_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 41113_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 38921_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 38921_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 40511_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 40511_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 46651_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 46651_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 46171_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 46171_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 08895_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 08895_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 31122_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 31122_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 39142_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 39142_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 42413_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 42413_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 36688_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 36688_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 30562_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 30562_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 41016_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 41016_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 38466_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 38466_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 46830_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 46830_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 43808_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 43808_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 34563_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 34563_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 44461_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 44461_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 21624_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 21624_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 46635_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 46635_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 37717_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 37717_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 46621_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 46621_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 33215_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 33215_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 43434_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 43434_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 47043_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 47043_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 30975_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 30975_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 45902_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 45902_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 39091_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 39091_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 36460_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 36460_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 33625_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 33625_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 24847_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 24847_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 41386_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 41386_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 38814_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 38814_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 20791_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 20791_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 47524_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 47524_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 46104_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 46104_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 33226_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 33226_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 21761_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 21761_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 34497_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 34497_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 42953_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 42953_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 47551_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 47551_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 42529_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 42529_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 29998_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 29998_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 11980_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 11980_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 25189_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
The candidate 25189_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375 did not pass the final checks
**** FOUND 03:35:58.23 +14:29:33.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 10602_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 10602_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 38105_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 38105_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 37590_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 37590_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 44756_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 44756_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 38515_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 38515_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 20927_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 20927_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 44092_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 44092_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 39059_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 39059_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 21043_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 21043_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 19649_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 19649_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 44352_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 44352_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 45997_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 45997_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 42994_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 42994_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 45264_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 45264_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 41107_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 41107_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 41327_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 41327_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 34183_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 34183_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35806_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 35806_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 38941_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 38941_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 42638_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 42638_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36937_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 36937_fd_Tau-05-Q1b1x1_2026-08-24_03-23-31_20.00sec_-0.00C_LIGHTs_0375
make_report_in_HTML.sh Phase 2 (HTML assembly): 6s
make_report_in_HTML.sh TOTAL: 921s
Prepared the HTML report for the field Tau-05-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
03:42:28.33 +17:37:28.4
03:43:16.67 +17:34:21.6
03:41:32.79 +17:17:41.6
03:42:03.35 +17:02:31.2
03:38:29.52 +15:36:50.6
03:39:06.56 +15:36:07.4
03:38:44.47 +15:24:01.4
03:38:44.68 +15:22:30.4
03:38:14.69 +15:20:43.1
03:38:18.91 +15:14:42.4
03:38:30.66 +15:12:47.0
03:36:30.64 +14:41:35.9
03:36:28.64 +14:34:35.4
03:36:04.07 +14:27:48.8
03:42:17.82 +13:30:49.1
03:42:06.19 +13:27:27.9
03:42:07.85 +13:20:14.1
03:42:05.19 +13:14:11.0
03:42:19.11 +13:12:25.1
03:42:40.46 +13:08:33.4
03:42:24.28 +13:03:27.1
03:31:38.88 +08:57:21.1
03:30:44.60 +08:57:32.6
03:30:43.05 +09:00:26.2
03:32:53.25 +09:03:59.5
03:33:44.01 +09:13:09.4
03:33:11.85 +09:18:13.7
03:33:35.49 +09:19:19.0
03:33:45.06 +09:19:38.8
03:36:36.14 +10:10:18.3
03:36:55.15 +10:18:02.7
03:36:52.87 +10:20:00.7
03:36:40.89 +10:23:33.8
03:36:46.49 +10:38:01.4
03:36:48.29 +10:33:09.3
03:36:47.49 +10:36:56.5
03:36:51.45 +10:40:53.1
03:37:14.30 +10:39:56.1
03:36:28.91 +10:41:33.8
03:37:21.04 +10:43:52.6
03:38:03.25 +10:46:22.9
03:37:45.28 +10:46:49.0
03:37:55.28 +10:46:30.7
03:37:09.95 +10:48:11.3
03:38:05.85 +10:47:26.7
03:37:38.51 +10:57:57.9
03:37:45.14 +11:03:45.5
03:38:07.41 +11:06:21.3
03:37:48.94 +11:11:08.7
03:38:19.02 +11:09:07.0
03:37:50.14 +11:12:45.2
03:37:43.95 +11:13:37.7
03:34:39.24 +09:53:46.3
03:37:58.82 +11:25:22.3
03:37:58.54 +11:27:04.8
03:38:29.79 +11:27:00.7
03:38:15.64 +11:29:00.0
03:38:10.35 +11:30:23.6
03:38:06.35 +11:32:01.4
03:38:04.64 +11:36:25.7
03:38:54.30 +11:40:32.5
03:38:15.43 +11:43:54.2
03:34:50.40 +09:49:04.0
03:38:41.89 +11:48:18.3
03:40:54.91 +12:34:20.7
03:35:08.70 +09:46:03.4
03:35:19.86 +09:44:17.9
03:40:18.68 +12:06:18.1
03:40:08.92 +12:10:21.6
03:39:51.61 +12:08:08.8
03:39:47.83 +12:12:26.3
03:40:33.82 +12:11:44.4
03:40:22.93 +12:11:01.6
03:40:26.08 +12:14:34.7
03:39:42.94 +12:17:37.8
03:40:19.44 +12:20:15.2
03:40:45.52 +12:21:21.7
03:41:11.96 +12:31:30.5
########### Completed Tau-05-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 ####
03:42:40.46 +13:08:33.4
03:36:30.64 +14:41:35.9
03:43:16.67 +17:34:21.6
03:38:15.64 +11:29:00.0
03:38:07.41 +11:06:21.3
03:42:17.82 +13:30:49.1
03:41:11.96 +12:31:30.5
03:33:45.06 +09:19:38.8
03:39:06.56 +15:36:07.4
03:30:43.05 +09:00:26.2
03:36:04.07 +14:27:48.8
03:42:24.28 +13:03:27.1
03:37:14.30 +10:39:56.1
03:37:38.51 +10:57:57.9
03:37:50.14 +11:12:45.2
03:38:03.25 +10:46:22.9
03:37:45.14 +11:03:45.5
03:40:22.93 +12:11:01.6
03:39:51.61 +12:08:08.8
03:42:28.33 +17:37:28.4
03:42:19.11 +13:12:25.1
03:38:05.85 +10:47:26.7
03:37:58.82 +11:25:22.3
03:36:52.87 +10:20:00.7
03:42:07.85 +13:20:14.1
03:37:48.94 +11:11:08.7
03:36:51.45 +10:40:53.1
03:40:26.08 +12:14:34.7
03:38:54.30 +11:40:32.5
03:33:35.49 +09:19:19.0
03:38:41.89 +11:48:18.3
03:38:18.91 +15:14:42.4
03:40:33.82 +12:11:44.4
03:36:48.29 +10:33:09.3
03:39:47.83 +12:12:26.3
03:31:38.88 +08:57:21.1
03:38:04.64 +11:36:25.7
03:39:42.94 +12:17:37.8
03:42:05.19 +13:14:11.0
03:35:19.86 +09:44:17.9
03:37:09.95 +10:48:11.3
03:36:55.15 +10:18:02.7
03:32:53.25 +09:03:59.5
03:36:28.64 +14:34:35.4
03:34:39.24 +09:53:46.3
03:37:21.04 +10:43:52.6
03:38:44.47 +15:24:01.4
03:40:19.44 +12:20:15.2
03:40:08.92 +12:10:21.6
03:30:44.60 +08:57:32.6
03:38:30.66 +15:12:47.0
03:33:11.85 +09:18:13.7
03:38:10.35 +11:30:23.6
03:40:45.52 +12:21:21.7
03:37:58.54 +11:27:04.8
03:42:06.19 +13:27:27.9
03:42:03.35 +17:02:31.2
03:41:32.79 +17:17:41.6
03:36:47.49 +10:36:56.5
03:36:46.49 +10:38:01.4
03:40:54.91 +12:34:20.7
03:36:28.91 +10:41:33.8
03:38:44.68 +15:22:30.4
03:38:15.43 +11:43:54.2
03:37:55.28 +10:46:30.7
03:38:14.69 +15:20:43.1
03:38:29.52 +15:36:50.6
03:34:50.40 +09:49:04.0
03:40:18.68 +12:06:18.1
03:38:06.35 +11:32:01.4
03:35:08.70 +09:46:03.4
03:38:19.02 +11:09:07.0
03:37:43.95 +11:13:37.7
03:33:44.01 +09:13:09.4
03:36:36.14 +10:10:18.3
03:37:45.28 +10:46:49.0
03:38:29.79 +11:27:00.7
03:36:40.89 +10:23:33.8
###################################################################################
03:42:40.46 +13:08:33.4 -- not an asteroid (will add it to exclusion list)
03:36:30.64 +14:41:35.9 -- not an asteroid (will add it to exclusion list)
03:43:16.67 +17:34:21.6 -- not an asteroid (will add it to exclusion list)
03:38:15.64 +11:29:00.0 -- not an asteroid (will add it to exclusion list)
03:38:07.41 +11:06:21.3 -- not an asteroid (will add it to exclusion list)
03:42:17.82 +13:30:49.1 -- not an asteroid (will add it to exclusion list)
03:41:11.96 +12:31:30.5 -- not an asteroid (will add it to exclusion list)
03:33:45.06 +09:19:38.8 -- not an asteroid (will add it to exclusion list)
03:39:06.56 +15:36:07.4 -- not an asteroid (will add it to exclusion list)
03:30:43.05 +09:00:26.2 -- not an asteroid (will add it to exclusion list)
03:36:04.07 +14:27:48.8 -- not an asteroid (will add it to exclusion list)
03:42:24.28 +13:03:27.1 -- not an asteroid (will add it to exclusion list)
03:37:14.30 +10:39:56.1 -- not an asteroid (will add it to exclusion list)
03:37:38.51 +10:57:57.9 -- not an asteroid (will add it to exclusion list)
03:37:50.14 +11:12:45.2 -- not an asteroid (will add it to exclusion list)
03:38:03.25 +10:46:22.9 -- not an asteroid (will add it to exclusion list)
03:37:45.14 +11:03:45.5 -- not an asteroid (will add it to exclusion list)
03:40:22.93 +12:11:01.6 -- not an asteroid (will add it to exclusion list)
03:39:51.61 +12:08:08.8 -- not an asteroid (will add it to exclusion list)
03:42:28.33 +17:37:28.4 -- not an asteroid (will add it to exclusion list)
03:42:19.11 +13:12:25.1 -- not an asteroid (will add it to exclusion list)
03:38:05.85 +10:47:26.7 -- not an asteroid (will add it to exclusion list)
03:37:58.82 +11:25:22.3 -- not an asteroid (will add it to exclusion list)
03:36:52.87 +10:20:00.7 -- not an asteroid (will add it to exclusion list)
03:42:07.85 +13:20:14.1 -- not an asteroid (will add it to exclusion list)
03:37:48.94 +11:11:08.7 -- not an asteroid (will add it to exclusion list)
03:36:51.45 +10:40:53.1 -- not an asteroid (will add it to exclusion list)
03:40:26.08 +12:14:34.7 -- not an asteroid (will add it to exclusion list)
03:38:54.30 +11:40:32.5 -- not an asteroid (will add it to exclusion list)
03:33:35.49 +09:19:19.0 -- not an asteroid (will add it to exclusion list)
03:38:41.89 +11:48:18.3 -- not an asteroid (will add it to exclusion list)
03:38:18.91 +15:14:42.4 -- not an asteroid (will add it to exclusion list)
03:40:33.82 +12:11:44.4 -- not an asteroid (will add it to exclusion list)
03:36:48.29 +10:33:09.3 -- not an asteroid (will add it to exclusion list)
03:39:47.83 +12:12:26.3 -- not an asteroid (will add it to exclusion list)
03:31:38.88 +08:57:21.1 -- not an asteroid (will add it to exclusion list)
03:38:04.64 +11:36:25.7 -- not an asteroid (will add it to exclusion list)
03:39:42.94 +12:17:37.8 -- not an asteroid (will add it to exclusion list)
03:42:05.19 +13:14:11.0 -- not an asteroid (will add it to exclusion list)
03:35:19.86 +09:44:17.9 -- not an asteroid (will add it to exclusion list)
03:37:09.95 +10:48:11.3 -- not an asteroid (will add it to exclusion list)
03:36:55.15 +10:18:02.7 -- not an asteroid (will add it to exclusion list)
03:32:53.25 +09:03:59.5 -- not an asteroid (will add it to exclusion list)
03:36:28.64 +14:34:35.4 -- not an asteroid (will add it to exclusion list)
03:34:39.24 +09:53:46.3 -- not an asteroid (will add it to exclusion list)
03:37:21.04 +10:43:52.6 -- not an asteroid (will add it to exclusion list)
03:38:44.47 +15:24:01.4 -- not an asteroid (will add it to exclusion list)
03:40:19.44 +12:20:15.2 -- not an asteroid (will add it to exclusion list)
03:40:08.92 +12:10:21.6 -- not an asteroid (will add it to exclusion list)
03:30:44.60 +08:57:32.6 -- not an asteroid (will add it to exclusion list)
03:38:30.66 +15:12:47.0 -- not an asteroid (will add it to exclusion list)
03:33:11.85 +09:18:13.7 -- not an asteroid (will add it to exclusion list)
03:38:10.35 +11:30:23.6 -- not an asteroid (will add it to exclusion list)
03:40:45.52 +12:21:21.7 -- not an asteroid (will add it to exclusion list)
03:37:58.54 +11:27:04.8 -- not an asteroid (will add it to exclusion list)
03:42:06.19 +13:27:27.9 -- not an asteroid (will add it to exclusion list)
03:42:03.35 +17:02:31.2 -- not an asteroid (will add it to exclusion list)
03:41:32.79 +17:17:41.6 -- not an asteroid (will add it to exclusion list)
03:36:47.49 +10:36:56.5 -- not an asteroid (will add it to exclusion list)
03:36:46.49 +10:38:01.4 -- not an asteroid (will add it to exclusion list)
03:40:54.91 +12:34:20.7 -- not an asteroid (will add it to exclusion list)
03:36:28.91 +10:41:33.8 -- not an asteroid (will add it to exclusion list)
03:38:44.68 +15:22:30.4 -- not an asteroid (will add it to exclusion list)
03:38:15.43 +11:43:54.2 -- not an asteroid (will add it to exclusion list)
03:37:55.28 +10:46:30.7 -- not an asteroid (will add it to exclusion list)
03:38:14.69 +15:20:43.1 -- not an asteroid (will add it to exclusion list)
03:38:29.52 +15:36:50.6 -- not an asteroid (will add it to exclusion list)
03:34:50.40 +09:49:04.0 -- not an asteroid (will add it to exclusion list)
03:40:18.68 +12:06:18.1 -- not an asteroid (will add it to exclusion list)
03:38:06.35 +11:32:01.4 -- not an asteroid (will add it to exclusion list)
03:35:08.70 +09:46:03.4 -- not an asteroid (will add it to exclusion list)
03:38:19.02 +11:09:07.0 -- not an asteroid (will add it to exclusion list)
03:37:43.95 +11:13:37.7 -- not an asteroid (will add it to exclusion list)
03:33:44.01 +09:13:09.4 -- not an asteroid (will add it to exclusion list)
03:36:36.14 +10:10:18.3 -- not an asteroid (will add it to exclusion list)
03:37:45.28 +10:46:49.0 -- not an asteroid (will add it to exclusion list)
03:38:29.79 +11:27:00.7 -- not an asteroid (will add it to exclusion list)
03:36:40.89 +10:23:33.8 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
03:30:43.05 +09:00:26.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:30:44.60 +08:57:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:31:38.88 +08:57:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:32:53.25 +09:03:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:33:11.85 +09:18:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:33:35.49 +09:19:19.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:33:44.01 +09:13:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:33:45.06 +09:19:38.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:34:39.24 +09:53:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:34:50.40 +09:49:04.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:35:08.70 +09:46:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:35:19.86 +09:44:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:36:04.07 +14:27:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:36:28.64 +14:34:35.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:36:28.91 +10:41:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:36:30.64 +14:41:35.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:36:36.14 +10:10:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:36:40.89 +10:23:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:36:46.49 +10:38:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:36:47.49 +10:36:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:36:48.29 +10:33:09.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:36:51.45 +10:40:53.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:36:52.87 +10:20:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:36:55.15 +10:18:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:37:09.95 +10:48:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:37:14.30 +10:39:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:37:21.04 +10:43:52.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:37:38.51 +10:57:57.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:37:43.95 +11:13:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:37:45.14 +11:03:45.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:37:45.28 +10:46:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:37:48.94 +11:11:08.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:37:50.14 +11:12:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:37:55.28 +10:46:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:37:58.54 +11:27:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:37:58.82 +11:25:22.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:38:03.25 +10:46:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:38:04.64 +11:36:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:38:05.85 +10:47:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:38:06.35 +11:32:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:38:07.41 +11:06:21.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:38:10.35 +11:30:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:38:14.69 +15:20:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:38:15.43 +11:43:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:38:15.64 +11:29:00.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:38:18.91 +15:14:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:38:19.02 +11:09:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:38:29.52 +15:36:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:38:29.79 +11:27:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:38:30.66 +15:12:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:38:41.89 +11:48:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:38:44.47 +15:24:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:38:44.68 +15:22:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:38:54.30 +11:40:32.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:39:06.56 +15:36:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:39:42.94 +12:17:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:39:47.83 +12:12:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:39:51.61 +12:08:08.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:40:08.92 +12:10:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:40:18.68 +12:06:18.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:40:19.44 +12:20:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:40:22.93 +12:11:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:40:26.08 +12:14:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:40:33.82 +12:11:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:40:45.52 +12:21:21.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:40:54.91 +12:34:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:41:11.96 +12:31:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:41:32.79 +17:17:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:42:03.35 +17:02:31.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:42:05.19 +13:14:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:42:06.19 +13:27:27.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:42:07.85 +13:20:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:42:17.82 +13:30:49.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:42:19.11 +13:12:25.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:42:24.28 +13:03:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:42:28.33 +17:37:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:42:40.46 +13:08:33.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:43:16.67 +17:34:21.6 -- 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)
03:30:43.05 +09:00:26.2 -- a known variable star
03:30:44.60 +08:57:32.6 -- not a known variable star
03:31:38.88 +08:57:21.1 -- not a known variable star
03:32:53.25 +09:03:59.5 -- a known variable star
03:33:11.85 +09:18:13.7 -- not a known variable star
03:33:35.49 +09:19:19.0 -- not a known variable star
03:33:44.01 +09:13:09.4 -- not a known variable star
03:33:45.06 +09:19:38.8 -- not a known variable star
03:34:39.24 +09:53:46.3 -- not a known variable star
03:34:50.40 +09:49:04.0 -- not a known variable star
03:35:08.70 +09:46:03.4 -- not a known variable star
03:35:19.86 +09:44:17.9 -- not a known variable star
03:36:04.07 +14:27:48.8 -- not a known variable star
03:36:28.64 +14:34:35.4 -- not a known variable star
03:36:28.91 +10:41:33.8 -- not a known variable star
03:36:30.64 +14:41:35.9 -- not a known variable star
03:36:36.14 +10:10:18.3 -- not a known variable star
03:36:40.89 +10:23:33.8 -- not a known variable star
03:36:46.49 +10:38:01.4 -- not a known variable star
03:36:47.49 +10:36:56.5 -- not a known variable star
03:36:48.29 +10:33:09.3 -- not a known variable star
03:36:51.45 +10:40:53.1 -- not a known variable star
03:36:52.87 +10:20:00.7 -- not a known variable star
03:36:55.15 +10:18:02.7 -- not a known variable star
03:37:09.95 +10:48:11.3 -- not a known variable star
03:37:14.30 +10:39:56.1 -- not a known variable star
03:37:21.04 +10:43:52.6 -- a known variable star
03:37:38.51 +10:57:57.9 -- not a known variable star
03:37:43.95 +11:13:37.7 -- not a known variable star
03:37:45.14 +11:03:45.5 -- not a known variable star
03:37:45.28 +10:46:49.0 -- not a known variable star
03:37:48.94 +11:11:08.7 -- a known variable star
03:37:50.14 +11:12:45.2 -- not a known variable star
03:37:55.28 +10:46:30.7 -- not a known variable star
03:37:58.54 +11:27:04.8 -- not a known variable star
03:37:58.82 +11:25:22.3 -- not a known variable star
03:38:03.25 +10:46:22.9 -- not a known variable star
03:38:04.64 +11:36:25.7 -- not a known variable star
03:38:05.85 +10:47:26.7 -- not a known variable star
03:38:06.35 +11:32:01.4 -- not a known variable star
03:38:07.41 +11:06:21.3 -- not a known variable star
03:38:10.35 +11:30:23.6 -- not a known variable star
03:38:14.69 +15:20:43.1 -- not a known variable star
03:38:15.43 +11:43:54.2 -- a known variable star
03:38:15.64 +11:29:00.0 -- not a known variable star
03:38:18.91 +15:14:42.4 -- not a known variable star
03:38:19.02 +11:09:07.0 -- not a known variable star
03:38:29.52 +15:36:50.6 -- a known variable star
03:38:29.79 +11:27:00.7 -- not a known variable star
03:38:30.66 +15:12:47.0 -- not a known variable star
03:38:41.89 +11:48:18.3 -- not a known variable star
03:38:44.47 +15:24:01.4 -- not a known variable star
03:38:44.68 +15:22:30.4 -- not a known variable star
03:38:54.30 +11:40:32.5 -- not a known variable star
03:39:06.56 +15:36:07.4 -- not a known variable star
03:39:42.94 +12:17:37.8 -- not a known variable star
03:39:47.83 +12:12:26.3 -- not a known variable star
03:39:51.61 +12:08:08.8 -- not a known variable star
03:40:08.92 +12:10:21.6 -- not a known variable star
03:40:18.68 +12:06:18.1 -- not a known variable star
03:40:19.44 +12:20:15.2 -- a known variable star
03:40:22.93 +12:11:01.6 -- not a known variable star
03:40:26.08 +12:14:34.7 -- not a known variable star
03:40:33.82 +12:11:44.4 -- not a known variable star
03:40:45.52 +12:21:21.7 -- not a known variable star
03:40:54.91 +12:34:20.7 -- a known variable star
03:41:11.96 +12:31:30.5 -- not a known variable star
03:41:32.79 +17:17:41.6 -- a known variable star
03:42:03.35 +17:02:31.2 -- not a known variable star
03:42:05.19 +13:14:11.0 -- a known variable star
03:42:06.19 +13:27:27.9 -- not a known variable star
03:42:07.85 +13:20:14.1 -- not a known variable star
03:42:17.82 +13:30:49.1 -- not a known variable star
03:42:19.11 +13:12:25.1 -- not a known variable star
03:42:24.28 +13:03:27.1 -- not a known variable star
03:42:28.33 +17:37:28.4 -- not a known variable star
03:42:40.46 +13:08:33.4 -- not a known variable star
03:43:16.67 +17:34:21.6 -- a known variable star
Found 67 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
78 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 78 (excluding asteroids and hot pixels, 67 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)2461276.84922612 -observatory V36
10:00:52.83 +14:01:03.8 Mercury (-1.8mag)
12:56:27.77 -08:41:00.8 Venus (-4.5mag)
06:35:29.55 +23:36:21.6 Mars (1.3mag)
08:57:14.11 +17:46:09.3 Jupiter (-1.8mag)
00:54:30.21 +02:59:03.4 Saturn (0.5mag)
04:13:10.06 +21:00:39.2 Uranus (5.7mag)
00:14:58.50 +00:05:10.4 Neptune (7.7mag)
20:26:40.36 -23:35:49.9 Pluto (14.5mag)
19:13:34.86 -26:25:58.0 Moon (-11.6mag)
-rw-r--r-- 1 apache apache 363 Aug 24 03:34 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461276.84922612:
08:57:13.00 +17:46:14.6 Io (6.1mag)
08:57:06.67 +17:46:45.0 Europa (6.3mag)
08:57:18.17 +17:45:48.7 Ganymede (5.6mag)
08:57:12.50 +17:46:19.9 Callisto (6.9mag)
08:54:43.12 +17:55:20.4 Himalia (15.7mag)
08:57:13.85 +17:46:11.4 Thebe (16.6mag)
08:54:22.84 +17:50:52.9 Elara (17.7mag)
09:01:20.84 +17:18:36.7 Pasiphae (17.9mag)
08:59:18.86 +18:00:14.4 Carme (19.0mag)
00:54:18.55 +02:59:20.8 Titan (8.4mag)
00:54:23.87 +02:59:04.5 Rhea (9.7mag)
00:55:06.10 +03:01:03.5 Iapetus (11.1mag)
00:54:28.67 +02:59:29.1 Hyperion (14.4mag)
00:53:32.61 +02:50:15.0 Phoebe (16.4mag)
-rw-r--r-- 1 apache apache 568 Aug 24 03:34 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461276.84922612:
20:24:08.60 -12:27:03.0 JWST
16:13:33.21 +47:30:14.8 Chandra
11:02:40.17 -59:32:38.5 XMM-Newton
-rw-r--r-- 1 apache apache 96 Aug 24 03:34 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461276.84922612 -observatory V36
03:30:02.70 +18:34:15.2 17.5mag P/1996 R2 (Lagerkvist)
17:59:59.72 -34:26:50.0 14.2mag P/2010 H2 (Vales)
07:08:12.84 -69:35:01.6 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:13:32.16 +33:21:15.7 17.7mag C/2017 K2 (PANSTARRS)
04:25:37.82 +42:53:17.9 17.6mag P/2021 N1 (ZTF)
22:25:02.37 +30:11:29.4 17.4mag C/2022 E2 (ATLAS)
06:58:41.19 +26:14:43.8 16.8mag C/2022 N2 (PANSTARRS)
10:36:33.77 +27:46:08.1 17.0mag C/2022 QE78 (ATLAS)
09:39:37.23 +05:17:39.8 18.0mag C/2022 R6 (PANSTARRS)
15:16:15.13 -12:58:05.5 18.0mag P/2023 B1 (PANSTARRS)
20:51:17.85 +63:44:15.6 18.0mag C/2023 H5 (Lemmon)
15:35:18.44 -14:24:44.2 14.6mag C/2023 R1 (PANSTARRS)
08:25:16.20 +32:06:47.9 15.6mag C/2024 E1 (Wierzchos)
15:05:41.36 +15:29:01.2 17.8mag C/2024 G6 (ATLAS)
18:44:52.45 +43:29:15.5 13.7mag C/2024 J3 (ATLAS)
20:46:24.00 +49:41:32.0 17.5mag C/2024 R4 (PANSTARRS)
05:27:07.63 -12:54:16.5 15.3mag C/2024 T5 (ATLAS)
07:05:38.41 +21:14:11.7 17.9mag C/2025 J1 (Borisov)
10:56:15.46 +19:48:56.2 17.0mag C/2025 V2 (Rankin)
13:08:49.57 +01:12:19.0 16.9mag C/2025 Y1 (ATLAS)
16:13:08.20 +76:02:25.4 16.4mag C/2026 A2 (Bok)
03:09:48.61 +46:20:57.8 17.3mag C/2026 B2 (Sun-Gao)
12:00:36.89 +10:06:19.4 17.4mag A/2026 E1
22:14:11.24 -32:49:30.2 7.2mag 10P/Tempel
11:39:00.03 -04:27:30.4 16.3mag 29P/Schwassmann-Wachmann
11:40:26.40 -00:37:20.3 17.4mag 63P/Wild
00:50:58.43 -06:12:49.8 15.4mag 65P/Gunn
06:11:01.00 +20:08:41.2 13.7mag 78P/Gehrels
20:24:20.94 -25:10:24.6 17.4mag 84P/Giclas
03:13:06.34 +14:37:22.2 16.9mag 88P/Howell
08:35:07.02 +25:16:17.2 16.4mag 93P/Lovas
04:53:39.03 +23:11:50.7 17.2mag 112P/Urata-Niijima
06:48:54.02 +27:55:46.7 16.0mag 114P/Wiseman-Skiff
09:56:14.81 +23:42:32.6 14.9mag 123P/West-Hartley
12:16:40.68 -16:20:21.7 17.3mag 124P/Mrkos
05:59:28.00 +20:59:32.5 16.0mag 128P/Shoemaker-Holt
06:55:06.47 +17:58:12.4 17.9mag 131P/Mueller
23:58:51.99 +03:01:45.4 17.4mag 139P/Vaisala-Oterma
03:06:52.36 -18:32:44.7 12.7mag 161P/Hartley-IRAS
08:10:01.03 +38:06:09.8 16.1mag 162P/Siding Spring
10:44:24.94 +27:11:50.2 12.3mag 169P/NEAT
03:08:56.89 +09:19:23.2 17.6mag 220P/McNaught
20:16:08.77 -51:32:40.3 18.0mag 259P/Garradd
04:09:00.26 +31:34:06.4 15.3mag 260P/McNaught
07:53:02.92 +36:57:02.2 17.3mag 295P/LINEAR
15:17:10.48 +01:19:44.6 17.8mag 391P/Kowalski
09:15:30.05 +17:33:58.0 17.9mag 450P/LONEOS
-rw-r--r-- 1 apache apache 2.3K Aug 24 03:34 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
21:28:47.85 +20:31:03.60 SN 2026sfn 2026-08-16.3 17.09
23:01:28.67 -61:00:39.00 SN 2026yib 2026-08-14.85 17.36
00:22:23.20 -32:16:02.70 SN 2026whu 2026-08-14.96 16.5
19:56:21.71 -37:24:19.90 ASASSN-26ew 2026-08-13.82 14.73
13:53:14.21 +00:26:52.00 SN 2026wkv 2026-08-10.12 15.83
05:21:07.61 +23:38:20.10 TCP J05210763+2338194 2026-08-10.59 9.34
01:28:20.49 +40:13:27.10 SN2026wpd 2026-08-9.34 16.37
23:47:50.87 +49:28:49.80 SN2026wjs 2026-08-9.35 17.12
16:03:20.92 +17:43:23.70 AT2026xau 2026-08-9.3 17.71
01:10:22.05 -09:34:08.50 SN2026weo 2026-08-7.46 15.76
00:56:54.35 -35:55:29.40 AT2026wdy 2026-08-5.05 16.08
22:08:07.63 -53:03:58.90 AT2026wek 2026-08-3.82 17.17
14:51:51.34 +66:13:24.60 ASASSN-26ev 2026-08-2.15 14.02
12:06:50.79 -36:16:06.20 SN2026wgm 2026-08-1.73 15.61
16:56:36.90 -59:29:26.00 ASASSN-26er 2026-07-25.82 15.09
01:21:27.83 -10:37:05.00 SN2026vbh 2026-07-25.61 15.97
21:17:31.59 +22:25:50.90 ASASSN-26eq 2026-07-24.37 15.13
18:53:36.89 +16:56:43.60 ASASSN-26ep 2026-07-23.47 -4.06
12:18:47.98 -30:48:47.50 ASASSN-26et 2026-07-22.76 13.98
13:00:47.82 +15:42:17.60 SN2026uwk 2026-07-21.75 16.38
18:52:31.11 -32:28:00.90 ASASSN-26en 2026-07-21.77 14.63
14:42:58.01 -62:32:59.10 ASASSN-26es 2026-07-20.79 15.36
20:12:45.57 -32:53:13.00 ASASSN-26em 2026-07-20.94 16.83
18:54:24.33 -46:11:51.70 ASASSN-26eu 2026-07-20.93 14.86
03:18:56.99 -80:55:10.40 AT2026ugi 2026-07-20.03 17.12
18:43:58.40 +24:22:41.80 ASASSN-26eo 2026-07-19.36 16.16
04:50:01.03 -02:22:33.80 ASASSN-26ej 2026-07-16.17 17.02
18:34:55.28 -31:41:00.90 ASASSN-26ek 2026-07-16.24 15.73
17:07:43.61 -44:21:53.50 ASASSN-26el 2026-07-15.86 16.01
14:45:08.35 +24:13:12.30 ASASSN-26ei 2026-07-16.17 16.46
10:00:46.44 -32:36:31.10 AT 2023mhb 2026-07-14.73 16.67
14:39:37.45 -11:22:36.20 AT 2026unl 2026-07-15.27 17.11
10:49:42.57 -11:25:55.80 ASASSN-26eh 2026-07-14.72 16.58
19:33:53.06 -07:15:00.80 ASASSN-22le 2026-07-14.15 15.5
02:45:40.52 -27:55:30.30 ASASSN-26ef 2026-07-12.35 15.86
23:26:43.80 +04:42:39.70 SN 2026qtn 2026-07-12.22 16.47
02:19:17.26 +28:57:15.40 ASASSN-26ec 2026-07-11.53 2.78
18:31:15.56 -05:34:31.50 AT2026stb 2026-07-11.28 -1.29
13:36:08.24 +23:29:05.00 AT2026pjf 2026-07-10.18 -0.72
17:33:39.82 +04:22:36.70 SN2026pir 2026-07-9.86 -0.66
11:21:41.26 -50:33:36.30 ASASSN-26ed 2026-07-8.8 -1.3
23:41:42.11 +26:29:49.10 AT2026qil 2026-07-9.3 16.15
20:21:30.50 -32:03:40.10 ASASSN-26ee 2026-07-7.22 15.53
19:37:44.09 -05:35:42.80 AT2026ryu 2026-07-7.17 14.88
11:06:55.46 -04:07:04.50 AT2026qqg 2026-07-5.01 16.82
19:07:23.69 -74:13:37.30 AT2026qly 2026-07-5.02 17.31
17:57:43.80 +27:18:40.10 ASASSN-26ea 2026-07-5.07 16.67
19:59:01.43 -32:07:34.30 ASASSN-26eb 2026-07-4.97 15.52
18:46:50.35 -57:44:13.20 SN 2026qqp 2026-07-5.03 -0.92
19:17:31.69 -39:55:29.90 ASASSN-26dz 2026-07-5.14 15.91
19:14:31.37 +12:03:52.90 AT 2026rdg 2026-07-3.43 11.81
04:05:50.09 -70:24:34.40 AT 2026qpr 2026-06-30.4 15.96
13:45:37.49 -05:59:35.80 SN 2026pub 2026-06-30.09 16.01
16:41:15.63 +39:17:14.70 SN 2026pel 2026-06-26.38 16.07
10:14:40.19 -35:38:21.30 ASASSN-26dy 2026-06-25.99 15.63
14:47:21.56 -40:15:51.30 ASASSN-26dv 2026-06-23.03 14.62
13:38:49.79 -77:21:06.70 ASASSN-26dw 2026-06-23.04 16.09
00:59:27.90 +33:08:13.20 SN 2026mke 2026-06-22.39 17.13
11:10:44.73 -30:20:45.50 SN 2026nmv 2026-06-22.06 16.56
21:36:15.68 -21:19:12.50 AT2026oxh 2026-06-22.15 17.14
17:31:38.38 -56:05:51.90 ASASSN-26dx 2026-06-22.02 14.72
14:10:13.44 -38:46:46.10 AT2026pvk 2026-06-22.06 16.53
20:56:47.23 -18:31:05.20 AT2026plb 2026-06-21.31 16.4
15:44:29.68 +21:00:59.30 SN2026ore 2026-06-21.29 17.57
23:50:05.98 -14:01:41.30 AT2026oxl 2026-06-21.52 17.64
17:36:54.73 -18:10:04.20 AT2026ouj 2026-06-20.92 15.15
00:34:04.08 -30:22:09.20 AT2026ntk 2026-06-18.09 17.34
20:49:13.39 +25:17:59.20 ASASSN-26du 2026-06-15.39 15.93
23:09:30.84 +32:40:42.00 SN2026oxc 2026-06-14.35 16.83
02:02:26.67 +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
-rw-r--r-- 1 apache apache 5.7K Aug 24 03:34 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
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
05:21:07.63 +23:38:19.4 TCP J05210763+2338194 2026-08-06.4109 11.2mag
22:57:17.96 +47:07:41.8 TCP J22571796+4707418 2026-08-09.3289 14.3mag
09:13:38.17 +76:28:18.1 PSN J09133817+7628181 2026-08-09.8037 15.4mag
00:43:17.29 +41:26:48.6 PNV J00431729+4126486 2026-08-14.0920 16.8mag
00:42:52.82 +41:10:58.6 PNV J00425282+4110586 2026-08-17.7723 19.9mag
00:42:52.83 +41:10:59.6 PNV J00425283+4110596 2026-08-18.6119 19.3mag
18:25:12.76 -22:25:29.3 TCP J18251276-2225293 2026-08-19.1062 9.4mag
18:03:09.04 +12:18:14.0 TCP J18030904+1218140 2026-08-19.5199 14.9mag
-rw-r--r-- 1 apache apache 190K Aug 24 03:34 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
22:16:10.733 +23:40:31.85 AT 2026xnv 2026-06-14.54 20.5
22:06:02.745 +21:38:59.91 AT 2026xnu 2026-06-14.54 20.68
12:04:33.241 +13:31:43.77 AT 2026xnt 2026-06-16.29 20.66
17:16:17.969 +32:53:41.29 AT 2026xns 2026-06-16.34 20.59
21:48:32.425 -29:28:38.76 AT 2026xnr 2026-06-16.55 19.93
20:44:08.930 -34:45:08.04 AT 2026xnq 2026-06-19.50 20.93
01:40:01.549 +15:24:08.32 AT 2026xnp 2026-06-21.59 20.11
22:59:54.981 +08:47:20.37 AT 2026xno 2026-06-22.57 20.61
22:34:44.112 -34:25:16.33 AT 2026xnn 2026-06-22.58 20.31
15:39:00.625 +01:51:45.97 AT 2026xnm 2026-07-09.30 20.53
22:18:23.260 +08:49:07.23 AT 2026xnl 2026-07-11.59 20.23
23:45:11.366 +23:12:01.58 AT 2026xnk 2026-07-16.50 20.23
17:52:40.604 +30:20:41.11 AT 2026xnj 2026-07-16.29 20.57
22:13:49.877 +15:15:41.07 AT 2026xni 2026-06-22.52 20.47
21:55:12.218 -25:50:43.90 AT 2026xnh 2026-07-08.51 20.23
17:42:05.047 +67:58:50.95 AT 2026xng 2026-08-05.89 19.07
15:05:35.464 +22:40:42.04 AT 2026xnf 2026-07-06.38 20.83
21:55:10.326 +01:47:27.63 AT 2026xne 2026-07-16.55 20.92
17:33:02.208 +23:15:50.89 AT 2026xnd 2026-07-19.39 20.4
17:58:43.835 +19:48:45.18 AT 2026xnc 2026-07-19.39 20.44
-rw-r--r-- 1 apache apache 87K Aug 24 03:34 tns_transients_list.txt
