This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR
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 06.3201 2461258.8201 11.42 05:08:31.68 +47:00:06.3
160.94801 4.01531 galactic Aur Second-epoch detections are separated by 0.8" and 7.4 pix
The object was found in VSX 2" ASASSN-V J050831.53+470006.8
Type: SR
# Max. Min./Amp. JD0 Period
12.620 V 12.970 V 2458559.47140 83.562083900000
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:08:31.68 +47:00:06.3: 12.41 +/- 0.01 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:08:31.68 +47:00:06.3: 12.42 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.42 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J050831.53+470006.8,2461258.8201,11.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J050831.53+470006.8 20260806.3201 11.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3201 2461258.8201 12.12 04:37:19.69 +48:15:49.5
156.64201 0.74611 galactic Per Second-epoch detections are separated by 3.6" and 8.6 pix
The object was found in VSX 2" ASASSN-V J043719.82+481547.7
Type: SR
# Max. Min./Amp. JD0 Period
13.680 V 13.890 V 2458433.60600 267.742709300000
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:37:19.69 +48:15:49.5: 13.31 +/- 0.03 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:37:19.69 +48:15:49.5: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.3201* 04 37 19.69 +48 15 49.5 12.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J043719.82+481547.7,2461258.8201,12.12,0.05,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
ASASSN-V J043719.82+481547.7 20260806.3201 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3201 2461258.8201 12.28 04:41:16.64 +50:40:21.5
155.26988 2.82779 galactic Per Second-epoch detections are separated by 1.5" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 260182697821637504 | 04:41:16.71 +50:40:23.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=1.333+/-0.029 (Very red! L if it's a dwarf)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:41:16.64 +50:40:21.5: 13.37 +/- 0.03 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:41:16.64 +50:40:21.5: 13.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.3201* 04 41 16.64 +50 40 21.5 12.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 260182697821637504,2461258.8201,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 260182697821637504 20260806.3201 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3201 2461258.8201 12.16 04:33:21.52 +45:50:52.4
157.96777 -1.38363 galactic Per Second-epoch detections are separated by 0.5" and 8.2 pix
The object was found in VSX 2" NSVS J0433217+455053
Type: L:
# Max. Min./Amp. JD0 Period
11.573 R1 Y 0.339 R1 289.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:33:21.52 +45:50:52.4: 13.31 +/- 0.03 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:33:21.52 +45:50:52.4: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.3201* 04 33 21.52 +45 50 52.4 12.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0433217+455053,2461258.8201,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0433217+455053 20260806.3201 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3201 2461258.8201 12.03 04:43:01.78 +43:37:41.4
160.76743 -1.58903 galactic Per Second-epoch detections are separated by 1.6" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J070.7570+43.6278 | 04:43:01.70 +43:37:40.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: M4 (LAMOST DR5) J-Ks=1.465+/-0.026 (Very red! L if it's a dwarf)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:43:01.78 +43:37:41.4: 13.29 +/- 0.03 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:43:01.78 +43:37:41.4: 13.29 +/- 0.03 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 06.3201* 04 43 01.78 +43 37 41.4 12.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J070.7570+43.6278,2461258.8201,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J070.7570+43.6278 20260806.3201 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3201 2461258.8201 12.21 04:45:15.30 +50:17:11.2
155.97719 3.05273 galactic Per Second-epoch detections are separated by 6.2" and 8.5 pix
The object was found in VSX 0" ASASSN-V J044515.28+501711.5
Type: SR
# Max. Min./Amp. JD0 Period
14.331 g Y 0.539 g 2458211.77480 196.642505900000
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:45:15.30 +50:17:11.2: 13.17 +/- 0.03 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:45:15.30 +50:17:11.2: 13.21 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.3201* 04 45 15.30 +50 17 11.2 12.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J044515.28+501711.5,2461258.8201,12.21,0.05,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
ASASSN-V J044515.28+501711.5 20260806.3201 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3201 2461258.8201 12.12 04:40:05.24 +49:46:42.7
155.81477 2.09342 galactic Per Second-epoch detections are separated by 3.5" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J070.0191+49.7759 | 04:40:05.01 +49:46:43.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=1.155+/-0.033 (M)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:40:05.24 +49:46:42.7: 13.16 +/- 0.03 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:40:05.24 +49:46:42.7: 13.15 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.3201* 04 40 05.24 +49 46 42.7 12.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J070.0191+49.7759,2461258.8201,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J070.0191+49.7759 20260806.3201 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3201 2461258.8201 12.16 04:32:37.07 +47:52:24.9
156.39749 -0.09748 galactic Per Second-epoch detections are separated by 0.5" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J068.1597+47.8808 | 04:32:37.02 +47:52:23.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5) J-Ks=0.828+/-0.028 (M)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:32:37.07 +47:52:24.9: 13.12 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:32:37.07 +47:52:24.9: 13.09 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.3201* 04 32 37.07 +47 52 24.9 12.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J068.1597+47.8808,2461258.8201,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J068.1597+47.8808 20260806.3201 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3201 2461258.8201 11.99 04:59:15.44 +47:36:00.2
159.51668 3.12801 galactic Aur Second-epoch detections are separated by 2.9" and 7.3 pix
The object was found in VSX 2" NSVS J0459158+473613
Type: SR
# Max. Min./Amp. JD0 Period
14.450 g Y 0.579 g 2458364.11950 77.998450200000
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:59:15.44 +47:36:00.2: 13.11 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:59:15.44 +47:36:00.2: 13.09 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0459158+473613,2461258.8201,11.99,0.05,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
NSVS J0459158+473613 20260806.3201 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3201 2461258.8201 12.12 04:30:32.94 +46:36:53.4
157.07551 -1.21465 galactic Per Second-epoch detections are separated by 2.4" and 8.3 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 J067.6367+46.6145 | 04:30:32.83 +46:36:52.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=1.493+/-0.033 (Very red! L if it's a dwarf)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:30:32.94 +46:36:53.4: 13.09 +/- 0.03 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:30:32.94 +46:36:53.4: 13.11 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.3201* 04 30 32.94 +46 36 53.4 12.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J067.6367+46.6145,2461258.8201,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J067.6367+46.6145 20260806.3201 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3201 2461258.8201 12.11 04:48:41.06 +45:08:23.6
160.27572 0.16141 galactic Per Second-epoch detections are separated by 2.1" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 254455887210040320 | 04:48:41.01 +45:08:23.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.370+/-0.047 (Very red! L if it's a dwarf)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:48:41.06 +45:08:23.6: 13.07 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:48:41.06 +45:08:23.6: 13.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.3201* 04 48 41.06 +45 08 23.6 12.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 254455887210040320,2461258.8201,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 254455887210040320 20260806.3201 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3201 2461258.8201 12.04 04:31:10.10 +46:35:45.1
157.16227 -1.15023 galactic Per Second-epoch detections are separated by 1.4" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 256902614116495360 | 04:31:10.03 +46:35:44.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.998+/-0.030 (M)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:31:10.10 +46:35:45.1: 13.02 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:31:10.10 +46:35:45.1: 13.01 +/- 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 06.3201* 04 31 10.10 +46 35 45.1 12.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 256902614116495360,2461258.8201,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 256902614116495360 20260806.3201 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3201 2461258.8201 11.87 04:46:57.75 +44:46:58.8
160.35161 -0.30161 galactic Per Second-epoch detections are separated by 2.1" and 8.3 pix
The object was found in VSX 1" ASASSN-V J044657.73+444658.4
Type: L
# Max. Min./Amp. JD0 Period
13.370 V 13.500 V
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:46:57.75 +44:46:58.8: 13.04 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:46:57.75 +44:46:58.8: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.3201* 04 46 57.75 +44 46 58.8 11.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J044657.73+444658.4,2461258.8201,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J044657.73+444658.4 20260806.3201 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3201 2461258.8201 12.12 04:34:23.18 +49:20:20.2
155.52104 1.11275 galactic Per Second-epoch detections are separated by 1.7" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 258558375549453568 | 04:34:23.16 +49:20:20.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.897+/-0.032 (M)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:34:23.18 +49:20:20.2: 13.04 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:34:23.18 +49:20:20.2: 13.06 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.3201* 04 34 23.18 +49 20 20.2 12.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 258558375549453568,2461258.8201,12.12,0.05,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 258558375549453568 20260806.3201 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3201 2461258.8201 11.96 05:02:33.10 +47:27:40.5
159.96815 3.48205 galactic Aur Second-epoch detections are separated by 0.7" and 7.4 pix
The object was found in VSX 2" NSVS J0502321+472733
Type: SR
# Max. Min./Amp. JD0 Period
14.293 g Y 0.383 g 2458387.61160 89.592063000000
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:02:33.10 +47:27:40.5: 13.06 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:02:33.10 +47:27:40.5: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0502321+472733,2461258.8201,11.96,0.05,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
NSVS J0502321+472733 20260806.3201 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3201 2461258.8201 12.01 04:36:32.49 +50:46:20.9
154.69570 2.33509 galactic Per Second-epoch detections are separated by 1.4" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 258931865905261568 | 04:36:32.33 +50:46:20.7 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: M4 (LAMOST DR5) J-Ks=1.640+/-0.039 (Very red! L if it's a dwarf)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:36:32.49 +50:46:20.9: 13.03 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:36:32.49 +50:46:20.9: 13.04 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.3201* 04 36 32.49 +50 46 20.9 12.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 258931865905261568,2461258.8201,12.01,0.05,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
Large-amplitude variable Gaia DR2 258931865905261568 20260806.3201 12.01CV 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 06.3201 2461258.8201 11.93 04:55:11.20 +46:50:06.9
159.68503 2.11097 galactic Aur Second-epoch detections are separated by 1.9" and 7.5 pix
The object was found in VSX 1" ASASSN-V J045511.31+465007.7
Type: SR
# Max. Min./Amp. JD0 Period
13.210 V 13.620 V 2457362.90000 69.800000000000
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:55:11.20 +46:50:06.9: 13.01 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:55:11.20 +46:50:06.9: 13.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J045511.31+465007.7,2461258.8201,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J045511.31+465007.7 20260806.3201 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3201 2461258.8201 12.04 04:32:10.65 +48:08:53.1
156.14654 0.03594 galactic Per Second-epoch detections are separated by 1.1" and 8.0 pix
The object was found in VSX 1" ASASSN-V J043210.62+480852.2
Type: L
# Max. Min./Amp. JD0 Period
13.460 V 13.660 V
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:32:10.65 +48:08:53.1: 13.00 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:32:10.65 +48:08:53.1: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.3201* 04 32 10.65 +48 08 53.1 12.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J043210.62+480852.2,2461258.8201,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J043210.62+480852.2 20260806.3201 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3201 2461258.8201 11.97 04:31:32.26 +49:30:02.1
155.08720 0.88343 galactic Per Second-epoch detections are separated by 1.7" and 8.3 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 258714123943837440 | 04:31:32.36 +49:30:03.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.523+/-0.043 (Very red! L if it's a dwarf)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:31:32.26 +49:30:02.1: 12.98 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:31:32.26 +49:30:02.1: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.3201* 04 31 32.26 +49 30 02.1 12.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 258714123943837440,2461258.8201,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 258714123943837440 20260806.3201 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3201 2461258.8201 11.98 04:32:44.83 +47:45:33.1
156.49599 -0.15955 galactic Per Second-epoch detections are separated by 0.4" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 257564142160697984 | 04:32:44.71 +47:45:33.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=1.146+/-0.034 (M)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:32:44.83 +47:45:33.1: 12.95 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:32:44.83 +47:45:33.1: 12.98 +/- 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 06.3201* 04 32 44.83 +47 45 33.1 12.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 257564142160697984,2461258.8201,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 257564142160697984 20260806.3201 11.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3201 2461258.8201 11.79 04:46:00.20 +49:15:33.2
156.83750 2.47709 galactic Per Second-epoch detections are separated by 0.5" and 7.9 pix
The object was found in VSX 3" ASASSN-V J044600.01+491531.4
Type: SR
# Max. Min./Amp. JD0 Period
12.920 V 13.010 V 2457669.00000 632.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:46:00.20 +49:15:33.2: 12.84 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:46:00.20 +49:15:33.2: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.3201* 04 46 00.20 +49 15 33.2 11.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J044600.01+491531.4,2461258.8201,11.79,0.05,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
ASASSN-V J044600.01+491531.4 20260806.3201 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 06.3201 2461258.8201 12.02 04:36:54.10 +48:06:53.7
156.70468 0.59354 galactic Per Second-epoch detections are separated by 1.4" and 7.8 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 257501847955946368 | 04:36:54.11 +48:06:54.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.285+/-0.036 (Very red! L if it's a dwarf)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:36:54.10 +48:06:53.7: 12.93 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:36:54.10 +48:06:53.7: 12.94 +/- 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 06.3201* 04 36 54.10 +48 06 53.7 12.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 257501847955946368,2461258.8201,12.02,0.05,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 257501847955946368 20260806.3201 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3201 2461258.8201 11.69 04:37:47.84 +42:27:39.4
161.00868 -3.07835 galactic Per Second-epoch detections are separated by 0.9" and 8.3 pix
The object was found in VSX 1" ASASSN-V J043747.78+422740.0
Type: L
# Max. Min./Amp. JD0 Period
12.890 V 13.320 V
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:37:47.84 +42:27:39.4: 12.91 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:37:47.84 +42:27:39.4: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.3201* 04 37 47.84 +42 27 39.4 11.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J043747.78+422740.0,2461258.8201,11.69,0.05,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
ASASSN-V J043747.78+422740.0 20260806.3201 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3201 2461258.8201 11.85 04:46:33.63 +49:56:25.1
156.37692 2.98736 galactic Per Second-epoch detections are separated by 2.0" and 7.5 pix
The object was found in VSX 1" NSVS J0446335+495623
Type: M
# Max. Min./Amp. JD0 Period
16.863 g Y 2.569 g 2458577.97500 370.000000000000 C
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:46:33.63 +49:56:25.1: 12.89 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:46:33.63 +49:56:25.1: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.3201* 04 46 33.63 +49 56 25.1 11.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0446335+495623,2461258.8201,11.85,0.05,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
NSVS J0446335+495623 20260806.3201 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 06.3201 2461258.8201 11.86 05:09:25.66 +47:08:49.0
160.92208 4.22478 galactic Aur Second-epoch detections are separated by 3.8" and 7.5 pix
The object was found in VSX 0" ASASSN-V J050925.63+470849.0
Type: SR
# Max. Min./Amp. JD0 Period
13.550 V 14.600 V 2457798.80000 138.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:09:25.66 +47:08:49.0: 12.85 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:09:25.66 +47:08:49.0: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J050925.63+470849.0,2461258.8201,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J050925.63+470849.0 20260806.3201 11.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3201 2461258.8201 11.81 04:33:26.73 +47:26:26.0
156.80958 -0.29014 galactic Per Second-epoch detections are separated by 1.0" and 8.3 pix
The object was found in VSX 1" ASASSN-V J043326.67+472626.5
Type: L
# Max. Min./Amp. JD0 Period
13.430 V 13.750 V
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:33:26.73 +47:26:26.0: 12.84 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:33:26.73 +47:26:26.0: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.3201* 04 33 26.73 +47 26 26.0 11.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J043326.67+472626.5,2461258.8201,11.81,0.05,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
ASASSN-V J043326.67+472626.5 20260806.3201 11.81CV 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 06.3201 2461258.8201 11.82 04:31:24.23 +45:07:47.6
158.25950 -2.12382 galactic Per Second-epoch detections are separated by 3.9" and 8.4 pix
The object was found in VSX 2" ASASSN-V J043124.13+450745.9
Type: L
# Max. Min./Amp. JD0 Period
13.090 V 13.450 V
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:31:24.23 +45:07:47.6: 12.80 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:31:24.23 +45:07:47.6: 12.72 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.3201* 04 31 24.23 +45 07 47.6 11.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J043124.13+450745.9,2461258.8201,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J043124.13+450745.9 20260806.3201 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3201 2461258.8201 11.78 04:47:31.30 +50:21:21.2
156.15887 3.37339 galactic Per Second-epoch detections are separated by 0.8" and 8.0 pix
The object was found in VSX 1" ASASSN-V J044731.27+502120.8
Type: L
# Max. Min./Amp. JD0 Period
13.080 V 13.320 V
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:47:31.30 +50:21:21.2: 12.81 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:47:31.30 +50:21:21.2: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.3201* 04 47 31.30 +50 21 21.2 11.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J044731.27+502120.8,2461258.8201,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J044731.27+502120.8 20260806.3201 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3201 2461258.8201 11.87 05:05:06.63 +47:40:23.4
160.06143 3.95380 galactic Aur Second-epoch detections are separated by 2.4" and 7.5 pix
The object was found in VSX 3" NSVS J0505068+474025
Type: L:
# Max. Min./Amp. JD0 Period
11.102 R1 Y 0.360 R1 90.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:05:06.63 +47:40:23.4: 12.79 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:05:06.63 +47:40:23.4: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0505068+474025,2461258.8201,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0505068+474025 20260806.3201 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3201 2461258.8201 11.88 04:48:15.55 +49:48:51.0
156.65027 3.11501 galactic Per Second-epoch detections are separated by 1.0" and 7.7 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 259198909790853376 | 04:48:15.63 +49:48:50.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.275+/-0.037 (Very red! L if it's a dwarf)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:48:15.55 +49:48:51.0: 12.80 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:48:15.55 +49:48:51.0: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.3201* 04 48 15.55 +49 48 51.0 11.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 259198909790853376,2461258.8201,11.88,0.05,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 259198909790853376 20260806.3201 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3201 2461258.8201 11.79 04:44:52.94 +50:46:55.3
155.56172 3.33029 galactic Per Second-epoch detections are separated by 1.3" and 8.0 pix
The object was found in VSX 0" ASASSN-V J044452.91+504655.6
Type: SR
# Max. Min./Amp. JD0 Period
14.320 g Y 0.210 g 2458490.71600 187.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:44:52.94 +50:46:55.3: 12.75 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:44:52.94 +50:46:55.3: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.3201* 04 44 52.94 +50 46 55.3 11.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J044452.91+504655.6,2461258.8201,11.79,0.05,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
ASASSN-V J044452.91+504655.6 20260806.3201 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 06.3201 2461258.8201 11.76 04:42:27.60 +48:57:35.0
156.68514 1.84245 galactic Per Second-epoch detections are separated by 1.8" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 259051678313505792 | 04:42:27.36 +48:57:34.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M1 (LAMOST DR5) J-Ks=1.413+/-0.030 (Very red! L if it's a dwarf)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:42:27.60 +48:57:35.0: 12.64 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:42:27.60 +48:57:35.0: 12.70 +/- 0.02 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 06.3201* 04 42 27.60 +48 57 35.0 11.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 259051678313505792,2461258.8201,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 259051678313505792 20260806.3201 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3201 2461258.8201 11.58 04:33:56.19 +41:01:55.1
161.58399 -4.57200 galactic Per Second-epoch detections are separated by 3.6" and 8.7 pix
The object was found in VSX 2" ASASSN-V J043356.08+410154.1
Type: SR
# Max. Min./Amp. JD0 Period
13.230 V 13.410 V 2457719.99700 66.880000000000
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:33:56.19 +41:01:55.1: 12.70 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:33:56.19 +41:01:55.1: 12.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.3201* 04 33 56.19 +41 01 55.1 11.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J043356.08+410154.1,2461258.8201,11.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J043356.08+410154.1 20260806.3201 11.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3201 2461258.8201 11.77 04:56:00.68 +45:05:25.3
161.13479 1.12857 galactic Aur Second-epoch detections are separated by 1.1" and 7.6 pix
The object was not found in VSX
The object was found in ASASSN-V 1" ASASSN-V J045600.62+450524.8
Type: SR
MeanMag 13.06 m Amp. 0.13 m Period 22.8277866 d
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:56:00.68 +45:05:25.3: 12.69 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:56:00.68 +45:05:25.3: 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461258.8201,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260806.3201 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3201 2461258.8201 11.65 04:38:35.39 +42:37:55.3
160.97863 -2.85547 galactic Per Second-epoch detections are separated by 1.9" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J069.6472+42.6321 | 04:38:35.34 +42:37:55.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.294+/-0.035 (Very red! L if it's a dwarf)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:38:35.39 +42:37:55.3: 12.65 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:38:35.39 +42:37:55.3: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.3201* 04 38 35.39 +42 37 55.3 11.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J069.6472+42.6321,2461258.8201,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J069.6472+42.6321 20260806.3201 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3201 2461258.8201 11.69 05:16:27.62 +48:24:29.4
160.58550 5.92004 galactic Aur Second-epoch detections are separated by 1.2" and 7.2 pix
The object was found in VSX 2" ASASSN-V J051627.39+482429.6
Type: L
# Max. Min./Amp. JD0 Period
12.770 V 13.620 V
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:16:27.62 +48:24:29.4: 12.65 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:16:27.62 +48:24:29.4: 12.61 +/- 0.02 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J051627.39+482429.6,2461258.8201,11.69,0.05,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
ASASSN-V J051627.39+482429.6 20260806.3201 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3201 2461258.8201 11.59 04:38:31.93 +42:28:05.5
161.09384 -2.97259 galactic Per Second-epoch detections are separated by 0.9" and 8.1 pix
The object was found in VSX 1" ASASSN-V J043831.90+422804.8
Type: SR
# Max. Min./Amp. JD0 Period
13.830 g Y 0.390 g 2458561.69700 179.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:38:31.93 +42:28:05.5: 12.63 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:38:31.93 +42:28:05.5: 12.58 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.3201* 04 38 31.93 +42 28 05.5 11.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J043831.90+422804.8,2461258.8201,11.59,0.05,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
ASASSN-V J043831.90+422804.8 20260806.3201 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 06.3201 2461258.8201 11.69 04:48:04.79 +51:06:04.6
155.64437 3.92090 galactic Per Second-epoch detections are separated by 0.2" and 7.8 pix
The object was found in VSX 1" ASASSN-V J044804.77+510605.1
Type: SRS
# Max. Min./Amp. JD0 Period
13.090 V 13.240 V 2457245.10800 25.976000000000
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:48:04.79 +51:06:04.6: 12.62 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:48:04.79 +51:06:04.6: 12.63 +/- 0.02 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 06.3201* 04 48 04.79 +51 06 04.6 11.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J044804.77+510605.1,2461258.8201,11.69,0.05,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
ASASSN-V J044804.77+510605.1 20260806.3201 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3201 2461258.8201 11.48 05:02:05.77 +47:33:20.1
159.84626 3.47863 galactic Aur Second-epoch detections are separated by 2.3" and 7.8 pix
The object was found in VSX 1" ASASSN-V J050205.76+473321.4
Type: SR
# Max. Min./Amp. JD0 Period
12.780 V 12.950 V 2457441.00000 528.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:02:05.77 +47:33:20.1: 12.47 +/- 0.01 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:02:05.77 +47:33:20.1: 12.48 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J050205.76+473321.4,2461258.8201,11.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J050205.76+473321.4 20260806.3201 11.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3201 2461258.8201 11.54 04:32:11.28 +49:29:06.5
155.17065 0.94997 galactic Per Second-epoch detections are separated by 0.4" and 8.2 pix
The object was found in VSX10" Gaia DR3 258531540592695040
Type: SR|M
# Max. Min./Amp. JD0 Period
14.510 G 14.760 G 124.500000000000 M
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:32:11.28 +49:29:06.5: 12.44 +/- 0.01 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:32:11.28 +49:29:06.5: 12.46 +/- 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 06.3201* 04 32 11.28 +49 29 06.5 11.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 258531540592695040,2461258.8201,11.54,0.05,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 258531540592695040 20260806.3201 11.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3201 2461258.8201 11.35 04:37:59.94 +43:15:28.5
160.43973 -2.51836 galactic Per Second-epoch detections are separated by 1.9" and 8.4 pix
The object was found in VSX 0" NSVS J0437599+431527
Type: SR
# Max. Min./Amp. JD0 Period
14.249 g Y 0.449 g 2458368.97340 271.862258200000 C
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:37:59.94 +43:15:28.5: 12.42 +/- 0.01 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:37:59.94 +43:15:28.5: 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 06.3201* 04 37 59.94 +43 15 28.5 11.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0437599+431527,2461258.8201,11.35,0.05,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
NSVS J0437599+431527 20260806.3201 11.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3201 2461258.8201 11.46 04:28:13.17 +41:56:04.1
160.18897 -4.73812 galactic Per Second-epoch detections are separated by 1.6" and 8.7 pix
The object was found in VSX 2" NSVS J0428129+415603
Type: M
# Max. Min./Amp. JD0 Period
18.674 g Y 1.926 g 2458501.61100 395.626355800000 C
ATTENTION: measured mag 11.46 is 5.3 mag brighter than the VSX record maximum brightness 16.75 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:28:13.17 +41:56:04.1: 12.36 +/- 0.01 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:28:13.17 +41:56:04.1: 12.38 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.37 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.3201* 04 28 13.17 +41 56 04.1 11.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0428129+415603,2461258.8201,11.46,0.05,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
NSVS J0428129+415603 20260806.3201 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3201 2461258.8201 11.30 04:23:09.69 +41:43:07.7
159.68702 -5.56542 galactic Per Second-epoch detections are separated by 0.4" and 8.5 pix
The object was found in VSX 3" ASASSN-V J042309.53+414305.5
Type: L
# Max. Min./Amp. JD0 Period
13.270 V 13.770 V
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:23:09.69 +41:43:07.7: 12.35 +/- 0.01 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:23:09.69 +41:43:07.7: 12.35 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.35 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.3201* 04 23 09.69 +41 43 07.7 11.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J042309.53+414305.5,2461258.8201,11.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J042309.53+414305.5 20260806.3201 11.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3201 2461258.8201 11.37 04:42:50.78 +50:46:14.7
155.35956 3.07932 galactic Per Second-epoch detections are separated by 1.3" and 8.0 pix
The object was found in VSX 1" ASASSN-V J044250.73+504615.3
Type: SR
# Max. Min./Amp. JD0 Period
12.730 V 12.970 V 2458417.96570 271.154096700000
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:42:50.78 +50:46:14.7: 12.34 +/- 0.01 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:42:50.78 +50:46:14.7: 12.29 +/- 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 06.3201* 04 42 50.78 +50 46 14.7 11.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J044250.73+504615.3,2461258.8201,11.37,0.05,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
ASASSN-V J044250.73+504615.3 20260806.3201 11.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3201 2461258.8201 11.16 04:40:04.90 +41:04:20.1
162.33120 -3.68409 galactic Per Second-epoch detections are separated by 2.4" and 8.5 pix
The object was found in VSX 1" ASASSN-V J044004.81+410419.3
Type: SR
# Max. Min./Amp. JD0 Period
13.480 g Y 0.280 g 2458497.76400 530.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:40:04.90 +41:04:20.1: 12.17 +/- 0.01 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:40:04.90 +41:04:20.1: 12.17 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.17 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.3201* 04 40 04.90 +41 04 20.1 11.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J044004.81+410419.3,2461258.8201,11.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J044004.81+410419.3 20260806.3201 11.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3201 2461258.8201 10.87 04:40:30.25 +43:11:52.8
160.78833 -2.21749 galactic Per Second-epoch detections are separated by 0.4" and 8.0 pix
The object was found in VSX 1" V0748 Per
Type: LB
# Max. Min./Amp. JD0 Period
10.200 w 10.600 w 282.000000000000 C(N)
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:40:30.25 +43:11:52.8: 12.11 +/- 0.01 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:40:30.25 +43:11:52.8: 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 06.3201* 04 40 30.25 +43 11 52.8 10.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0748 Per,2461258.8201,10.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0748 Per 20260806.3201 10.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3201 2461258.8201 10.99 04:56:10.79 +46:41:27.9
159.90411 2.15321 galactic Aur Second-epoch detections are separated by 1.8" and 7.6 pix
The object was found in VSX 2" NSVS J0456106+464131
Type: SR
# Max. Min./Amp. JD0 Period
13.462 g Y 0.806 g 2458426.81800 185.091095800000
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:56:10.79 +46:41:27.9: 11.96 +/- 0.01 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:56:10.79 +46:41:27.9: 12.01 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.98 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0456106+464131,2461258.8201,10.99,0.05,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
NSVS J0456106+464131 20260806.3201 10.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3201 2461258.8201 10.79 04:49:43.87 +45:47:29.4
159.89421 0.72064 galactic Per Second-epoch detections are separated by 1.5" and 7.9 pix
The object was found in VSX 2" NSVS J0449439+454732
Type: L
# Max. Min./Amp. JD0 Period
10.339 R1 Y 0.533 R1 239.000000000000 N
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:49:43.87 +45:47:29.4: 11.73 +/- 0.01 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:49:43.87 +45:47:29.4: 11.71 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.72 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.3201* 04 49 43.87 +45 47 29.4 10.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0449439+454732,2461258.8201,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0449439+454732 20260806.3201 10.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3201 2461258.8201 10.64 05:10:55.29 +48:42:07.9
159.81023 5.34453 galactic Aur Second-epoch detections are separated by 0.5" and 7.5 pix
The object was found in VSX 1" ASASSN-V J051055.22+484207.5
Type: SR
# Max. Min./Amp. JD0 Period
11.360 V 12.690 V 2457039.80000 405.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:10:55.29 +48:42:07.9: 11.66 +/- 0.01 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:10:55.29 +48:42:07.9: 11.64 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.65 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J051055.22+484207.5,2461258.8201,10.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J051055.22+484207.5 20260806.3201 10.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3201 2461258.8201 10.59 04:13:46.66 +41:36:16.1
158.51427 -6.87899 galactic Per Second-epoch detections are separated by 1.7" and 8.9 pix
The object was found in VSX 3" ASASSN-V J041346.44+413614.4
Type: SR
# Max. Min./Amp. JD0 Period
12.540 V 13.240 V 2458384.54090 89.469230300000
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:13:46.66 +41:36:16.1: 11.53 +/- 0.01 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:13:46.66 +41:36:16.1: 11.54 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.53 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.3201* 04 13 46.66 +41 36 16.1 10.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J041346.44+413614.4,2461258.8201,10.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J041346.44+413614.4 20260806.3201 10.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3201 2461258.8201 10.33 04:22:53.21 +44:06:41.7
157.94137 -3.92174 galactic Per Second-epoch detections are separated by 0.6" and 8.4 pix
The object was found in VSX 1" ASASSN-V J042253.09+440641.1
Type: SR
# Max. Min./Amp. JD0 Period
12.170 V 12.730 V 2458365.52820 294.762151300000
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:22:53.21 +44:06:41.7: 11.32 +/- 0.01 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:22:53.21 +44:06:41.7: 11.32 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.32 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.3201* 04 22 53.21 +44 06 41.7 10.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J042253.09+440641.1,2461258.8201,10.33,0.05,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
ASASSN-V J042253.09+440641.1 20260806.3201 10.33CV 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461093.60953049 22.02.2026 02:37:33.434 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
First image: 2461093.60953049 22.02.2026 02:37:33.434 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
Last image: 2461258.82044103 06.08.2026 07:41:16.105 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.73
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 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): 22110
Objects passed selection criteria: 21915
Measurements per detected object (mean, median, min, max): 2.2 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.2 2.0 2 4
Average stars detected per image: 12732.5
Average stars matched: 12299.8 (96.6012 %)
Memory usage VmPeak: 247004 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Aug 5 15:05:04 CDT 2026
VaST build number 1.0rc89-189-g49d3cdfd
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-05)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Aug 6 02:45:15 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461093.60953049 22.02.2026 02:37:33.434 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
First image: 2461093.60953049 22.02.2026 02:37:33.434 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
Last image: 2461258.82044103 06.08.2026 07:41:16.105 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 100
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.37
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 26 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): 177082
Objects passed selection criteria: 176414
Measurements per detected object (mean, median, min, max): 2.2 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.2 2.0 2 4
Average stars detected per image: 105999
Average stars matched: 101442 (95.7007 %)
Memory usage VmPeak: 640648 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Aug 5 15:05:04 CDT 2026
VaST build number 1.0rc89-189-g49d3cdfd
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-05)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Aug 6 02:46:32 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits
SExtractor catalog cache: saved Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.cat to cache
SExtractor catalog cache: saved Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461258.81983845
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits exists and is non-empty
Saving wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits to local_wcs_cache/
'wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits' -> 'local_wcs_cache/wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits'
wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits exists and is non-empty
Saving wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits to local_wcs_cache/
'wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits' -> 'local_wcs_cache/wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits'
wcs_fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits exists and is non-empty
Saving wcs_fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits to local_wcs_cache/
'wcs_fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits' -> 'local_wcs_cache/wcs_fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits'
wcs_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits exists and is non-empty
Saving wcs_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits to local_wcs_cache/
'wcs_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits' -> 'local_wcs_cache/wcs_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits (1st reference image)
verification OK: wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
Image size: 941.6'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 04:48:00.727 +45:59:45.06 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits (1st new image)
verification OK: wcs_fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits
Image size: 944.9'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 04:47:55.713 +46:00:04.96 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 04:48:00.727 +45:59:45.06
Second-epoch image center 04:47:55.713 +46:00:04.96
Angular distance between the image centers 0.0155 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits (2nd new image)
verification OK: wcs_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits
Image size: 944.9'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 04:47:58.409 +45:59:26.91 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 04:48:00.727 +45:59:45.06
Second-epoch image center 04:47:58.409 +45:59:26.91
Angular distance between the image centers 0.0084 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 04:47:55.713 +46:00:04.96
Second-epoch second image center 04:47:58.409 +45:59:26.91
Angular distance between the image centers 0.01314 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits &> /tmp/tmp.hdv2oR1WKi
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits &> /tmp/tmp.oKVE6omfzF
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits &> /tmp/tmp.9eaerlpy6T
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits &> /tmp/tmp.Autizodwbn
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits
Calibrating the magnitude scale
Found non-empty wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits and wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits and wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat
Found non-empty wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits and wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat
The reference image (wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits) and catalog (wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat) found
'wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat' -> 'wcsmag.cat'
Read 23847 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 59.9496 to 84.6399 deg, Dec +39.9317 to +51.3292 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 59.9496 to 84.6399 deg, Dec 39.9317 to 51.3292 deg
Loaded 12139 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 8124 out of 9276 total matches.
Matched with Tycho-2 9276 out of 23847 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.951350
a=0.000000 b=1.000000 c=22.951350
From vast_summary.log: estimated ref. image limiting mag.: -7.73
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.22
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.22
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 23847 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 59.9496 to 84.6399 deg, Dec +39.9317 to +51.3292 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 59.9496 to 84.6399 deg, Dec 39.9317 to 51.3292 deg
Loaded 12139 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 8124 out of 9276 total matches.
Matched with Tycho-2 9276 out of 23847 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
Forced-photometry filter: calibrated wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits -> calib.txt_param_ref_wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits (aperture=6.1)
Read 23965 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 59.9494 to 84.6297 deg, Dec +39.9321 to +51.3293 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 59.9494 to 84.6297 deg, Dec 39.9321 to 51.3293 deg
Loaded 12131 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 8135 out of 9280 total matches.
Matched with Tycho-2 9280 out of 23965 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
Forced-photometry filter: calibrated wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits -> calib.txt_param_ref_wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits (aperture=6.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
2.1 pix Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
2.8 pix fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits
2.8 pix fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits
Limiting magnitude estimates:
15.2 mag. Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
15.2 mag. Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
11.4 mag. fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits
11.5 mag. fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits
All-image limiting magnitude estimate: 11.4 (SNR ) 9.7 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.hdv2oR1WKi (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits' -> 'wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
WCS_IMAGE_NAME=wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
WCS-calibrated image found: wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
Checking if the catalog wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat corresponding to the image wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits alredy exist and is non-empty...
Catalog wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat corresponding to the image wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
WCS catalog name: wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2564, bad_region=0, passed=23847
Got 23847 stars (including 21254 good ones) from the SExtractor catalog wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat
util/solve_plate_with_UCAC5 got 23847 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.3)
Done reading UCAC5 zone files...
Matched 4918 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4871 matched stars entering correct_measured_positions(), 4871 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4871 matched stars entering correct_measured_positions(), 23847 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.3)
Done reading UCAC5 zone files...
Matched 4918 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4872 matched stars entering correct_measured_positions(), 23847 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 4872 matched stars entering correct_measured_positions(), 23847 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 4872 stars left (next iteration limit 5358)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits N_match=4872 sigma_overall_arcsec=0.443 sigma_q1_arcsec=0.581 sigma_q2_arcsec=0.429 sigma_q3_arcsec=0.440 sigma_q4_arcsec=0.341 n_q1=1102 n_q2=1035 n_q3=1609 n_q4=1126 worst_quadrant_to_overall_ratio=1.312
The image catalog is written to wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits -region wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.oKVE6omfzF (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits' -> 'wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
WCS_IMAGE_NAME=wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
WCS-calibrated image found: wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
Checking if the catalog wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat corresponding to the image wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits alredy exist and is non-empty...
Catalog wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat corresponding to the image wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
WCS catalog name: wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2577, bad_region=0, passed=23965
Got 23965 stars (including 21358 good ones) from the SExtractor catalog wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat
util/solve_plate_with_UCAC5 got 23965 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.3)
Done reading UCAC5 zone files...
Matched 4914 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4868 matched stars entering correct_measured_positions(), 4868 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4868 matched stars entering correct_measured_positions(), 23965 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.3)
Done reading UCAC5 zone files...
Matched 4914 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4869 matched stars entering correct_measured_positions(), 23965 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 4869 matched stars entering correct_measured_positions(), 23965 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 4869 stars left (next iteration limit 5354)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits N_match=4869 sigma_overall_arcsec=0.448 sigma_q1_arcsec=0.587 sigma_q2_arcsec=0.429 sigma_q3_arcsec=0.436 sigma_q4_arcsec=0.343 n_q1=1104 n_q2=1036 n_q3=1603 n_q4=1126 worst_quadrant_to_overall_ratio=1.308
The image catalog is written to wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits -region wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.9eaerlpy6T (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits
WCS_IMAGE_NAME=wcs_fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits
WCS-calibrated image found: wcs_fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits
Checking if the catalog wcs_fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits.wcscat corresponding to the image wcs_fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits.wcscat corresponding to the image wcs_fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits
WCS catalog name: wcs_fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.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=64, bad_region=0, passed=1675
Got 1675 stars (including 1608 good ones) from the SExtractor catalog wcs_fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits.wcscat
util/solve_plate_with_UCAC5 got 1675 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.9'
Seting catalog search parameters based on the expected field of view 944.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013124 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010499 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.1 to 51.4)
Done reading UCAC5 zone files...
Matched 1564 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1540 matched stars entering correct_measured_positions(), 1537 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1539 matched stars entering correct_measured_positions(), 1670 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.1 to 51.4)
Done reading UCAC5 zone files...
Matched 1565 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1540 matched stars entering correct_measured_positions(), 1669 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 1540 matched stars entering correct_measured_positions(), 1669 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 1540 stars left (next iteration limit 1692)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=1540 robust_rms=7.269 arcsec worst_quadrant_rms=8.225 arcsec
SIP_REFIT: SIP order 3 trial: matched=1540 robust_rms=0.555 arcsec worst_quadrant_rms=1.636 arcsec
SIP_REFIT: SIP order 5 trial: matched=1540 robust_rms=0.443 arcsec worst_quadrant_rms=0.607 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=1540 robust_rms_before=1.506 arcsec robust_rms_before_corrected=0.487 arcsec robust_rms_after=0.443 arcsec worst_quadrant_rms_before=0.763 worst_quadrant_rms_after=0.607
verification OK: wcs_fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits
verification OK: wcs_fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits
Image size: 945.3'x626.9' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 04:47:55.860 +46:00:03.36 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 1675 stars ###
'wcs_fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/correct_sextractor_wcs_catalog_usingxy2sky4188804.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 1.506 -> 0.443 arcsec)
WCS_QUALITY_DIAG: file=fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits N_match=1540 sigma_overall_arcsec=0.464 sigma_q1_arcsec=0.492 sigma_q2_arcsec=0.698 sigma_q3_arcsec=0.326 sigma_q4_arcsec=0.487 n_q1=390 n_q2=303 n_q3=444 n_q4=403 worst_quadrant_to_overall_ratio=1.506
The image catalog is written to wcs_fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits -region wcs_fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.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.Autizodwbn (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits
WCS_IMAGE_NAME=wcs_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits
WCS-calibrated image found: wcs_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits
Checking if the catalog wcs_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits.wcscat corresponding to the image wcs_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits.wcscat corresponding to the image wcs_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits
WCS catalog name: wcs_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.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=63, bad_region=0, passed=1751
Got 1751 stars (including 1685 good ones) from the SExtractor catalog wcs_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits.wcscat
util/solve_plate_with_UCAC5 got 1751 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.9'
Seting catalog search parameters based on the expected field of view 944.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013124 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010499 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.1 to 51.3)
Done reading UCAC5 zone files...
Matched 1639 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1612 matched stars entering correct_measured_positions(), 1611 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1612 matched stars entering correct_measured_positions(), 1749 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.1 to 51.3)
Done reading UCAC5 zone files...
Matched 1640 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1613 matched stars entering correct_measured_positions(), 1748 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 1612 matched stars entering correct_measured_positions(), 1748 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 1612 stars left (next iteration limit 1773)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=1612 robust_rms=7.814 arcsec worst_quadrant_rms=8.236 arcsec
SIP_REFIT: SIP order 3 trial: matched=1612 robust_rms=0.540 arcsec worst_quadrant_rms=1.516 arcsec
SIP_REFIT: SIP order 5 trial: matched=1612 robust_rms=0.422 arcsec worst_quadrant_rms=0.588 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=1612 robust_rms_before=1.457 arcsec robust_rms_before_corrected=0.516 arcsec robust_rms_after=0.422 arcsec worst_quadrant_rms_before=0.779 worst_quadrant_rms_after=0.588
verification OK: wcs_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits
verification OK: wcs_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits
Image size: 945.2'x626.8' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 04:47:58.564 +45:59:25.35 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 1751 stars ###
'wcs_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/correct_sextractor_wcs_catalog_usingxy2sky4188718.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 1.457 -> 0.422 arcsec)
WCS_QUALITY_DIAG: file=fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits N_match=1612 sigma_overall_arcsec=0.436 sigma_q1_arcsec=0.453 sigma_q2_arcsec=0.662 sigma_q3_arcsec=0.337 sigma_q4_arcsec=0.431 n_q1=404 n_q2=306 n_q3=481 n_q4=421 worst_quadrant_to_overall_ratio=1.519
The image catalog is written to wcs_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits -region wcs_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits sigma_overall=0.443 worst_q_ratio=1.312
ref2=Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits sigma_overall=0.448 worst_q_ratio=1.308
new1=fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits sigma_overall=0.464 worst_q_ratio=1.506
new2=fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits sigma_overall=0.436 worst_q_ratio=1.519
reference average sigma_overall=0.4455 worst_q_ratio=1.31
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044_astrometric_residuals.png (4872 matched stars from wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.40 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045_astrometric_residuals.png (4869 matched stars from wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.40 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286_astrometric_residuals.png (1540 matched stars from wcs_fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.37 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287_astrometric_residuals.png (1612 matched stars from wcs_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.34 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/wcs_fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits'
Saving fully-calibrated image wcs_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/wcs_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits'
Preparing the HTML report for the field Per-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Per-03-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/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits
SExtractor catalog cache: saved Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.cat to cache
SExtractor catalog cache: saved Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
Creating symlink local_wcs_cache/wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
Creating symlink local_wcs_cache/wcs_fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits
Creating symlink local_wcs_cache/wcs_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits
Creating symlink local_wcs_cache/exclusion_list.txt
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_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits exists and is non-empty
wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits exists and is non-empty
wcs_fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits exists and is non-empty
wcs_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits (1st reference image)
verification OK: wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
Image size: 941.6'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 04:48:00.727 +45:59:45.06 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits (1st new image)
verification OK: wcs_fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits
Image size: 944.9'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 04:47:55.713 +46:00:04.96 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 04:48:00.727 +45:59:45.06
Second-epoch image center 04:47:55.713 +46:00:04.96
Angular distance between the image centers 0.0155 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits (2nd new image)
verification OK: wcs_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits
Image size: 944.9'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 04:47:58.409 +45:59:26.91 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 04:48:00.727 +45:59:45.06
Second-epoch image center 04:47:58.409 +45:59:26.91
Angular distance between the image centers 0.0084 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 04:47:55.713 +46:00:04.96
Second-epoch second image center 04:47:58.409 +45:59:26.91
Angular distance between the image centers 0.01314 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits &> /tmp/tmp.I6j2fk2Ksb
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits &> /tmp/tmp.PNUIwyxdpm
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits &> /tmp/tmp.D9yIXmAO16
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits &> /tmp/tmp.3Mp6rBoHXG
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits
Calibrating the magnitude scale
Found non-empty wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits and wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits and wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat
Found non-empty wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits and wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat
The reference image (wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits) and catalog (wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat) found
'wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat' -> 'wcsmag.cat'
Read 195814 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 59.9096 to 84.6822 deg, Dec +39.9252 to +51.3404 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 59.9096 to 84.6822 deg, Dec 39.9252 to 51.3404 deg
Loaded 12199 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): 6231 out of 9378 total matches.
Matched with Tycho-2 9378 out of 195814 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.807400
a=0.000000 b=1.000000 c=22.807400
From vast_summary.log: estimated ref. image limiting mag.: -7.37
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.44
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.44
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 195814 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 59.9096 to 84.6822 deg, Dec +39.9252 to +51.3404 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 59.9096 to 84.6822 deg, Dec 39.9252 to 51.3404 deg
Loaded 12199 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): 6231 out of 9378 total matches.
Matched with Tycho-2 9378 out of 195814 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
Forced-photometry filter: calibrated wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits -> calib.txt_param_ref_wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits (aperture=4.5)
Read 196080 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 59.9097 to 84.6518 deg, Dec +39.9253 to +51.3374 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 59.9097 to 84.6518 deg, Dec 39.9253 to 51.3374 deg
Loaded 12186 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): 6203 out of 9379 total matches.
Matched with Tycho-2 9379 out of 196080 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
Forced-photometry filter: calibrated wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits -> calib.txt_param_ref_wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits (aperture=4.5)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 97 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.9 pix Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
1.9 pix Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
2.6 pix fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits
2.6 pix fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits
Limiting magnitude estimates:
15.4 mag. Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
15.4 mag. Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
12.4 mag. fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits
12.5 mag. fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits
All-image limiting magnitude estimate: 12.4 (SNR ) 12.1 (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.I6j2fk2Ksb (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits' -> 'wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
WCS_IMAGE_NAME=wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
WCS-calibrated image found: wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
Checking if the catalog wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat corresponding to the image wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits alredy exist and is non-empty...
Catalog wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat corresponding to the image wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
WCS catalog name: wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=57, blended=26966, bad_region=1, passed=195757
Got 195757 stars (including 168489 good ones) from the SExtractor catalog wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat
util/solve_plate_with_UCAC5 got 195757 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.3)
Done reading UCAC5 zone files...
Matched 4920 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4885 matched stars entering correct_measured_positions(), 4885 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4885 matched stars entering correct_measured_positions(), 195757 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.3)
Done reading UCAC5 zone files...
Matched 4920 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4885 matched stars entering correct_measured_positions(), 195757 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 4885 matched stars entering correct_measured_positions(), 195757 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 4885 stars left (next iteration limit 5373)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits N_match=4885 sigma_overall_arcsec=0.425 sigma_q1_arcsec=0.549 sigma_q2_arcsec=0.408 sigma_q3_arcsec=0.426 sigma_q4_arcsec=0.329 n_q1=1093 n_q2=1064 n_q3=1516 n_q4=1212 worst_quadrant_to_overall_ratio=1.293
The image catalog is written to wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits -region wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.PNUIwyxdpm (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits' -> 'wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
WCS_IMAGE_NAME=wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
WCS-calibrated image found: wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
Checking if the catalog wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat corresponding to the image wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits alredy exist and is non-empty...
Catalog wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat corresponding to the image wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
WCS catalog name: wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=67, blended=27081, bad_region=0, passed=196013
Got 196013 stars (including 168638 good ones) from the SExtractor catalog wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat
util/solve_plate_with_UCAC5 got 196013 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.3)
Done reading UCAC5 zone files...
Matched 4917 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4877 matched stars entering correct_measured_positions(), 4877 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4877 matched stars entering correct_measured_positions(), 196013 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.3)
Done reading UCAC5 zone files...
Matched 4917 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4877 matched stars entering correct_measured_positions(), 196013 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 4877 matched stars entering correct_measured_positions(), 196013 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 4877 stars left (next iteration limit 5364)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits N_match=4877 sigma_overall_arcsec=0.435 sigma_q1_arcsec=0.573 sigma_q2_arcsec=0.418 sigma_q3_arcsec=0.426 sigma_q4_arcsec=0.344 n_q1=1089 n_q2=1072 n_q3=1507 n_q4=1209 worst_quadrant_to_overall_ratio=1.318
The image catalog is written to wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits -region wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.D9yIXmAO16 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits
WCS_IMAGE_NAME=wcs_fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits
WCS-calibrated image found: wcs_fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits
Checking if the catalog wcs_fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits.wcscat corresponding to the image wcs_fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits.wcscat corresponding to the image wcs_fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits
WCS catalog name: wcs_fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.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=1, blended=315, bad_region=2, passed=16721
Got 16721 stars (including 16385 good ones) from the SExtractor catalog wcs_fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits.wcscat
util/solve_plate_with_UCAC5 got 16721 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.9'
Seting catalog search parameters based on the expected field of view 944.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013124 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010499 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.0 to 51.4)
Done reading UCAC5 zone files...
Matched 4897 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4833 matched stars entering correct_measured_positions(), 4837 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4833 matched stars entering correct_measured_positions(), 16721 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.0 to 51.4)
Done reading UCAC5 zone files...
Matched 4897 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4831 matched stars entering correct_measured_positions(), 16721 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Accuracy estimation diagnostic: 4831 matched stars entering correct_measured_positions(), 16721 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 4831 stars left (next iteration limit 5316)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits N_match=4831 sigma_overall_arcsec=0.590 sigma_q1_arcsec=0.611 sigma_q2_arcsec=0.787 sigma_q3_arcsec=0.453 sigma_q4_arcsec=0.596 n_q1=1235 n_q2=958 n_q3=1356 n_q4=1282 worst_quadrant_to_overall_ratio=1.334
The image catalog is written to wcs_fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits -region wcs_fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.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.3Mp6rBoHXG (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits
WCS_IMAGE_NAME=wcs_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits
WCS-calibrated image found: wcs_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits
Checking if the catalog wcs_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits.wcscat corresponding to the image wcs_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits.wcscat corresponding to the image wcs_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits
WCS catalog name: wcs_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.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=340, bad_region=2, passed=17611
Got 17611 stars (including 17245 good ones) from the SExtractor catalog wcs_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits.wcscat
util/solve_plate_with_UCAC5 got 17611 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.9'
Seting catalog search parameters based on the expected field of view 944.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013124 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010499 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.0 to 51.4)
Done reading UCAC5 zone files...
Matched 4898 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4838 matched stars entering correct_measured_positions(), 4841 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4838 matched stars entering correct_measured_positions(), 17611 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.0 to 51.4)
Done reading UCAC5 zone files...
Matched 4901 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4840 matched stars entering correct_measured_positions(), 17611 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 4840 matched stars entering correct_measured_positions(), 17611 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Excluding outliers - 4840 stars left (next iteration limit 5321)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits N_match=4840 sigma_overall_arcsec=0.569 sigma_q1_arcsec=0.600 sigma_q2_arcsec=0.779 sigma_q3_arcsec=0.450 sigma_q4_arcsec=0.547 n_q1=1223 n_q2=929 n_q3=1426 n_q4=1262 worst_quadrant_to_overall_ratio=1.369
The image catalog is written to wcs_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits -region wcs_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.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_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.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_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/wcs_fd_Per-03-Q1b1x1_2026-08-06_02-40-24_20.00sec_0.00C_LIGHTs_0286.fits
Saving fully-calibrated image wcs_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.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_2026-08-06_CI_Per-03-Q1b1x1_024233_TTUQ1b1x1_4047223_HDXAgfDR/wcs_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287.fits
Preparing the HTML report for the field Per-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:11:45.69 +47:08:21.6: 11.77 +/- 0.01 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:08:31.68 +47:00:06.3: 12.41 +/- 0.01 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:11:45.69 +47:08:21.6: 11.76 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.77 +/- 0.01
Forced photometry filter REJECTED candidate at 05:11:45.69 +47:08:21.6: ref_mag=11.77 +/- 0.01 new_mean_mag=11.9444 delta=-0.18 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:37:19.69 +48:15:49.5: 13.31 +/- 0.03 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:41:16.64 +50:40:21.5: 13.37 +/- 0.03 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:08:31.68 +47:00:06.3: 12.42 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.42 +/- 0.01
Forced photometry filter KEPT candidate at 05:08:31.68 +47:00:06.3: ref_mag=12.42 +/- 0.01 new_mean_mag=11.4181 delta=1.00 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:33:21.52 +45:50:52.4: 13.31 +/- 0.03 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:37:19.69 +48:15:49.5: 13.29 +/- 0.03 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:41:16.64 +50:40:21.5: 13.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Forced photometry reference-image weighted average: 13.36 +/- 0.02
Forced photometry filter KEPT candidate at 04:37:19.69 +48:15:49.5: ref_mag=13.30 +/- 0.02 new_mean_mag=12.1126 delta=1.19 (need > 0.90)
Forced photometry filter KEPT candidate at 04:41:16.64 +50:40:21.5: ref_mag=13.36 +/- 0.02 new_mean_mag=12.2777 delta=1.08 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:43:01.78 +43:37:41.4: 13.29 +/- 0.03 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:26:31.76 +41:11:14.5: 10.23 +/- 0.00 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:40:05.24 +49:46:42.7: 13.16 +/- 0.03 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:45:15.30 +50:17:11.2: 13.17 +/- 0.03 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:33:21.52 +45:50:52.4: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.02
Forced photometry filter KEPT candidate at 04:33:21.52 +45:50:52.4: ref_mag=13.32 +/- 0.02 new_mean_mag=12.0950 delta=1.22 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:32:37.07 +47:52:24.9: 13.12 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:59:15.44 +47:36:00.2: 13.11 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:43:01.78 +43:37:41.4: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:26:31.76 +41:11:14.5: 10.23 +/- 0.00 detection
Forced photometry filter KEPT candidate at 04:43:01.78 +43:37:41.4: ref_mag=13.29 +/- 0.02 new_mean_mag=12.0321 delta=1.26 (need > 0.90)
Forced photometry reference-image weighted average: 10.23 +/- 0.00
Forced photometry filter REJECTED candidate at 05:26:31.76 +41:11:14.5: ref_mag=10.23 +/- 0.00 new_mean_mag=11.3320 delta=-1.10 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:45:15.30 +50:17:11.2: 13.21 +/- 0.03 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:40:05.24 +49:46:42.7: 13.15 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Forced photometry filter KEPT candidate at 04:45:15.30 +50:17:11.2: ref_mag=13.19 +/- 0.02 new_mean_mag=12.1845 delta=1.01 (need > 0.90)
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Forced photometry filter KEPT candidate at 04:40:05.24 +49:46:42.7: ref_mag=13.16 +/- 0.02 new_mean_mag=12.1152 delta=1.04 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:32:37.07 +47:52:24.9: 13.09 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.02
Forced photometry filter KEPT candidate at 04:32:37.07 +47:52:24.9: ref_mag=13.11 +/- 0.02 new_mean_mag=12.1426 delta=0.96 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:59:15.44 +47:36:00.2: 13.09 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.02
Forced photometry filter KEPT candidate at 04:59:15.44 +47:36:00.2: ref_mag=13.10 +/- 0.02 new_mean_mag=11.9641 delta=1.14 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:30:32.94 +46:36:53.4: 13.09 +/- 0.03 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:30:32.94 +46:36:53.4: 13.11 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.02
Forced photometry filter KEPT candidate at 04:30:32.94 +46:36:53.4: ref_mag=13.10 +/- 0.02 new_mean_mag=12.1227 delta=0.98 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:48:41.06 +45:08:23.6: 13.07 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:48:41.06 +45:08:23.6: 13.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.02
Forced photometry filter KEPT candidate at 04:48:41.06 +45:08:23.6: ref_mag=13.10 +/- 0.02 new_mean_mag=12.0711 delta=1.03 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:31:10.10 +46:35:45.1: 13.02 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:31:10.10 +46:35:45.1: 13.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.01
Forced photometry filter KEPT candidate at 04:31:10.10 +46:35:45.1: ref_mag=13.02 +/- 0.01 new_mean_mag=12.0346 delta=0.98 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:46:57.75 +44:46:58.8: 13.04 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:34:23.18 +49:20:20.2: 13.04 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:46:57.75 +44:46:58.8: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.01
Forced photometry filter KEPT candidate at 04:46:57.75 +44:46:58.8: ref_mag=13.06 +/- 0.01 new_mean_mag=11.8686 delta=1.19 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:34:23.18 +49:20:20.2: 13.06 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Forced photometry filter KEPT candidate at 04:34:23.18 +49:20:20.2: ref_mag=13.05 +/- 0.02 new_mean_mag=12.1117 delta=0.94 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:02:33.10 +47:27:40.5: 13.06 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:02:33.10 +47:27:40.5: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Forced photometry filter KEPT candidate at 05:02:33.10 +47:27:40.5: ref_mag=13.09 +/- 0.02 new_mean_mag=11.9306 delta=1.16 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:36:32.49 +50:46:20.9: 13.03 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:36:32.49 +50:46:20.9: 13.04 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.02
Forced photometry filter KEPT candidate at 04:36:32.49 +50:46:20.9: ref_mag=13.03 +/- 0.02 new_mean_mag=11.9949 delta=1.04 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:55:11.20 +46:50:06.9: 13.01 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:55:11.20 +46:50:06.9: 13.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.01
Forced photometry filter KEPT candidate at 04:55:11.20 +46:50:06.9: ref_mag=13.01 +/- 0.01 new_mean_mag=11.9415 delta=1.07 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:32:10.65 +48:08:53.1: 13.00 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:32:10.65 +48:08:53.1: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.02
Forced photometry filter KEPT candidate at 04:32:10.65 +48:08:53.1: ref_mag=12.99 +/- 0.02 new_mean_mag=12.0342 delta=0.95 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:31:32.26 +49:30:02.1: 12.98 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:31:32.26 +49:30:02.1: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.02
Forced photometry filter KEPT candidate at 04:31:32.26 +49:30:02.1: ref_mag=12.97 +/- 0.02 new_mean_mag=11.9893 delta=0.99 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:32:44.83 +47:45:33.1: 12.95 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:32:44.83 +47:45:33.1: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.01
Forced photometry filter KEPT candidate at 04:32:44.83 +47:45:33.1: ref_mag=12.96 +/- 0.01 new_mean_mag=11.9750 delta=0.99 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:46:00.20 +49:15:33.2: 12.84 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:36:54.10 +48:06:53.7: 12.93 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:46:00.20 +49:15:33.2: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.01
Forced photometry filter KEPT candidate at 04:46:00.20 +49:15:33.2: ref_mag=12.81 +/- 0.01 new_mean_mag=11.7969 delta=1.02 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:36:54.10 +48:06:53.7: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.01
Forced photometry filter KEPT candidate at 04:36:54.10 +48:06:53.7: ref_mag=12.93 +/- 0.01 new_mean_mag=11.9890 delta=0.95 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:37:47.84 +42:27:39.4: 12.91 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:37:47.84 +42:27:39.4: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.02
Forced photometry filter KEPT candidate at 04:37:47.84 +42:27:39.4: ref_mag=12.92 +/- 0.02 new_mean_mag=11.6391 delta=1.28 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:46:33.63 +49:56:25.1: 12.89 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:46:33.63 +49:56:25.1: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.02
Forced photometry filter KEPT candidate at 04:46:33.63 +49:56:25.1: ref_mag=12.91 +/- 0.02 new_mean_mag=11.8487 delta=1.06 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:09:25.66 +47:08:49.0: 12.85 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:33:26.73 +47:26:26.0: 12.84 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:09:25.66 +47:08:49.0: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.01
Forced photometry filter KEPT candidate at 05:09:25.66 +47:08:49.0: ref_mag=12.84 +/- 0.01 new_mean_mag=11.8027 delta=1.04 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:33:26.73 +47:26:26.0: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.01
Forced photometry filter KEPT candidate at 04:33:26.73 +47:26:26.0: ref_mag=12.88 +/- 0.01 new_mean_mag=11.7824 delta=1.10 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:31:24.23 +45:07:47.6: 12.80 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:47:31.30 +50:21:21.2: 12.81 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:31:24.23 +45:07:47.6: 12.72 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.01
Forced photometry filter KEPT candidate at 04:31:24.23 +45:07:47.6: ref_mag=12.76 +/- 0.01 new_mean_mag=11.8120 delta=0.95 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:47:31.30 +50:21:21.2: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.01
Forced photometry filter KEPT candidate at 04:47:31.30 +50:21:21.2: ref_mag=12.80 +/- 0.01 new_mean_mag=11.7805 delta=1.02 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:05:06.63 +47:40:23.4: 12.79 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:05:06.63 +47:40:23.4: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.01
Forced photometry filter KEPT candidate at 05:05:06.63 +47:40:23.4: ref_mag=12.79 +/- 0.01 new_mean_mag=11.8146 delta=0.98 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:48:15.55 +49:48:51.0: 12.80 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:48:15.55 +49:48:51.0: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.01
Forced photometry filter KEPT candidate at 04:48:15.55 +49:48:51.0: ref_mag=12.82 +/- 0.01 new_mean_mag=11.8516 delta=0.96 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:44:52.94 +50:46:55.3: 12.75 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:44:52.94 +50:46:55.3: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.01
Forced photometry filter KEPT candidate at 04:44:52.94 +50:46:55.3: ref_mag=12.75 +/- 0.01 new_mean_mag=11.7894 delta=0.96 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:42:27.60 +48:57:35.0: 12.64 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:33:56.19 +41:01:55.1: 12.70 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:56:00.68 +45:05:25.3: 12.69 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:42:27.60 +48:57:35.0: 12.70 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.01
Forced photometry filter KEPT candidate at 04:42:27.60 +48:57:35.0: ref_mag=12.67 +/- 0.01 new_mean_mag=11.7187 delta=0.95 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:33:56.19 +41:01:55.1: 12.73 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:56:00.68 +45:05:25.3: 12.68 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.01
Forced photometry filter KEPT candidate at 04:33:56.19 +41:01:55.1: ref_mag=12.71 +/- 0.01 new_mean_mag=11.5602 delta=1.15 (need > 0.90)
Forced photometry reference-image weighted average: 12.69 +/- 0.01
Forced photometry filter KEPT candidate at 04:56:00.68 +45:05:25.3: ref_mag=12.69 +/- 0.01 new_mean_mag=11.7356 delta=0.95 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:38:35.39 +42:37:55.3: 12.65 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:16:27.62 +48:24:29.4: 12.65 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:38:35.39 +42:37:55.3: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.01
Forced photometry filter KEPT candidate at 04:38:35.39 +42:37:55.3: ref_mag=12.68 +/- 0.01 new_mean_mag=11.6357 delta=1.05 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:16:27.62 +48:24:29.4: 12.61 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Forced photometry filter KEPT candidate at 05:16:27.62 +48:24:29.4: ref_mag=12.63 +/- 0.01 new_mean_mag=11.6883 delta=0.94 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:38:31.93 +42:28:05.5: 12.63 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:38:31.93 +42:28:05.5: 12.58 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.01
Forced photometry filter KEPT candidate at 04:38:31.93 +42:28:05.5: ref_mag=12.60 +/- 0.01 new_mean_mag=11.5917 delta=1.01 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:48:04.79 +51:06:04.6: 12.62 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:48:04.79 +51:06:04.6: 12.63 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Forced photometry filter KEPT candidate at 04:48:04.79 +51:06:04.6: ref_mag=12.63 +/- 0.01 new_mean_mag=11.6794 delta=0.95 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:02:05.77 +47:33:20.1: 12.47 +/- 0.01 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:32:11.28 +49:29:06.5: 12.44 +/- 0.01 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:02:05.77 +47:33:20.1: 12.48 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.48 +/- 0.01
Forced photometry filter KEPT candidate at 05:02:05.77 +47:33:20.1: ref_mag=12.48 +/- 0.01 new_mean_mag=11.4552 delta=1.02 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:32:11.28 +49:29:06.5: 12.46 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.45 +/- 0.01
Forced photometry filter KEPT candidate at 04:32:11.28 +49:29:06.5: ref_mag=12.45 +/- 0.01 new_mean_mag=11.5376 delta=0.91 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:37:59.94 +43:15:28.5: 12.42 +/- 0.01 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:37:59.94 +43:15:28.5: 12.43 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.43 +/- 0.01
Forced photometry filter KEPT candidate at 04:37:59.94 +43:15:28.5: ref_mag=12.43 +/- 0.01 new_mean_mag=11.3492 delta=1.08 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:28:13.17 +41:56:04.1: 12.36 +/- 0.01 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:28:13.17 +41:56:04.1: 12.38 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.37 +/- 0.01
Forced photometry filter KEPT candidate at 04:28:13.17 +41:56:04.1: ref_mag=12.37 +/- 0.01 new_mean_mag=11.4396 delta=0.93 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:23:09.69 +41:43:07.7: 12.35 +/- 0.01 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:23:09.69 +41:43:07.7: 12.35 +/- 0.01 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:42:50.78 +50:46:14.7: 12.34 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.35 +/- 0.01
Forced photometry filter KEPT candidate at 04:23:09.69 +41:43:07.7: ref_mag=12.35 +/- 0.01 new_mean_mag=11.2863 delta=1.06 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:40:04.90 +41:04:20.1: 12.17 +/- 0.01 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:42:50.78 +50:46:14.7: 12.29 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.31 +/- 0.01
Forced photometry filter KEPT candidate at 04:42:50.78 +50:46:14.7: ref_mag=12.31 +/- 0.01 new_mean_mag=11.3696 delta=0.95 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:40:04.90 +41:04:20.1: 12.17 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.17 +/- 0.01
Forced photometry filter KEPT candidate at 04:40:04.90 +41:04:20.1: ref_mag=12.17 +/- 0.01 new_mean_mag=11.1649 delta=1.00 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:40:30.25 +43:11:52.8: 12.11 +/- 0.01 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:56:10.79 +46:41:27.9: 11.96 +/- 0.01 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:40:30.25 +43:11:52.8: 12.13 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.12 +/- 0.01
Forced photometry filter KEPT candidate at 04:40:30.25 +43:11:52.8: ref_mag=12.12 +/- 0.01 new_mean_mag=10.8698 delta=1.25 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:39:55.06 +49:45:11.7: 11.89 +/- 0.01 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:49:43.87 +45:47:29.4: 11.73 +/- 0.01 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:56:10.79 +46:41:27.9: 12.01 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.98 +/- 0.01
Forced photometry filter KEPT candidate at 04:56:10.79 +46:41:27.9: ref_mag=11.98 +/- 0.01 new_mean_mag=10.9928 delta=0.99 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:39:55.06 +49:45:11.7: 11.91 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.90 +/- 0.01
Forced photometry filter REJECTED candidate at 04:39:55.06 +49:45:11.7: ref_mag=11.90 +/- 0.01 new_mean_mag=11.0251 delta=0.88 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:49:43.87 +45:47:29.4: 11.71 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.72 +/- 0.00
Forced photometry filter KEPT candidate at 04:49:43.87 +45:47:29.4: ref_mag=11.72 +/- 0.00 new_mean_mag=10.7619 delta=0.96 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:10:55.29 +48:42:07.9: 11.66 +/- 0.01 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:13:46.66 +41:36:16.1: 11.53 +/- 0.01 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:10:55.29 +48:42:07.9: 11.64 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.65 +/- 0.00
Forced photometry filter KEPT candidate at 05:10:55.29 +48:42:07.9: ref_mag=11.65 +/- 0.00 new_mean_mag=10.6353 delta=1.01 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:13:46.66 +41:36:16.1: 11.54 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.53 +/- 0.00
Forced photometry filter KEPT candidate at 04:13:46.66 +41:36:16.1: ref_mag=11.53 +/- 0.00 new_mean_mag=10.5869 delta=0.94 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:22:53.21 +44:06:41.7: 11.32 +/- 0.01 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:22:53.21 +44:06:41.7: 11.32 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.32 +/- 0.00
Forced photometry filter KEPT candidate at 04:22:53.21 +44:06:41.7: ref_mag=11.32 +/- 0.00 new_mean_mag=10.3242 delta=1.00 (need > 0.90)
Adding exclusion_list_local.txt__out02877.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07488.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08012.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08329.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09120.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103754.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103994.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out105541.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out111228.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out126535.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135112.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13760.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out144114.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out145470.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14915.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out154649.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out155842.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167834.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168788.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173277.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out185020.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out185318.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out188807.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20260.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22049.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23282.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28365.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28622.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out30809.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31436.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35495.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36918.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38179.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out49553.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51647.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51695.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54836.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55844.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out57651.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out57751.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out57807.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out59241.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out62357.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out63615.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out65512.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72087.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75002.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78284.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78749.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out92588.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out92635.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 36s
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: 30s
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Considering the candidate 223889_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
The candidate 223889_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 223890_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
The candidate 223890_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 04:45:17.18 +49:15:54.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 223891_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
The candidate 223891_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 04:11:32.37 +49:09:46.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 223892_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
The candidate 223892_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
Rejecting candidate due to large distance (15.2") between the two second-epoch detections
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Considering the candidate 223925_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
The candidate 223925_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 04:23:59.85 +41:56:29.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 223952_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
The candidate 223952_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 04:43:31.92 +49:59:18.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 223959_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
The candidate 223959_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 05:06:37.15 +46:13:49.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 112681_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
The candidate 112681_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 04:59:06.15 +44:41:37.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65512_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 65512_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 215754_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
The candidate 215754_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 05:12:52.33 +46:43:03.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33869_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
The candidate 33869_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 04:39:41.66 +49:09:28.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67230_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
The candidate 67230_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 04:34:12.69 +47:15:37.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 25749_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
The candidate 25749_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 04:21:35.37 +49:37:17.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 49553_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 49553_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 09120_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 09120_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 137318_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
The candidate 137318_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
Rejecting candidate due to large distance (43.3") between the two second-epoch detections
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Considering the candidate 90264_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
The candidate 90264_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 04:28:44.17 +45:57:37.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 92635_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 92635_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 135112_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 135112_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 174616_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
The candidate 174616_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 14915_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 14915_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 23282_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 23282_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 55844_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 55844_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 57751_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 57751_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 78284_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 78284_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 103994_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 103994_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 10149_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
The candidate 10149_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 04:45:26.28 +50:36:37.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78749_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 78749_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 111228_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 111228_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 30809_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 30809_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 59241_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 59241_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 08329_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 08329_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 16061_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
The candidate 16061_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 04:25:28.85 +50:14:23.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93325_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
The candidate 93325_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 04:52:33.26 +45:41:38.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72087_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 72087_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 51695_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 51695_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 28365_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 28365_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 57807_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 57807_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 31436_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 31436_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 51647_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 51647_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 185318_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 185318_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 20260_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 20260_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 187518_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
The candidate 187518_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 04:41:48.81 +42:34:53.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 62357_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 62357_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 63615_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 63615_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 52822_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
The candidate 52822_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 05:11:33.61 +47:40:46.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105541_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 105541_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 13760_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 13760_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 54836_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 54836_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 22049_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 22049_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 98748_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
The candidate 98748_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 05:02:48.47 +45:16:20.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 07488_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 07488_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 06844_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
The candidate 06844_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 05:27:03.86 +50:07:25.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 36918_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 36918_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 154649_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 154649_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 103754_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 103754_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 188807_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 188807_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 38179_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 38179_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 185020_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 185020_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 02877_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 02877_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 137331_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
The candidate 137331_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 04:39:53.36 +43:33:31.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 121914_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
The candidate 121914_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 04:23:41.43 +44:16:48.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57651_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 57651_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 28622_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 28622_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 144114_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 144114_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 173277_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 173277_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 168788_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 168788_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 64981_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
The candidate 64981_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 05:03:12.46 +47:09:04.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 156003_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
The candidate 156003_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 04:20:52.64 +41:03:31.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 08012_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 08012_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 51769_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
The candidate 51769_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 04:33:43.75 +48:06:53.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 155842_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 155842_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 168590_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
The candidate 168590_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 05:04:44.11 +41:24:17.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31765_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
The candidate 31765_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 04:51:30.75 +49:14:10.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 06031_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
The candidate 06031_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 04:36:18.02 +50:56:45.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 145470_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 145470_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 60260_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
The candidate 60260_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 04:48:11.58 +47:38:29.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75002_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 75002_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 24390_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
The candidate 24390_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 92588_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 92588_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 35495_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 35495_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 167834_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 167834_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 95776_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
The candidate 95776_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 04:32:36.78 +45:40:13.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 126535_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 126535_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 21271_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
The candidate 21271_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 04:54:15.05 +49:54:00.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 50556_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
The candidate 50556_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 04:41:24.27 +48:17:58.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 143340_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
The candidate 143340_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 04:42:54.43 +43:21:55.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 131779_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
The candidate 131779_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 05:01:57.75 +43:49:24.7 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 146564_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
The candidate 146564_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 04:33:24.94 +43:03:50.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 83998_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
The candidate 83998_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 05:16:41.09 +45:59:38.8 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 82040_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
The candidate 82040_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 04:21:33.44 +46:29:54.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 145826_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
The candidate 145826_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 05:02:28.44 +41:04:34.7 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 58324_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
The candidate 58324_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 04:08:39.89 +47:42:43.4 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 155855_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
The candidate 155855_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 04:36:41.49 +41:15:55.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 145464_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
The candidate 145464_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 05:18:15.65 +42:47:30.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 161730_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
The candidate 161730_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 05:06:30.67 +41:14:03.6 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 49450_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287
The candidate 49450_fd_Per-03-Q1b1x1_2026-08-06_02-41-16_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 04:14:54.13 +48:24:31.8 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 4s
make_report_in_HTML.sh TOTAL: 70s
Prepared the HTML report for the field Per-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
04:48:04.79 +51:06:04.6
04:44:52.94 +50:46:55.3
04:42:50.78 +50:46:14.7
04:36:32.49 +50:46:20.9
04:41:16.64 +50:40:21.5
04:56:00.68 +45:05:25.3
04:48:41.06 +45:08:23.6
04:31:24.23 +45:07:47.6
04:46:57.75 +44:46:58.8
04:22:53.21 +44:06:41.7
04:43:01.78 +43:37:41.4
04:47:31.30 +50:21:21.2
04:37:59.94 +43:15:28.5
04:40:30.25 +43:11:52.8
04:45:15.30 +50:17:11.2
04:33:56.19 +41:01:55.1
04:40:04.90 +41:04:20.1
04:13:46.66 +41:36:16.1
04:23:09.69 +41:43:07.7
04:28:13.17 +41:56:04.1
04:38:31.93 +42:28:05.5
04:37:47.84 +42:27:39.4
04:38:35.39 +42:37:55.3
04:46:33.63 +49:56:25.1
04:48:15.55 +49:48:51.0
04:40:05.24 +49:46:42.7
04:31:32.26 +49:30:02.1
04:32:11.28 +49:29:06.5
04:34:23.18 +49:20:20.2
04:46:00.20 +49:15:33.2
05:10:55.29 +48:42:07.9
04:42:27.60 +48:57:35.0
05:16:27.62 +48:24:29.4
04:37:19.69 +48:15:49.5
04:36:54.10 +48:06:53.7
04:32:10.65 +48:08:53.1
05:05:06.63 +47:40:23.4
04:32:37.07 +47:52:24.9
05:02:05.77 +47:33:20.1
04:59:15.44 +47:36:00.2
04:32:44.83 +47:45:33.1
05:02:33.10 +47:27:40.5
05:09:25.66 +47:08:49.0
04:33:26.73 +47:26:26.0
05:08:31.68 +47:00:06.3
04:55:11.20 +46:50:06.9
04:56:10.79 +46:41:27.9
04:30:32.94 +46:36:53.4
04:31:10.10 +46:35:45.1
04:49:43.87 +45:47:29.4
04:33:21.52 +45:50:52.4
########### Completed Per-03-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
05:08:31.68 +47:00:06.3
04:37:19.69 +48:15:49.5
04:41:16.64 +50:40:21.5
04:33:21.52 +45:50:52.4
04:43:01.78 +43:37:41.4
04:45:15.30 +50:17:11.2
04:40:05.24 +49:46:42.7
04:32:37.07 +47:52:24.9
04:59:15.44 +47:36:00.2
04:30:32.94 +46:36:53.4
04:48:41.06 +45:08:23.6
04:31:10.10 +46:35:45.1
04:46:57.75 +44:46:58.8
04:34:23.18 +49:20:20.2
05:02:33.10 +47:27:40.5
04:36:32.49 +50:46:20.9
04:55:11.20 +46:50:06.9
04:32:10.65 +48:08:53.1
04:31:32.26 +49:30:02.1
04:32:44.83 +47:45:33.1
04:46:00.20 +49:15:33.2
04:36:54.10 +48:06:53.7
04:37:47.84 +42:27:39.4
04:46:33.63 +49:56:25.1
05:09:25.66 +47:08:49.0
04:33:26.73 +47:26:26.0
04:31:24.23 +45:07:47.6
04:47:31.30 +50:21:21.2
05:05:06.63 +47:40:23.4
04:48:15.55 +49:48:51.0
04:44:52.94 +50:46:55.3
04:42:27.60 +48:57:35.0
04:33:56.19 +41:01:55.1
04:56:00.68 +45:05:25.3
04:38:35.39 +42:37:55.3
05:16:27.62 +48:24:29.4
04:38:31.93 +42:28:05.5
04:48:04.79 +51:06:04.6
05:02:05.77 +47:33:20.1
04:32:11.28 +49:29:06.5
04:37:59.94 +43:15:28.5
04:28:13.17 +41:56:04.1
04:23:09.69 +41:43:07.7
04:42:50.78 +50:46:14.7
04:40:04.90 +41:04:20.1
04:40:30.25 +43:11:52.8
04:56:10.79 +46:41:27.9
04:49:43.87 +45:47:29.4
05:10:55.29 +48:42:07.9
04:13:46.66 +41:36:16.1
04:22:53.21 +44:06:41.7
###################################################################################
05:08:31.68 +47:00:06.3 -- not an asteroid (will add it to exclusion list)
04:37:19.69 +48:15:49.5 -- not an asteroid (will add it to exclusion list)
04:41:16.64 +50:40:21.5 -- not an asteroid (will add it to exclusion list)
04:33:21.52 +45:50:52.4 -- not an asteroid (will add it to exclusion list)
04:43:01.78 +43:37:41.4 -- not an asteroid (will add it to exclusion list)
04:45:15.30 +50:17:11.2 -- not an asteroid (will add it to exclusion list)
04:40:05.24 +49:46:42.7 -- not an asteroid (will add it to exclusion list)
04:32:37.07 +47:52:24.9 -- not an asteroid (will add it to exclusion list)
04:59:15.44 +47:36:00.2 -- not an asteroid (will add it to exclusion list)
04:30:32.94 +46:36:53.4 -- not an asteroid (will add it to exclusion list)
04:48:41.06 +45:08:23.6 -- not an asteroid (will add it to exclusion list)
04:31:10.10 +46:35:45.1 -- not an asteroid (will add it to exclusion list)
04:46:57.75 +44:46:58.8 -- not an asteroid (will add it to exclusion list)
04:34:23.18 +49:20:20.2 -- not an asteroid (will add it to exclusion list)
05:02:33.10 +47:27:40.5 -- not an asteroid (will add it to exclusion list)
04:36:32.49 +50:46:20.9 -- not an asteroid (will add it to exclusion list)
04:55:11.20 +46:50:06.9 -- not an asteroid (will add it to exclusion list)
04:32:10.65 +48:08:53.1 -- not an asteroid (will add it to exclusion list)
04:31:32.26 +49:30:02.1 -- not an asteroid (will add it to exclusion list)
04:32:44.83 +47:45:33.1 -- not an asteroid (will add it to exclusion list)
04:46:00.20 +49:15:33.2 -- not an asteroid (will add it to exclusion list)
04:36:54.10 +48:06:53.7 -- not an asteroid (will add it to exclusion list)
04:37:47.84 +42:27:39.4 -- not an asteroid (will add it to exclusion list)
04:46:33.63 +49:56:25.1 -- not an asteroid (will add it to exclusion list)
05:09:25.66 +47:08:49.0 -- not an asteroid (will add it to exclusion list)
04:33:26.73 +47:26:26.0 -- not an asteroid (will add it to exclusion list)
04:31:24.23 +45:07:47.6 -- not an asteroid (will add it to exclusion list)
04:47:31.30 +50:21:21.2 -- not an asteroid (will add it to exclusion list)
05:05:06.63 +47:40:23.4 -- not an asteroid (will add it to exclusion list)
04:48:15.55 +49:48:51.0 -- not an asteroid (will add it to exclusion list)
04:44:52.94 +50:46:55.3 -- not an asteroid (will add it to exclusion list)
04:42:27.60 +48:57:35.0 -- not an asteroid (will add it to exclusion list)
04:33:56.19 +41:01:55.1 -- not an asteroid (will add it to exclusion list)
04:56:00.68 +45:05:25.3 -- not an asteroid (will add it to exclusion list)
04:38:35.39 +42:37:55.3 -- not an asteroid (will add it to exclusion list)
05:16:27.62 +48:24:29.4 -- not an asteroid (will add it to exclusion list)
04:38:31.93 +42:28:05.5 -- not an asteroid (will add it to exclusion list)
04:48:04.79 +51:06:04.6 -- not an asteroid (will add it to exclusion list)
05:02:05.77 +47:33:20.1 -- not an asteroid (will add it to exclusion list)
04:32:11.28 +49:29:06.5 -- not an asteroid (will add it to exclusion list)
04:37:59.94 +43:15:28.5 -- not an asteroid (will add it to exclusion list)
04:28:13.17 +41:56:04.1 -- not an asteroid (will add it to exclusion list)
04:23:09.69 +41:43:07.7 -- not an asteroid (will add it to exclusion list)
04:42:50.78 +50:46:14.7 -- not an asteroid (will add it to exclusion list)
04:40:04.90 +41:04:20.1 -- not an asteroid (will add it to exclusion list)
04:40:30.25 +43:11:52.8 -- not an asteroid (will add it to exclusion list)
04:56:10.79 +46:41:27.9 -- not an asteroid (will add it to exclusion list)
04:49:43.87 +45:47:29.4 -- not an asteroid (will add it to exclusion list)
05:10:55.29 +48:42:07.9 -- not an asteroid (will add it to exclusion list)
04:13:46.66 +41:36:16.1 -- not an asteroid (will add it to exclusion list)
04:22:53.21 +44:06:41.7 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
04:13:46.66 +41:36:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:22:53.21 +44:06:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:23:09.69 +41:43:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:28:13.17 +41:56:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:30:32.94 +46:36:53.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:31:10.10 +46:35:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:31:24.23 +45:07:47.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:31:32.26 +49:30:02.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:32:10.65 +48:08:53.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:32:11.28 +49:29:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:32:37.07 +47:52:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:32:44.83 +47:45:33.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:33:21.52 +45:50:52.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:33:26.73 +47:26:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:33:56.19 +41:01:55.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:34:23.18 +49:20:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:36:32.49 +50:46:20.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:36:54.10 +48:06:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:37:19.69 +48:15:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:37:47.84 +42:27:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:37:59.94 +43:15:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:38:31.93 +42:28:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:38:35.39 +42:37:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:40:04.90 +41:04:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:40:05.24 +49:46:42.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:40:30.25 +43:11:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:41:16.64 +50:40:21.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:42:27.60 +48:57:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:42:50.78 +50:46:14.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:43:01.78 +43:37:41.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:44:52.94 +50:46:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:45:15.30 +50:17:11.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:46:00.20 +49:15:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:46:33.63 +49:56:25.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:46:57.75 +44:46:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:47:31.30 +50:21:21.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:48:04.79 +51:06:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:48:15.55 +49:48:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:48:41.06 +45:08:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:49:43.87 +45:47:29.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:11.20 +46:50:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:00.68 +45:05:25.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:10.79 +46:41:27.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:15.44 +47:36:00.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:02:05.77 +47:33:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:02:33.10 +47:27:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:05:06.63 +47:40:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:08:31.68 +47:00:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:09:25.66 +47:08:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:10:55.29 +48:42:07.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:16:27.62 +48:24:29.4 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
04:13:46.66 +41:36:16.1 -- a known variable star
04:22:53.21 +44:06:41.7 -- a known variable star
04:23:09.69 +41:43:07.7 -- a known variable star
04:28:13.17 +41:56:04.1 -- a known variable star
04:30:32.94 +46:36:53.4 -- not a known variable star
04:31:10.10 +46:35:45.1 -- not a known variable star
04:31:24.23 +45:07:47.6 -- a known variable star
04:31:32.26 +49:30:02.1 -- not a known variable star
04:32:10.65 +48:08:53.1 -- a known variable star
04:32:11.28 +49:29:06.5 -- a known variable star
04:32:37.07 +47:52:24.9 -- not a known variable star
04:32:44.83 +47:45:33.1 -- not a known variable star
04:33:21.52 +45:50:52.4 -- a known variable star
04:33:26.73 +47:26:26.0 -- a known variable star
04:33:56.19 +41:01:55.1 -- a known variable star
04:34:23.18 +49:20:20.2 -- not a known variable star
04:36:32.49 +50:46:20.9 -- not a known variable star
04:36:54.10 +48:06:53.7 -- not a known variable star
04:37:19.69 +48:15:49.5 -- a known variable star
04:37:47.84 +42:27:39.4 -- a known variable star
04:37:59.94 +43:15:28.5 -- a known variable star
04:38:31.93 +42:28:05.5 -- a known variable star
04:38:35.39 +42:37:55.3 -- not a known variable star
04:40:04.90 +41:04:20.1 -- a known variable star
04:40:05.24 +49:46:42.7 -- not a known variable star
04:40:30.25 +43:11:52.8 -- a known variable star
04:41:16.64 +50:40:21.5 -- not a known variable star
04:42:27.60 +48:57:35.0 -- not a known variable star
04:42:50.78 +50:46:14.7 -- a known variable star
04:43:01.78 +43:37:41.4 -- not a known variable star
04:44:52.94 +50:46:55.3 -- a known variable star
04:45:15.30 +50:17:11.2 -- a known variable star
04:46:00.20 +49:15:33.2 -- a known variable star
04:46:33.63 +49:56:25.1 -- a known variable star
04:46:57.75 +44:46:58.8 -- a known variable star
04:47:31.30 +50:21:21.2 -- a known variable star
04:48:04.79 +51:06:04.6 -- a known variable star
04:48:15.55 +49:48:51.0 -- not a known variable star
04:48:41.06 +45:08:23.6 -- not a known variable star
04:49:43.87 +45:47:29.4 -- a known variable star
04:55:11.20 +46:50:06.9 -- a known variable star
04:56:00.68 +45:05:25.3 -- a known variable star
04:56:10.79 +46:41:27.9 -- a known variable star
04:59:15.44 +47:36:00.2 -- a known variable star
05:02:05.77 +47:33:20.1 -- a known variable star
05:02:33.10 +47:27:40.5 -- a known variable star
05:05:06.63 +47:40:23.4 -- a known variable star
05:08:31.68 +47:00:06.3 -- a known variable star
05:09:25.66 +47:08:49.0 -- a known variable star
05:10:55.29 +48:42:07.9 -- a known variable star
05:16:27.62 +48:24:29.4 -- a known variable star
Found 15 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
51 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 51 (excluding asteroids and hot pixels, 15 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461258.81983845 -observatory V36
07:46:12.08 +20:23:19.7 Mercury (-0.3mag)
11:56:02.80 -00:06:56.9 Venus (-4.3mag)
05:43:44.09 +23:32:52.0 Mars (1.3mag)
08:41:13.62 +18:47:38.2 Jupiter (-1.8mag)
00:56:32.61 +03:16:43.1 Saturn (0.6mag)
04:11:30.46 +20:56:22.5 Uranus (5.8mag)
00:16:12.47 +00:13:56.4 Neptune (7.7mag)
20:28:19.41 -23:29:26.7 Pluto (14.4mag)
02:52:52.68 +21:13:06.6 Moon (-10.3mag)
-rw-r--r-- 1 apache apache 363 Aug 6 02:45 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461258.81983845:
08:41:19.17 +18:47:14.3 Io (6.0mag)
08:41:08.87 +18:47:59.1 Europa (6.3mag)
08:41:11.48 +18:47:51.3 Ganymede (5.6mag)
08:41:00.75 +18:48:36.4 Callisto (6.7mag)
08:38:49.38 +18:45:51.7 Himalia (15.7mag)
08:41:12.39 +18:47:43.9 Thebe (16.6mag)
08:38:20.09 +18:44:45.8 Elara (17.7mag)
08:45:19.57 +18:28:00.0 Pasiphae (17.9mag)
08:44:32.03 +18:57:29.9 Carme (19.0mag)
00:56:29.88 +03:17:10.2 Titan (8.4mag)
00:56:26.67 +03:16:45.3 Rhea (9.7mag)
00:56:36.53 +03:15:06.3 Iapetus (11.1mag)
00:56:18.99 +03:16:56.5 Hyperion (14.4mag)
00:55:57.51 +03:10:09.0 Phoebe (16.5mag)
-rw-r--r-- 1 apache apache 568 Aug 6 02:45 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461258.81983845:
18:55:28.90 -23:59:27.5 JWST
17:19:49.75 +39:11:27.1 Chandra
10:16:14.48 -57:08:58.3 XMM-Newton
-rw-r--r-- 1 apache apache 96 Aug 6 02:45 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461258.81983845 -observatory V36
03:11:30.23 +17:12:58.3 17.7mag P/1996 R2 (Lagerkvist)
18:02:22.50 -34:38:21.7 14.0mag P/2010 H2 (Vales)
06:52:00.63 -68:49:52.2 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:09:18.68 +32:57:12.8 17.7mag C/2017 K2 (PANSTARRS)
03:38:01.58 +36:46:54.2 16.7mag P/2021 N1 (ZTF)
22:40:11.87 +31:33:36.6 17.3mag C/2022 E2 (ATLAS)
06:41:34.90 +26:34:25.7 16.8mag C/2022 N2 (PANSTARRS)
10:19:48.46 +28:33:18.9 17.0mag C/2022 QE78 (ATLAS)
09:27:35.07 +05:17:44.6 17.9mag C/2022 R6 (PANSTARRS)
15:12:10.04 -12:12:41.8 17.9mag P/2023 B1 (PANSTARRS)
21:13:16.98 +66:13:18.7 17.9mag C/2023 H5 (Lemmon)
15:49:47.99 -12:45:29.4 14.3mag C/2023 R1 (PANSTARRS)
08:05:56.96 +31:15:36.6 15.2mag C/2024 E1 (Wierzchos)
15:07:16.68 +15:36:57.7 17.7mag C/2024 G6 (ATLAS)
19:05:32.74 +42:58:05.5 13.7mag C/2024 J3 (ATLAS)
21:13:31.47 +49:05:07.2 17.6mag C/2024 R4 (PANSTARRS)
05:13:36.19 -12:59:33.4 15.5mag C/2024 T5 (ATLAS)
06:54:58.88 +24:29:27.6 17.9mag C/2025 J1 (Borisov)
07:29:59.64 -15:52:48.1 17.7mag C/2025 R3 (PANSTARRS)
10:30:15.61 +21:01:30.4 17.3mag C/2025 V2 (Rankin)
12:56:59.84 +02:28:32.7 17.0mag C/2025 Y1 (ATLAS)
16:03:39.34 +78:00:33.9 16.8mag C/2026 A2 (Bok)
03:06:45.49 +46:08:51.6 17.1mag C/2026 B2 (Sun-Gao)
11:45:13.61 +08:20:35.4 17.3mag A/2026 E1
21:56:12.87 -26:29:53.9 6.9mag 10P/Tempel
11:27:49.47 -03:16:56.2 16.2mag 29P/Schwassmann-Wachmann
04:36:52.74 +32:16:16.4 18.0mag 47P/Ashbrook-Jackson
11:03:48.39 +05:15:54.2 17.2mag 63P/Wild
00:54:17.77 -05:22:54.4 15.4mag 65P/Gunn
05:31:13.38 +20:43:42.6 13.7mag 78P/Gehrels
20:39:42.05 -23:18:12.6 17.8mag 84P/Giclas
02:58:49.53 +13:32:50.7 16.7mag 88P/Howell
07:51:00.83 +27:54:57.2 16.1mag 93P/Lovas
04:01:00.02 +16:08:02.2 17.6mag 112P/Urata-Niijima
05:50:11.34 +30:30:20.9 16.3mag 114P/Wiseman-Skiff
09:13:58.66 +26:58:12.4 15.0mag 123P/West-Hartley
11:39:55.56 -09:32:07.4 17.1mag 124P/Mrkos
05:33:44.49 +21:11:10.3 16.1mag 128P/Shoemaker-Holt
06:25:15.09 +18:59:30.5 17.9mag 131P/Mueller
00:03:41.04 +03:25:19.8 17.6mag 139P/Vaisala-Oterma
03:21:32.74 -19:44:41.8 14.0mag 161P/Hartley-IRAS
07:09:34.55 +37:41:45.6 15.8mag 162P/SidingSpring
15:48:15.99 +39:34:12.3 12.3mag 169P/NEAT
02:39:29.26 +09:28:40.3 17.6mag 220P/McNaught
16:40:37.98 -09:57:04.5 17.7mag 235P/LINEAR
20:23:39.38 -52:50:57.2 17.8mag 259P/Garradd
03:16:33.93 +24:21:40.5 15.4mag 260P/McNaught
06:59:37.76 +37:45:12.3 17.3mag 295P/LINEAR
15:09:52.67 +03:20:54.3 17.7mag 391P/Kowalski
08:59:08.98 +18:28:09.7 17.9mag 450P/LONEOS
-rw-r--r-- 1 apache apache 2.5K Aug 6 02:45 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
22:08:07.63 -53:03:58.90 AT2026wek 2026-08-3.82 17.17
14:51:51.34 +66:13:24.60 ASASSN-26ev 2026-08-2.15 14.02
12:06:50.79 -36:16:06.20 SN2026wgm 2026-08-1.73 15.61
16:56:36.90 -59:29:26.00 ASASSN-26er 2026-07-25.82 15.09
01:21:27.83 -10:37:05.00 SN2026vbh 2026-07-25.61 15.97
21:17:31.59 +22:25:50.90 ASASSN-26eq 2026-07-24.37 15.13
18:53:36.89 +16:56:43.60 ASASSN-26ep 2026-07-23.47 -4.06
12:18:47.98 -30:48:47.50 ASASSN-26et 2026-07-22.76 13.98
13:00:47.82 +15:42:17.60 SN2026uwk 2026-07-21.75 16.38
18:52:31.11 -32:28:00.90 ASASSN-26en 2026-07-21.77 14.63
14:42:58.01 -62:32:59.10 ASASSN-26es 2026-07-20.79 15.36
20:12:45.57 -32:53:13.00 ASASSN-26em 2026-07-20.94 16.83
18:54:24.33 -46:11:51.70 ASASSN-26eu 2026-07-20.93 14.86
03:18:56.99 -80:55:10.40 AT2026ugi 2026-07-20.03 17.12
18:43:58.40 +24:22:41.80 ASASSN-26eo 2026-07-19.36 16.16
04:50:01.03 -02:22:33.80 ASASSN-26ej 2026-07-16.17 17.02
18:34:55.28 -31:41:00.90 ASASSN-26ek 2026-07-16.24 15.73
17:07:43.61 -44:21:53.50 ASASSN-26el 2026-07-15.86 16.01
14:45:08.35 +24:13:12.30 ASASSN-26ei 2026-07-16.17 16.46
10:00:46.44 -32:36:31.10 AT 2023mhb 2026-07-14.73 16.67
14:39:37.45 -11:22:36.20 AT 2026unl 2026-07-15.27 17.11
10:49:42.57 -11:25:55.80 ASASSN-26eh 2026-07-14.72 16.58
19:33:53.06 -07:15:00.80 ASASSN-22le 2026-07-14.15 15.5
02:45:40.52 -27:55:30.30 ASASSN-26ef 2026-07-12.35 15.86
23:26:43.80 +04:42:39.70 SN 2026qtn 2026-07-12.22 16.47
02:19:17.26 +28:57:15.40 ASASSN-26ec 2026-07-11.53 2.78
18:31:15.56 -05:34:31.50 AT2026stb 2026-07-11.28 -1.29
13:36:08.24 +23:29:05.00 AT2026pjf 2026-07-10.18 -0.72
17:33:39.82 +04:22:36.70 SN2026pir 2026-07-9.86 -0.66
11:21:41.26 -50:33:36.30 ASASSN-26ed 2026-07-8.8 -1.3
23:41:42.11 +26:29:49.10 AT2026qil 2026-07-9.3 16.15
20:21:30.50 -32:03:40.10 ASASSN-26ee 2026-07-7.22 15.53
19:37:44.09 -05:35:42.80 AT2026ryu 2026-07-7.17 14.88
11:06:55.46 -04:07:04.50 AT2026qqg 2026-07-5.01 16.82
19:07:23.69 -74:13:37.30 AT2026qly 2026-07-5.02 17.31
17:57:43.80 +27:18:40.10 ASASSN-26ea 2026-07-5.07 16.67
19:59:01.43 -32:07:34.30 ASASSN-26eb 2026-07-4.97 15.52
18:46:50.35 -57:44:13.20 SN 2026qqp 2026-07-5.03 -0.92
19:17:31.69 -39:55:29.90 ASASSN-26dz 2026-07-5.14 15.91
19:14:31.37 +12:03:52.90 AT 2026rdg 2026-07-3.43 11.81
04:05:50.09 -70:24:34.40 AT 2026qpr 2026-06-30.4 15.96
13:45:37.49 -05:59:35.80 SN 2026pub 2026-06-30.09 16.01
16:41:15.63 +39:17:14.70 SN 2026pel 2026-06-26.38 16.07
10:14:40.19 -35:38:21.30 ASASSN-26dy 2026-06-25.99 15.63
14:47:21.56 -40:15:51.30 ASASSN-26dv 2026-06-23.03 14.62
13:38:49.79 -77:21:06.70 ASASSN-26dw 2026-06-23.04 16.09
00:59:27.90 +33:08:13.20 SN 2026mke 2026-06-22.39 17.13
11:10:44.73 -30:20:45.50 SN 2026nmv 2026-06-22.06 16.56
21:36:15.68 -21:19:12.50 AT2026oxh 2026-06-22.15 17.14
17:31:38.38 -56:05:51.90 ASASSN-26dx 2026-06-22.02 14.72
14:10:13.44 -38:46:46.10 AT2026pvk 2026-06-22.06 16.53
20:56:47.23 -18:31:05.20 AT2026plb 2026-06-21.31 16.4
15:44:29.68 +21:00:59.30 SN2026ore 2026-06-21.29 17.57
23:50:05.98 -14:01:41.30 AT2026oxl 2026-06-21.52 17.64
17:36:54.73 -18:10:04.20 AT2026ouj 2026-06-20.92 15.15
00:34:04.08 -30:22:09.20 AT2026ntk 2026-06-18.09 17.34
20:49:13.39 +25:17:59.20 ASASSN-26du 2026-06-15.39 15.93
23:09:30.84 +32:40:42.00 SN2026oxc 2026-06-14.35 16.83
02:02:26.67 +32:04:22.70 AT2026ovz 2026-06-14.6 15.52
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:33.11 -68:48:32.90 ASASSN-26no 2026-05-24.03 8.35
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.72 -58:37:47.60 ASASSN-26dn 2026-05-20.01 14.64
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.28 +22:02:03.40 AT2026lxf 2026-05-8.07 13.88
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:49.13 -61:36:14.60 ASASSN-26dd 2026-05-5.15 15.93
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
-rw-r--r-- 1 apache apache 5.7K Aug 6 02:45 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
12:24:25.10 +28:47:12.0 TCP J12242510+2847120 2026-05-31.6015 14.8mag
00:56:07.13 +43:01:40.6 TCP J00560713+4301406 2026-06-01.4135 12.2mag
00:42:41.64 +41:15:16.2 PNV J00424164+4115162 2026-06-02.029 17.4mag
00:42:38.68 +41:15:58.2 PNV J00423868+4115582 2026-06-05.1224 19.97Umag
19:00:42.95 -48:31:01.7 PNV J19004295-4831017 2026-05-25.0752 14.2mag
09:55:21.28 +69:02:52.6 PNV J09552128+6902526 2026-06-13.933 18.9mag
19:51:21.42 +37:06:40.0 TCP J19512142+3706400 2026-06-17.2942 16.8mag
19:57:03.87 +37:41:46.4 TCP J19570387+3741464 2026-06-18.2638 17.5mag
00:42:32.04 +41:10:28.3 PNV J00423204+4110283 2026-06-26.059 16.6mag
02:19:17.36 +28:57:15.8 TCP J02191736+2857158 2026-07-12.3549 12.5mag
00:44:56.43 +41:57:41.6 PNV J00445643+4157416 2026-07-13.8026 17.98Cmag
00:42:55.36 +41:17:27.0 PNV J00425536+4117270 2026-07-20.1813 17.7mag
20:35:43.64 +61:31:32.9 TCP J20354364+6131329 2026-07-20.5443 14.4mag
21:17:31.48 +22:25:51.0 TCP J21173148+2225510 2026-07-23.5577 14.8mag
00:41:24.04 +40:49:02.8 PNV J00412404+4049028 2026-07-25.0157 18.7mag
00:43:04.26 +41:02:28.6 PNV J00430426+4102286 2026-07-26.1512 20mag
14:51:51.40 +66:13:24.0 TCP J14515140+6613240 2026-07-29.2561 13.5mag
00:43:06.15 +41:22:08.2 PNV J00430615+4122082 2026-07-30.0085 19.4mag
00:41:33.23 +41:10:12.2 PNV J00413323+4110122 2026-08-02.8913 17.1mag
-rw-r--r-- 1 apache apache 189K Aug 6 02:45 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
09:39:31.292 -08:28:35.35 AT 2026vla 2026-02-21.40 20.65
17:07:24.157 +32:28:59.94 AT 2026vkz 2026-06-16.33 21.89
18:55:34.805 +34:42:05.78 AT 2026vky 2026-06-22.39 21.01
15:27:13.875 -10:50:21.14 AT 2026vkx 2026-06-14.35 20.55
13:36:43.476 +25:28:01.16 AT 2026vkw 2026-06-25.38 20.6
04:43:04.292 -16:08:54.64 AT 2026vkv 2026-01-12.30 21.72
04:48:25.928 -18:19:58.05 AT 2026vku 2026-01-26.25 21.35
12:55:24.686 +13:58:33.13 AT 2026vkt 2026-06-05.34 21.42
11:39:28.884 +47:23:59.43 AT 2026vks 2026-01-14.61 21.82
10:26:55.799 -14:09:20.42 AT 2026vkr 2026-01-13.55 21.98
12:26:22.284 +20:06:25.68 AT 2026vkq 2026-02-13.60 20.86
12:08:12.778 +41:30:56.83 AT 2026vkp 2026-06-15.27 20.88
05:11:50.298 -12:02:24.75 AT 2026vko 2026-02-15.23 20.49
00:35:37.087 -45:29:22.45 AT 2026vkn 2026-06-26.42 23.13
04:11:06.535 -49:23:35.67 AT 2026vkm 2026-07-09.42 22.31
23:40:19.411 -26:01:53.34 AT 2026vkl 2026-07-20.59 21.47
22:23:27.160 +00:54:32.97 AT 2026vkk 2026-07-14.55 21.17
21:14:05.875 -09:55:36.50 AT 2026vkj 2026-07-20.46 21.9
17:17:56.970 +19:09:32.22 AT 2026vki 2026-07-19.39 21.8
17:18:18.165 +24:21:20.44 AT 2026vkh 2026-07-19.40 21.78
-rw-r--r-- 1 apache apache 87K Aug 6 02:45 tns_transients_list.txt
