Started working on galaxy PGC032779_GROUP at Thu Jun 18 17:11:08 2020 Read 2 galaxy(ies) from /global/cscratch1/sd/ioannis/SGA-data-dr9alpha/163/PGC032779_GROUP/PGC032779_GROUP-largegalaxy-sample.fits Reading /global/cscratch1/sd/ioannis/SGA-data-dr9alpha/163/PGC032779_GROUP/PGC032779_GROUP-largegalaxy-tractor.fits Read 274 sources from /global/cscratch1/sd/ioannis/SGA-data-dr9alpha/163/PGC032779_GROUP/PGC032779_GROUP-largegalaxy-tractor.fits Reading /global/cscratch1/sd/ioannis/SGA-data-dr9alpha/163/PGC032779_GROUP/PGC032779_GROUP-largegalaxy-maskbits.fits.fz Sort by flux! [ 3981.0881 1159.1737] Reading /global/cscratch1/sd/ioannis/SGA-data-dr9alpha/163/PGC032779_GROUP/PGC032779_GROUP-largegalaxy-image-g.fits.fz Reading /global/cscratch1/sd/ioannis/SGA-data-dr9alpha/163/PGC032779_GROUP/PGC032779_GROUP-largegalaxy-model-g.fits.fz Reading /global/cscratch1/sd/ioannis/SGA-data-dr9alpha/163/PGC032779_GROUP/PGC032779_GROUP-largegalaxy-invvar-g.fits.fz Reading /global/cscratch1/sd/ioannis/SGA-data-dr9alpha/163/PGC032779_GROUP/PGC032779_GROUP-largegalaxy-image-r.fits.fz Reading /global/cscratch1/sd/ioannis/SGA-data-dr9alpha/163/PGC032779_GROUP/PGC032779_GROUP-largegalaxy-model-r.fits.fz Reading /global/cscratch1/sd/ioannis/SGA-data-dr9alpha/163/PGC032779_GROUP/PGC032779_GROUP-largegalaxy-invvar-r.fits.fz Reading /global/cscratch1/sd/ioannis/SGA-data-dr9alpha/163/PGC032779_GROUP/PGC032779_GROUP-largegalaxy-image-z.fits.fz Reading /global/cscratch1/sd/ioannis/SGA-data-dr9alpha/163/PGC032779_GROUP/PGC032779_GROUP-largegalaxy-model-z.fits.fz Reading /global/cscratch1/sd/ioannis/SGA-data-dr9alpha/163/PGC032779_GROUP/PGC032779_GROUP-largegalaxy-invvar-z.fits.fz Reading /global/cscratch1/sd/ioannis/SGA-data-dr9alpha/163/PGC032779_GROUP/PGC032779_GROUP-largegalaxy-psf-r.fits.fz Building masked image for central 1/2. Central position has been masked, possibly by a star (or saturated core). Pixels used: 43923 Peak Img[j, k]: 572 531 Mean (j, k): 572.09 529.69 Theta (deg): 3.8 Astro PA (deg): 86.2 Eps: 0.080 Major axis (pix): 145.4 Iteratively unmasking pixels: r=145.36 pixels r=145.36 pixels r=174.43 pixels 572.090175925 571.743 529.691477951 531.261 Building masked image for central 2/2. Pixels used: 8645 Peak Img[j, k]: 320 396 Mean (j, k): 319.50 395.91 Theta (deg): 5.1 Astro PA (deg): 84.9 Eps: 0.358 Major axis (pix): 74.3 319.501202687 319.601 395.91489379 396.022 Starting ellipse-fitting for galaxy 1368544 Fitting g-band took......81.392 sec Fitting r-band took......71.634 sec Fitting z-band took......88.682 sec Time for all images = 241.709 sec Performing elliptical aperture photometry. g CoG modeling succeeded with a chi^2 minimum of 292.91 r CoG modeling succeeded with a chi^2 minimum of 53.90 z CoG modeling succeeded with a chi^2 minimum of 335.84 Time = 0.089 min WARNING: The unit 'mgy / arcsec2' could not be saved in native FITS format and cannot be recovered in reading. If pyyaml is installed, it can roundtrip within astropy by using QTable both to write and read back, though one has to enable the unit before reading. [astropy.io.fits.convenience] Writing /global/cscratch1/sd/ioannis/SGA-data-dr9alpha/163/PGC032779_GROUP/PGC032779_GROUP-largegalaxy-1368544-ellipse.fits Starting ellipse-fitting for galaxy 1059425 Fitting g-band took......11.194 sec Fitting r-band took......10.781 sec Fitting z-band took......10.976 sec Time for all images = 32.951 sec Performing elliptical aperture photometry. g CoG modeling succeeded with a chi^2 minimum of 1850.09 r CoG modeling succeeded with a chi^2 minimum of 2353.02 z CoG modeling succeeded with a chi^2 minimum of 640.00 Time = 0.050 min WARNING: The unit 'mgy / arcsec2' could not be saved in native FITS format and cannot be recovered in reading. If pyyaml is installed, it can roundtrip within astropy by using QTable both to write and read back, though one has to enable the unit before reading. [astropy.io.fits.convenience] Writing /global/cscratch1/sd/ioannis/SGA-data-dr9alpha/163/PGC032779_GROUP/PGC032779_GROUP-largegalaxy-1059425-ellipse.fits Finished galaxy PGC032779_GROUP in 6.012 minutes.