[PDF] Top 20 Measuring Photometric Properties Of Sdss And Manga Galaxies

... 5.1 Top left and right: Cutouts of the galaxy image, zoomed in on the right to highlight the area covered by MaNGA IFUs (shown as a white hexagon). The color scale is representative of the surface brightness ... See full document

... that MaNGA galaxies are observed using the BOSS Spectrograph (Gunn et ...the MaNGA Data Reduction Pipeline (DRP; Law et ...and SDSS- I/II spec2d reductions allows a very similar foreground ... See full document

... calculated using the ONS calibration (Pilyugin, V´ılchez & Thuan 2010). The red dashed line represents the N/O expected when nitrogen is only a primary nucleosynthetic product, while the blue dashed line represents a ... See full document

... meters are obtained from the SDSS 3 0 fi ber spectra, so they combine to probe the recent SFH of the central 1 – 2 kpc of the MaNGA galaxies. We take the measurements of these parameters from the MPA ... See full document

... all galaxies at lower mass show some net ...high-mass galaxies that have signi fi cant rotation do not stand out in other galaxy properties, except for a higher incidence of ionized gas ...central ... See full document

... of galaxies but also revealed how the star formation rates (SFRs), metallicities, stellar populations, morphologies, and black hole growth rates of galaxies vary with mass, environment, and ...hundred ... See full document

... (SDSS) galaxies at i < 21 using clustering redshifts, from which we also compute targeting completeness measurements for the Baryon Oscillation Spec- troscopic Survey ...of galaxies with only ... See full document

... for galaxies in the clean sample classified by spirals and fast/slow ETGs where the symbols are as in Figure ...The galaxies are enclosed between two regimes defined by Equation 4 (red) and Figure 9 (dashed ... See full document

... gas properties, redshift, and environment, these measurements constrain the physics governing star for- mation and assembly over cosmic time, and would reveal potential IMF variations, which are assumed to be con- ... See full document

... Nearby Galaxies at APO (MaNGA), and the Extended Baryon Oscillation Spectroscopic Survey ...from SDSS-IV, Data Release 13 ...nearby galaxies from ...the SDSS-III BOSS data, improving ... See full document

... and MaNGA (Bundy et ...population properties in the multivariate space of galaxy parameters to be ...population properties with central velocity dispersion (Sánchez-Blázquez et ...300 galaxies ... See full document

... the MaNGA Data Analysis Pipeline (DAP) version ...of galaxies, and preferentially masks spaxels classified as star ...small galaxies with areas similar to the PSF area, and the effect of correlated ... See full document

... mean properties between bins can be detected at the 5 sigma level even when the measurement pre- cision for individual galaxies is comparable to this ... See full document

... (red) galaxies, as a function of local ...central galaxies (see also Table ...massive galaxies as part of the MASSIVE survey, where it is found that even at large radius, internal properties ... See full document

... excitation properties of the ionized gas in a sample of 646 galaxies using integral field spectroscopy data from the Sloan Digital Sky Survey IV Mapping Nearby Galaxies at Apache Point Observatory ... See full document

... valley galaxies faced two main ...transitional galaxies largely rely on the single- fi ber SDSS spectroscopy, which lacks spatial information and covers only the central part of nearby ...of ... See full document

... of galaxies can serve as a probe of their assembly ...early-type galaxies are dynamically hot systems, many of them show some rotation ( ...of galaxies is in fl uenced in complex ways by mergers ( ... See full document

... various properties such as large-scale environmental density and halo age using semi-analytical galaxy models applied to the Millennium simulation (Springel et ...satellite galaxies to merge with the ... See full document

... Nearby Galaxies at Apache Point Observatory ( MaNGA ) is an integral- fi eld spectroscopic survey that is one of three core programs in the fourth-generation Sloan Digital Sky Survey ( SDSS-IV ) .... ... See full document

... the SDSS and SDSS-II has been provided by the Alfred ...The SDSS website is http://www.sdss.org/. The SDSS is managed by the Astrophysical Research Con- sortium for the Participating ... See full document