[PDF] Top 20 Observing strategy for the SDSS IV/MaNGA IFU galaxy survey

... the MaNGA fi bers have an inner light-sensitive core diameter ( ID ) of 120 μ m ( corresponding to ...for MaNGA, as illustrated in Figure ...total IFU footprint by chemically stripping the protective ... See full document

... Section 6 describes our spatial binning approach and the importance of including spatial covariance in these calculations. Section 7 goes into particular depth with regard to the assessments of the stellar kinematics. We ... See full document

... Since MaNGA is an imaging spectroscopic survey, image quality is important and the 56% fi ll factor of circular fi ber apertures within the hexagonal MaNGA IFU footprint ( Law et ... See full document

... IFS survey is the SDSS- IV / MaNGA galaxy survey operating at the ...the SDSS telescope and sizable detector real estate, MaNGA uses multiple fi ber bundles to ... See full document

... The MaNGA survey (Bundy et ...the SDSS and aims to obtain spatially resolved spectroscopy of nearly 10 000 galaxies (median redshift z ∼ ...2020. MaNGA uses the five different types of ... See full document

... The MaNGA survey (Bundy et ...Sky Survey (SDSS) and aims to obtain spatially resolved spectroscopy of 10,000 nearly galaxies (median redshift z ∼ ...2020. MaNGA uses 5 different types ... See full document

... MaNGA will ultimately obtain integral- fi eld spectroscopy of 10,000 nearby galaxies with the 2.5 m Sloan Foundation Telescope ( Gunn et al. 2006 ) and the BOSS spectrographs ( Smee et al. 2013 ) . Fibers are ... See full document

... produce galaxy wide post-starburst ...the galaxy-wide MaNGA survey allows us to address these ques- tions from a new angle, compared to the single fibre surveys carried out in the ...uniform ... See full document

... of observing more than one galaxy ...spectrograph survey (SAMI; see Croom et ...the survey) utilises 13 IFUs identical in size and shape (hexabundles containing 61 fi- bres each) with the aim ... See full document

... local galaxy population are providing the next step forward in these ...studies. IFU spectroscopy, pioneered by the SAURON and ATLAS-3D projects (Bacon et ...and MaNGA (Bundy et al. 2015) are ... See full document

... this IFU at a specific orientation so that each star landed on portions of the IFU corresponding to a different V-groove slit ...the IFU. Third, the same galaxy was observed with both the ... See full document

... strong galaxy-galaxy gravitational lens candidates identified in the Sloan Digital Sky Survey IV ...(SILO) survey extends the methodology of the Sloan Lens ACS Survey (SLACS) and ... See full document

... P- MaNGA bundle ma003 was a particularly important test ...this IFU at a specific orientation so that each star landed on por- tions of the IFU corresponding to a different V-groove slit ...the ... See full document

... Future observations that can directly resolve gas dis- tributions in large and diverse samples of galaxies out to large radii will be highly valuable to further test the fragmentation-driven star formation scenario. Wide ... See full document

... DiskMass survey (Bershady et al. 2010) used two fiber-fed Integral Field Unit (IFU), SparsePak on WIYN and PPak on the Calar Alto ...this survey utilized high spectral resolu- tion in three narrow ... See full document

... this galaxy is also likely to be an S0 galaxy, but the stellar populations show a very different ...this galaxy un- derwent the transformation into an S0 longer ago than 7443-12701, however the small ... See full document

... key galaxy evolutionary processes. A serendipitous observation by the MaNGA survey has revealed a large, asymmetric H α complex with no optical counterpart that extends ≈ 8 ″ (≈ ...host galaxy ... See full document

... In order to control for the degeneracies between mass, metallicity and dust (all of which can redden a galaxy’s op- tical colour and mimic the effects of quenching) we selected a sub-sample of fast rotators from those ... See full document

... bimodal galaxy population, includ- ing colour, SFR and passive fraction are found to depend both on stellar mass and environment (Blanton et ...legacy SDSS, it has been demonstrated that the change in EW(H ... See full document

... solely galaxy mergers as the source for misaligned cold gas only predicts 2% of ETGs to have ∆PA > 30 ◦ ...incident galaxy mergers in their GALFORM ... See full document