[PDF] Top 20 The data reduction pipeline for the SDSS IV MaNGA IFU Galaxy Survey

... We examine this behavior as a function of wavelength in Figure 11 ( left-hand panel ) by plotting the 1 σ width of the Gaussian that best fi ts the distribution of un fl agged pixel values at a given wavelength across all ... See full document

... the galaxy environment, whether measured as local environmental density or through central/satellite classification, does not appear to have any significant effect on age and metallicity gradients in ...recent ... See full document

... the MaNGA prototype instrument in Bel fi ore et ...a galaxy class that arguably should be renamed from LINER ( Low Ionization Nuclear Emission Region ) galaxies to LIER ...the galaxy population as a ... See full document

... overlap MaNGA and other IFU surveys will be particularly ...complete data for large sam- ples will also enable exploration into whether the behavior of Q thermal , τ, and Q thermal τ are universal ... See full document

... Sky Survey (SDSS-IV) began observations in July ...Spectroscopic Survey (TDSS) and the SPectroscopic IDentification of ERosita Sources ...first data release from SDSS-IV, ... See full document

... section) are calculated on the Voronoi binned (VOR10) maps which are binned to achieve a target SNR of 10 in the r-band continuum. Further details of the Voronoi binning, stellar continuum and emis- sion line fitting ... 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

... the MaNGA 7 fibre ...fibre IFU mini-bundles results in a ∼ 1% photo- metric uncertainty (Yan et ...the IFU bundle metrology (location of fibre, dithering and atmospheric chromatic differential ... See full document

... science-ready data products are produced by the Data Reduction Pipeline (DRP; Law et ...the reduction, calibra- tion and sky-subtraction for MaNGA ...the data that is ... 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

... of galaxy evolution. MaNGA has the unique potential to break the degener- acy between mass and light by combining state-of-the-art dynamical modeling ...in MaNGA survey data will ... See full document

... ( MaNGA ) survey, one of three core programs of the fourth-generation Sloan Digital Sky Survey ( SDSS-IV ) , is producing a massive, high-dimensional integral fi eld spectroscopic ... 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

... the MaNGA data analysis pipeline (DAP version ...the galaxy in order to cleanly subtract the absorption lines from the ...a galaxy and the ellipticity within it, e ... See full document

... Flagging of the DAP output stellar kinematics is some- what minimal in DR15 with three basic flags applied (see Tables 8 and 9): (1) If a spectrum (binned or oth- erwise) does not meet either the binning or minimum S/N ... See full document

... To dither, we simply modify the location of the expected guide star position. Rather than requiring all the stars to be located at the center of the guider fi ber bundle, we require them to be located 0 83 from the center ... 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

... ( 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 ) .... MaNGA ’ s 17 pluggable ... 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