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

... First, any systematic error in the emission-line model will propagate to biases in the spectral indices mea- sured with passbands that span emission-line regions because the emission-line model is subtracted from the ... See full document

... expected MaNGA data quality, and thereby constrain the hardware design and observing strategy for the ...an overview of the SDSS ...the MaNGA legacy hardware and IFU ferrule ... See full document

... science-ready data products are produced by the Data Reduction Pipeline (DRP; Law et ...for MaNGA observations. To al- low the user to quickly access the data that is relevant to their ... 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

... 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

... 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

... in MaNGA survey data will provide unique access to gravity-sensitive features (Conroy & van Dokkum 2012b) that constrain the faint end of the IMF ...the galaxy, as well as the shape and ... See full document

... plate, galaxy targets were centered in the focal plane to maximize throughput for 5400 ˚ A ...current data reduction pipeline, the routines developed in Margala et ... 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

... by SDSS, for instance, cannot cover most of the light in nearby ...the SDSS 3 00 fibers with the total flux of all main sample galaxies in SDSS, 80% of galaxies have less than 36% of their light ... 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

... 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

... 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

... ( 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

... DiskMass survey ( Bershady et ...this survey utilized high spectral resolution in three narrow wavelength windows around 515, 660, and 860 ...) survey used a fi ber- fed integral fi eld spectrograph, ... 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

... the analysis of a small sample observed with the MaNGA prototype instrument in Bel fi ore et ...a galaxy class that arguably should be renamed from LINER ( Low Ionization Nuclear Emission Region ) ... See full document

... an analysis during commissioning revealed the OH skyline residuals were signi fi cantly worse in R1 than in the R2 ...of SDSS-IV, but which nonetheless affected the commissioning plates 7443 and ... See full document

... the MaNGA primary and secondary samples are selected to be volume limited within a prescribed redshift ...Seventeen galaxy IFUs (ranging from 19-fibre IFU, 12 arcsec on sky diameter, to 127-fibre ... See full document