English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Tools annual

Global: Zendy Free Plan

Global: Zendy Tools monthly

Global: Zendy Plus monthly

In this paper we present the MOSFIRE Deep Evolution Field (MOSDEF) survey.The MOSDEF survey aims to obtain moderate-resolution (R=3000-3650) rest-frameoptical spectra (~3700-7000 Angstrom) for ~1500 galaxies at 1.37<z<3.80 inthree well-studied CANDELS fields: AEGIS, COSMOS, and GOODS-N. Targets areselected in three redshift intervals: 1.37<z<1.70, 2.09<z<2.61, and2.95<z<3.80, down to fixed H_AB (F160W) magnitudes of 24.0, 24.5 and 25.0,respectively, using the photometric and spectroscopic catalogs from the 3D-HSTsurvey. We target both strong nebular emission lines (e.g., [OII], Hbeta,[OIII], 5008, Halpha, [NII], and [SII]) and stellar continuum and absorptionfeatures (e.g., Balmer lines, Ca-II H and K, Mgb, 4000 Angstrom break). Here wepresent an overview of our survey, the observational strategy, the datareduction and analysis, and the sample characteristics based on spectraobtained during the first 24 nights. To date, we have completed 21 masks,obtaining spectra for 591 galaxies. For ~80% of the targets we derive a robustredshift from either emission or absorption lines. In addition, we confirm 55additional galaxies, which were serendipitously detected. The MOSDEF galaxysample includes unobscured star-forming, dusty star-forming, and quiescentgalaxies and spans a wide range in stellar mass (~10^9-10^11.5 Msol) and starformation rate (~10^0-10^3 Msol/yr). The spectroscopically confirmed sample isroughly representative of an H-band limited galaxy sample at these redshifts.With its large sample size, broad diversity in galaxy properties, and wealth ofavailable ancillary data, MOSDEF will transform our understanding of thestellar, gaseous, metal, dust, and black hole content of galaxies during thetime when the universe was most active.

The MOSFIRE Deep Evolution Field (MOSDEF) Survey: Rest-Frame Optical Spectroscopy for ~1500 H-Selected Galaxies at 1.37 < z < 3.8