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11 papers · 2 filters
The MOSFIRE Deep Evolution Field (MOSDEF) Survey: Rest-Frame Optical Spectroscopy for ~1500 H-Selected Galaxies at 1.37 < z < 3.8
Mariska Kriek, Alice E. Shapley, Naveen A. Reddy +21
In this paper we present the MOSFIRE Deep Evolution Field (MOSDEF) survey. The MOSDEF survey aims to obtain moderate-resolution (R=3000-3650) rest-frame optical spectra (~3700-7000…
On the importance of using appropriate spectral models to derive physical properties of galaxies at 0.7<z<2.8
Camilla Pacifici, Elisabete da Cunha, Stéphane Charlot +14
Interpreting observations of distant galaxies in terms of constraints on physical parameters - such as stellar mass, star-formation rate (SFR) and dust optical depth - requires spe…
Constraining the Low-Mass Slope of the Star Formation Sequence at 0.5<z<2.5
Katherine E. Whitaker, Marijn Franx, Joel Leja +9
We constrain the slope of the star formation rate () to stellar mass () relation down to ($\log(\mathrm{M_{\…
Geometry of Star-Forming Galaxies from SDSS, 3D-HST and CANDELS
A. van der Wel, Yu-Yen Chang, E. F. Bell +18
We determine the intrinsic, 3-dimensional shape distribution of star-forming galaxies at 0<z<2.5, as inferred from their observed projected axis ratios. In the present-day universe…
Reconciling the observed star-forming sequence with the observed stellar mass function
Joel Leja, Pieter van Dokkum, Marijn Franx +1
We examine the connection between the observed star-forming sequence (SFR ) and the observed evolution of the stellar mass function between . We find…
Resolved Star Formation on Sub-galactic Scales in a Merger at z=1.7
Katherine E. Whitaker, Jane R. Rigby, Gabriel B. Brammer +4
We present a detailed analysis of Hubble Space Telescope (HST), Wide Field Camera 3 (WFC3) G141 grism spectroscopy for seven star-forming regions of the highly magnified lensed sta…
The Nature of Extreme Emission Line Galaxies at z=1-2: Kinematics and Metallicities from Near-Infrared Spectroscopy
Michael V. Maseda, Arjen van der Wel, Hans-Walter Rix +21
We present near-infrared spectroscopy of a sample of 22 Extreme Emission Line Galaxies at redshifts 1.3 < z < 2.3, confirming that these are low-mass (M* = 10^8 - 10^9 M_sun) galax…
A Massive Galaxy in its Core Formation Phase Three Billion Years After the Big Bang
Erica Nelson, Pieter van Dokkum, Marijn Franx +13
Most massive galaxies are thought to have formed their dense stellar cores at early cosmic epochs. However, cores in their formation phase have not yet been observed. Previous stud…
Dense cores in galaxies out to z=2.5 in SDSS, UltraVISTA, and the five 3D-HST/CANDELS fields
Pieter van Dokkum, Rachel Bezanson, Arjen van der Wel +15
The dense interiors of massive galaxies are among the most intriguing environments in the Universe. In this paper we ask when these dense cores were formed and determine how galaxi…
3D-HST WFC3-selected Photometric Catalogs in the Five CANDELS/3D-HST Fields: Photometry, Photometric Redshifts and Stellar Masses
Rosalind E. Skelton, Katherine E. Whitaker, Ivelina G. Momcheva +24
The 3D-HST and CANDELS programs have provided WFC3 and ACS spectroscopy and photometry over ~900 square arcminutes in five fields: AEGIS, COSMOS, GOODS-North, GOODS-South, and the…
Bulge Growth and Quenching since z = 2.5 in CANDELS/3D-HST
Philipp Lang, Stijn Wuyts, Rachel S. Somerville +20
Exploiting the deep high-resolution imaging of all 5 CANDELS fields, and accurate redshift information provided by 3D-HST, we investigate the relation between structure and stellar…