Search Publications

Breaking the Curve with CANDELS: A Bayesian Approach to Reveal the Non-Universality of the Dust-Attenuation Law at High Redshift
DOI: 10.3847/0004-637X/827/1/20 Bibcode: 2016ApJ...827...20S

Papovich, Casey; Finkelstein, Steven L.; Pérez-González, Pablo G. +13 more

Dust attenuation affects nearly all observational aspects of galaxy evolution, yet very little is known about the form of the dust-attenuation law in the distant universe. Here, we model the spectral energy distributions of galaxies at z ∼ 1.5-3 from CANDELS with rest-frame UV to near-IR imaging under different assumptions about the dust law, and …

2016 The Astrophysical Journal
eHST 122
The Dragonfly Nearby Galaxies Survey. II. Ultra-Diffuse Galaxies near the Elliptical Galaxy NGC 5485
DOI: 10.3847/1538-4357/833/2/168 Bibcode: 2016ApJ...833..168M

van Dokkum, Pieter; Abraham, Roberto; Danieli, Shany +4 more

We present the unexpected discovery of four ultra-diffuse galaxies (UDGs) in a group environment. We recently identified seven extremely low surface brightness galaxies in the vicinity of the spiral galaxy M101, using data from the Dragonfly Telephoto Array. The galaxies have effective radii of 10″-38″ and central surface brightnesses of 25.6-27.7…

2016 The Astrophysical Journal
eHST 121
Evolution of Stellar-to-Halo Mass Ratio at z = 0 - 7 Identified by Clustering Analysis with the Hubble Legacy Imaging and Early Subaru/Hyper Suprime-Cam Survey Data
DOI: 10.3847/0004-637X/821/2/123 Bibcode: 2016ApJ...821..123H

Ono, Yoshiaki; Ouchi, Masami; Harikane, Yuichi +15 more

We present clustering analysis results from 10,381 Lyman break galaxies (LBGs) at z ∼ 4-7, identified in the Hubble legacy deep imaging and new complimentary large-area Subaru/Hyper Suprime-Cam data. We measure the angular correlation functions of these LBGs at z ∼ 4, 5, 6, and 7 and fit these measurements using halo occupation distribution (HOD) …

2016 The Astrophysical Journal
eHST 120
Resolving the Discrepancy of Galaxy Merger Fraction Measurements at z ∼ 0-3
DOI: 10.3847/0004-637X/830/2/89 Bibcode: 2016ApJ...830...89M

Zirm, Andrew W.; Toft, Sune; Man, Allison W. S.

We measure the merger fraction of massive galaxies using the UltraVISTA/COSMOS catalog, complemented with the deeper, higher resolution 3DHST+CANDELS catalog, presenting the largest mass-complete photometric merger sample up to z∼ 3. We find that the variation in the mass ratio probe can explain the discrepant redshift evolution of the merger frac…

2016 The Astrophysical Journal
eHST 120
The Connection Between Reddening, Gas Covering Fraction, and the Escape of Ionizing Radiation at High Redshift
DOI: 10.3847/0004-637X/828/2/108 Bibcode: 2016ApJ...828..108R

Pettini, Max; Shapley, Alice E.; Steidel, Charles C. +2 more

Using a large sample of spectroscopically confirmed z∼ 3 galaxies, we establish an empirical relationship between reddening (E(B-V)), neutral gas covering fraction ({f}{{cov}}({{H}} {{I}})), and the escape of ionizing (Lyman continuum, LyC) photons. Our sample includes 933 galaxies at z∼ 3,121 of which have deep spectroscopic observatio…

2016 The Astrophysical Journal
eHST 119
A New Population of Compton-thick AGNs Identified Using the Spectral Curvature above 10 keV
DOI: 10.3847/0004-637X/825/2/85 Bibcode: 2016ApJ...825...85K

Harrison, F. A.; Stern, D.; Alexander, D. M. +19 more

We present a new metric that uses the spectral curvature (SC) above 10 keV to identify Compton-thick active galactic nuclei (AGNs) in low-quality Swift/Burst Alert Telescope (BAT) X-ray data. Using NuSTAR, we observe nine high SC-selected AGNs. We find that high-sensitivity spectra show that the majority are Compton-thick (78% or 7/9) and the rema…

2016 The Astrophysical Journal
XMM-Newton 118
Globular Clusters Indicate That Ultra-diffuse Galaxies Are Dwarfs
DOI: 10.3847/0004-637X/830/1/23 Bibcode: 2016ApJ...830...23B

Beasley, Michael A.; Trujillo, Ignacio

We present an analysis of archival HST/ACS imaging in the F475W (g 475), F606W (V 606), and F814W (I 814) bands of the globular cluster (GC) system of a large (3.4 kpc effective radius) ultra-diffuse galaxy (DF17) believed to be located in the Coma Cluster of galaxies. We detect 11 GCs down to the 5σ completeness l…

2016 The Astrophysical Journal
eHST 118
A Universal Density Structure for Circumgalactic Gas
DOI: 10.3847/0004-637X/830/2/87 Bibcode: 2016ApJ...830...87S

Stern, Jonathan; Hennawi, Joseph F.; Prochaska, J. Xavier +1 more

We develop a new method to constrain the physical conditions in the cool (∼104 K) circumgalactic medium (CGM) from measurements of ionic column densities by assuming that the cool CGM spans a large range of gas densities and that small high-density clouds are hierarchically embedded in large low-density clouds. The new method combines t…

2016 The Astrophysical Journal
eHST 118
Balloon-Borne Submillimeter Polarimetry of the Vela C Molecular Cloud: Systematic Dependence of Polarization Fraction on Column Density and Local Polarization-Angle Dispersion
DOI: 10.3847/0004-637X/824/2/134 Bibcode: 2016ApJ...824..134F

Ward-Thompson, Derek; Fissel, Laura M.; Nakamura, Fumitaka +27 more

We present results for Vela C obtained during the 2012 flight of the Balloon-borne Large Aperture Submillimeter Telescope for Polarimetry. We mapped polarized intensity across almost the entire extent of this giant molecular cloud, in bands centered at 250, 350, and 500 µm. In this initial paper, we show our 500 µm data smoothed to a r…

2016 The Astrophysical Journal
Herschel 116
Highest Redshift Image of Neutral Hydrogen in Emission: A CHILES Detection of a Starbursting Galaxy at z = 0.376
DOI: 10.3847/2041-8205/824/1/L1 Bibcode: 2016ApJ...824L...1F

Strader, Jay; Scoville, Nick; Yun, Min S. +32 more

Our current understanding of galaxy evolution still has many uncertainties associated with the details of the accretion, processing, and removal of gas across cosmic time. The next generation of radio telescopes will image the neutral hydrogen (H I) in galaxies over large volumes at high redshifts, which will provide key insights into these proces…

2016 The Astrophysical Journal
eHST 114