activity
20092024
most citedGeometry of Star-Forming Galaxies from SDSS, 3D-HST and CANDELS

180 citations · 802 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.EP2024★ 13 cited

TESS Giants Transiting Giants. VI. Newly Discovered Hot Jupiters Provide Evidence for Efficient Obliquity Damping after the Main Sequence

Nicholas Saunders, Samuel K. Grunblatt, Ashley Chontos +53

The degree of alignment between a star's spin axis and the orbital plane of its planets (the stellar obliquity) is related to interesting and poorly understood processes that occur…

astro-ph.EP2018★ 142 cited

A candidate super-Earth planet orbiting near the snow line of Barnard's star

I. Ribas, M. Tuomi, A. Reiners +60

At a distance of 1.8 parsecs, Barnard's star (Gl 699) is a red dwarf with the largest apparent motion of any known stellar object. It is the closest single star to the Sun, second…

astro-ph.GA2016★ 179 cited

The evolution of star formation histories of quiescent galaxies

Camilla Pacifici, Susan A. Kassin, Benjamin J. Weiner +22

Although there has been much progress in understanding how galaxies evolve, we still do not understand how and when they stop forming stars and become quiescent. We address this by…

astro-ph.GA2015★ 98 cited

Ultradeep IRAC Imaging Over The HUDF And GOODS-South: Survey Design And Imaging Data Release

I. Labbe, P. A. Oesch, G. D. Illingworth +11

The IRAC ultradeep field (IUDF) and IRAC Legacy over GOODS (IGOODS) programs are two ultradeep imaging surveys at 3.6μm and 4.5μm with the Spitzer Infrared Array Camera (IRAC). The…

astro-ph.GA2014★ 180 cited

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…

astro-ph.GA2014★ 39 cited

Rest-Frame Optical Emission Lines in z~3.5 Lyman Break selected Galaxies: The Ubiquity of Unusually High [OIII]/Hbeta Ratios at 2 Gyr

B. P. Holden, P. A. Oesch, V. G. Gonzalez +6

We present K-band spectra of rest-frame optical emission lines for 24 star-forming galaxies at z~3.2-3.7 using MOSFIRE on the Keck 1 telescope. Strong rest-frame optical [O III] an…

astro-ph.CO2011★ 86 cited

The SWELLS survey. II. Breaking the disk-halo degeneracy in the spiral galaxy gravitational lens SDSS J2141-0001

A. A. Dutton, B. J. Brewer, P. J. Marshall +6

The degeneracy among the disk, bulge and halo contributions to galaxy rotation curves prevents an understanding of the distribution of baryons and dark matter in disk galaxies. In…

astro-ph.CO2009★ 65 cited

A Spectroscopically Confirmed Excess of 24 micron Sources in a Super Galaxy Group at z=0.37: Enhanced Dusty Star Formation Relative to the Cluster and Field Environment

Kim-Vy H. Tran, Amelie Saintonge, John Moustakas +5

To trace how dust-obscured star formation varies with environment, we compare the fraction of 24 micron sources in a super galaxy group to the field and a rich galaxy cluster at z~…