output
20022020
most citedThe Transiting Exoplanet Survey Satellite

4.1k citations

Showing 2012Show all

11 papers · 1 filter

astro-ph.CO2012134 cited

The Carnegie-Irvine Galaxy Survey. III. The Three-Component Structure of Nearby Elliptical Galaxies

Song Huang, Luis C. Ho, Chien Y. Peng +2

Motivated by recent developments in our understanding of the formation and evolution of massive galaxies, we explore the detailed photometric structure of a representative sample o…

astro-ph.CO201228 cited

Intragroup and Galaxy-Linked Diffuse X-ray Emission in Hickson Compact Groups

Tyler D. Desjardins, Sarah C. Gallagher, Panayiotis Tzanavaris +9

Isolated compact groups of galaxies (CGs) present a range of dynamical states, group velocity dispersions, and galaxy morphologies with which to study galaxy evolution, particularl…

astro-ph.IM201219 cited

Exploring the NRO Opportunity for a Hubble-sized Wide-field Near-IR Space Telescope -- NEW WFIRST

Alan Dressler, David Spergel, Matt Mountain +24

We discuss scientific, technical and programmatic issues related to the use of an NRO 2.4m telescope for the WFIRST initiative of the 2010 Decadal Survey. We show that this impleme…

cond-mat.supr-con201218 cited

High-pressure effects on single crystals electron-doped rCeCuO

C. R. Rotundu, V. V. Struzhkin, M. S. Somayazulu +3

We present high pressure diamond anvil cell synchrotron X-ray, resistivity, and ac-susceptibility measurements on electron-doped cuprate PrCeCuO to much higher…

astro-ph.SR2012120 cited

Observable Signatures of Planet Accretion in Red Giant Stars I: Rapid Rotation and Light Element Replenishment

Joleen K. Carlberg, Katia Cunha, Verne V. Smith +1

The orbital angular momentum of a close-orbiting giant planet can be sufficiently large that, if transferred to the envelope of the host star during the red giant branch (RGB) evol…

astro-ph.CO201269 cited

A unified picture of breaks and truncations in spiral galaxies from SDSS and S^{4}G imaging

Ignacio Martín-Navarro, Judit Bakos, Ignacio Trujillo +21

The mechanism causing breaks in the radial surface brightness distribution of spiral galaxies is not yet well known. Despite theoretical efforts, there is not a unique explanation…