output
19932026
most citedObservational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant

19.6k citations

Showing 2014 · astro-ph.GAShow all

192 papers · 2 filters

astro-ph.GA2014★ 20 cited

A Newly Recognized Very Young Supernova Remnant in M83

William P. Blair, P. Frank Winkler, Knox S. Long +7

As part of a spectroscopic survey of supernova remnant candidates in M83 using the Gemini-South telescope and GMOS, we have discovered one object whose spectrum shows very broad li…

astro-ph.GA2014★ 13 cited

CLASH: Extreme Emission Line Galaxies and Their Implication on Selection of High-Redshift Galaxies

Xingxing Huang, Wei Zheng, Junxian Wang +23

We utilize the CLASH (Cluster Lensing And Supernova survey with Hubble) observations of 25 clusters to search for extreme emission-line galaxies (EELGs). The selections are carried…

astro-ph.GA2014★ 12 cited

Star Formation in High-Redshift Cluster Ellipticals

Cory R. Wagner, Mark Brodwin, Gregory F. Snyder +11

We measure the star formation rates (SFRs) of massive () early-type galaxies (ETGs) in a sample of 11 high-redshift () galaxy clusters…

astro-ph.GA2014★ 119 cited

A Critical Look at the Mass-Metallicity-SFR Relation in the Local Universe. I. An Improved Analysis Framework and Confounding Systematics

Samir Salim, Janice C. Lee, Chun Ly +5

It has been proposed that the mass-metallicity relation of galaxies exhibits a secondary dependence on star formation rate (SFR), and that the resulting M-Z-SFR relation may be red…

astro-ph.GA2014★ 114 cited

Probing the Fermi Bubbles in Ultraviolet Absorption: A Spectroscopic Signature of the Milky Way's Biconical Nuclear Outflow

Andrew J. Fox, Rongmon Bordoloi, Blair D. Savage +9

Giant lobes of plasma extend 55 degrees above and below the Galactic Center, glowing in emission from gamma rays (the Fermi Bubbles) to microwaves (the WMAP haze) and polarized rad…

astro-ph.GA2014★ 149 cited

ZFOURGE/CANDELS: On the Evolution of M* Galaxy Progenitors from z=3 to 0.5

Casey Papovich, I. Labbé, R. Quadri +38

Galaxies with stellar masses near M* contain the majority of stellar mass in the universe, and are therefore of special interest in the study of galaxy evolution. The Milky Way (MW…