output
20062026
most citedPhosphorene nanoribbons, nanotubes and van der Waals multilayers

619 citations

Showing 2015 · astro-ph.GAShow all

6 papers · 2 filters

astro-ph.GA2015★ 2 cited

Keck/ESI Long-slit Spectroscopy of SBS 1421+511: A Recoiling Quasar Nucleus in An Active Galaxy Pair?

Luming Sun, Hongyan Zhou, Lei Hao +6

We present Keck/ESI long-slit spectroscopy of SBS 1421+511, a system consisting of a quasar at z = 0.276 and an extended source 3" northern to the quasar. The quasar shows a blue-s…

astro-ph.GA2015★ 99 cited

Infrared color selection of massive galaxies at z > 3

T. Wang, D. Elbaz, C. Schreiber +29

We introduce a new color-selection technique to identify high-redshift, massive galaxies that are systematically missed by Lyman-break selection. The new selection is based on the…

astro-ph.GA2015★ 17 cited

Identification of z~>2 Herschel 500 micron sources using color-deconfusion

X. W. Shu, D. Elbaz, N. Bourne +19

We present a new method to search for candidate z~>2 Herschel 500μm sources in the GOODS-North field, using a S500μm/S24μm "color deconfusion" technique. Potential high-z sources a…

astro-ph.GA2015★ 28 cited

Discovery of Extremely Broad Balmer Absorption Lines in SDSS J152350.42+391405.2

Shaohua Zhang, Hongyan Zhou, Xiheng Shi +7

We present the discovery of Balmer line absorption from H to H in an iron low-ionization broad absorption line (FeLoBAL) quasar SDSS J152350.42+391405.2 (hereafter J1523), by…

astro-ph.GA2015★ 43 cited

Young Galaxy Candidates in the Hubble Frontier Fields. II. MACS,J0416-2403

Leopoldo Infante, Wei Zheng, Nicolas Laporte +14

We searched for z > 7 Lyman-break galaxies (LBGs) in the optical-to-mid-infrared Hubble Frontier Field and associated parallel field observations of the strong-lensing cluster MACS…

astro-ph.GA2015★ 43 cited

A Comprehensive Study of Broad Absorption Line Quasars: I. Prevalence of HeI* Absorption Line Multiplets in Low-Ionization Objects

Wen-Juan Liu, Hongyan Zhou, Tuo Ji +13

Neutral Helium multiplets, HeI*3189,3889,10830 are very useful diagnostics to the geometry and physical conditions of the absorbing gas in quasars. So far only a handful of HeI* de…