Results 101 to 110 of about 14,388 (158)
Reverberation mapping of active galactic nuclei: from X-ray corona to dusty torus. [PDF]
Cackett EM, Bentz MC, Kara E.
europepmc +1 more source
The connection between galaxies and dark matter halos is often quantified using the stellar mass–halo mass (SMHM) relation. Optical and near-infrared imaging surveys have led to a broadly consistent picture of the evolving SMHM relation based on ...
Andrew B. Newman +8 more
doaj +1 more source
Transformative science from the lunar farside: observations of the dark ages and exoplanetary systems at low radio frequencies. [PDF]
Burns JO.
europepmc +1 more source
One of the current challenges in galaxy evolution studies is to establish the mechanisms that govern the escape of ionizing radiation from galaxies.
A. Saldana-Lopez +26 more
doaj +1 more source
The MOSDEF-KCWI Survey: Spectral Properties of Lyα Halos around z ∼ 2 Star-forming Galaxies
We present Keck Cosmic Web Imager integral field observations of extended Ly α emission in the circumgalactic medium of 27 typical star-forming galaxies at z ∼ 2, drawn from the Multi-Object Spectrometer for Infra-Red Exploration (MOSFIRE) Deep Evolution
Andrew Weldon +3 more
doaj +1 more source
High-redshift star formation in the Atacama large millimetre/submillimetre array era. [PDF]
Hodge JA, da Cunha E.
europepmc +1 more source
Observational Signatures of Lyman Alpha Emission from Early Galaxy Formation
The next generation of telescopes aim to directly observe the first generation of galaxies that initiated the reionization process in our Universe. The Lyman Alpha (Lya) emission line is robustly predicted to be the most prominent intrinsic spectral ...
Dijkstra, Mark
core
We report the identification of a quasar overdensity in the BOSSJ0210 field, dubbed the Cosmic Himalayas, consisting of 11 quasars at z = 2.16−2.20, the densest overdensity of quasars (17 σ ) in the ∼10,000 deg ^2 of the Sloan Digital Sky Survey (SDSS ...
Yongming Liang +29 more
doaj +1 more source
MUSEQuBES: Connecting H i Absorption with Lyα Emitters at z ≈ 3.3
We present a comprehensive analysis of H i absorption around 96 Ly α emitters (LAEs) at z ≈ 3.3 (median Ly α luminosity ≈10 ^42 erg s ^−1 ). These LAEs were identified within eight MUSE fields, each $1^{\prime} \times 1^{\prime} $ on the sky and ...
Eshita Banerjee +8 more
doaj +1 more source
In this work, we test the frequent assumption that Ly α -emitting galaxies (LAEs) are experiencing their first major burst of star formation at the time of observation.
Nicole M. Firestone +29 more
doaj +1 more source

