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Related papers: Physics of Prodigious Lyman Continuum Leakers

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FUSE spectra of star-forming regions in nearby galaxies are compared to composite spectra of Lyman-break galaxies (LBGs), binned by strength of Lyman alpha emission and by mid-UV luminosity. Several far-UV spectral features, including lines…

Astrophysics · Physics 2008-11-26 William C. Keel

Finding and elucidating the properties of Lyman-continuum(LyC)-emitting galaxies is an important step for our understanding of cosmic reionization. Although the z - 0.3-0.4 LyC emitters found recently show strong optical emission lines, no…

Astrophysics of Galaxies · Physics 2020-11-25 L. Ramambason , D. Schaerer , G. Stasińska , Y. I. Izotov , N. G. Guseva , J. M Vílchez , R. Amorín , C. Morisset

At cosmic dawn, the 21-centimeter signal from intergalactic hydrogen was driven by Lyman-$\alpha$ photons from some of the earliest stars, producing a spatial pattern that reflected the distribution of galaxies at that time. Due to the…

Cosmology and Nongalactic Astrophysics · Physics 2023-11-28 Itamar Reis , Rennan Barkana , Anastasia Fialkov

The first galaxies that formed at a redshift ~20-30 emitted continuum photons with energies between the Lyman-alpha and Lyman limit wavelengths of hydrogen, to which the neutral universe was transparent except at the Lyman-series…

Astrophysics · Physics 2008-11-26 Rennan Barkana , Abraham Loeb

Ly{\alpha} emission, Ly{\alpha} absorption and MgII absorption are powerful tracers of neutral hydrogen. Hydrogen is the most abundant element in the universe and plays a central role in galaxy formation via gas accretion and outflows, as…

Astrophysics of Galaxies · Physics 2015-06-22 Luke A. Barnes , Thibault Garel , Glenn G. Kacprzak

We report the first space-based very deep near-infrared continuum observations of a uniform sample of z = 6.5 galaxies with log(L(L_alpha)) = 42.5 - 43 erg/s selected from narrow-band line searches and with spectroscopically confirmed Ly…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-28 Lennox L. Cowie , Esther M. Hu , Antoinette Songaila

We use state-of-the-art simulations to explore the physical evolution of galaxies in the first billion years of cosmic time. First, we demonstrate that our model reproduces the basic statistical properties of the observed Lyman-break galaxy…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-12 Pratika Dayal , James S. Dunlop , Umberto Maio , Benedetta Ciardi

We constrain the X-ray emission properties of Lyman break galaxies (LBGs) at z ~ 3-6 using the 2 Ms Chandra Deep Field-North and 1 Ms Chandra Deep Field-South. Large samples of LBGs were discovered using HST as part of the Great…

We study the properties of Ly-alpha emitters in a cosmological framework by computing the escape of Ly-alpha photons through galactic outflows. We combine the GALFORM semi-analytical model of galaxy formation with a Monte Carlo Ly-alpha…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-30 Alvaro Orsi , Cedric G. Lacey , Carlton M. Baugh

This paper is the second in a series aimed at examining the gaseous environments of z$\le$0.3 quasars and ultraluminous infrared galaxies (ULIRGs) as a function of AGN/host galaxy properties across the merger sequence. This second paper…

Astrophysics of Galaxies · Physics 2022-08-17 Weizhe Liu , Sylvain Veilleux , David S. N. Rupke , Todd M. Tripp , Frederick Hamann , Crystal Martin

We study the global dust and (molecular) gas content in the Lyman Alpha Reference Sample (LARS), i.e. 14 local star-forming galaxies. We characterize their interstellar medium and relate newly derived properties to quantities relevant for…

Astrophysics of Galaxies · Physics 2020-11-25 J. Puschnig , M. Hayes , G. Östlin , J. Cannon , I. Smirnova-Pinchukova , B. Husemann , D. Kunth , J. Bridge , E. C. Herenz , M. Messa , I. Oteo

Using deep near-IR and optical observations of the HDF-N from the HST NICMOS and WFPC2 and from the ground, we examine the spectral energy distributions (SEDs) of Lyman break galaxies (LBGs) at 2.0 < z < 3.5. The UV-to-optical rest-frame…

Astrophysics · Physics 2008-11-26 Casey Papovich , Mark Dickinson , Henry C. Ferguson

We investigate the process of rapid star formation quenching in a sample of 12 massive galaxies at intermediate redshift (z~0.6) that host high-velocity ionized gas outflows (v>1000 km/s). We conclude that these fast outflows are most…

We present new results on the Ly-alpha emission-line kinematics of 18 z~2-3 star-forming galaxies with multiple-peaked Ly-alpha profiles. With our large spectroscopic database of UV-selected star-forming galaxies at these redshifts, we have…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-28 Kristin R. Kulas , Alice E. Shapley , Juna A. Kollmeier , Zheng Zheng , Charles C. Steidel , Kevin N. Hainline

We report the detection of Lyman continuum (LyC) photons from three massive ($\text{M}_{*}>10^{10}\:\text{M}_{\odot}$) spiral galaxies at a redshift of nearly 1 in the AstroSat UV Deep Field South. Notably, all three systems are viewed at…

Astrophysics of Galaxies · Physics 2026-01-27 Soumil Maulick , Kanak Saha

We analyze the spectra of $10$ Green Pea galaxies, previously studied by Henry et al. (2015), using a semi-analytical line transfer (SALT) model to interpret emission and absorption features observed in UV galactic spectra. We focus our…

Astrophysics of Galaxies · Physics 2021-01-20 Cody Carr , Claudia Scarlata , Alaina Henry , Nino Panagia

To date no direct detection of Lyman continuum emission has been measured for intermediate--redshift z~1 star-forming galaxies . We combine HST grism spectroscopy with GALEX UV and ground--based optical imaging to extend the search for…

We present observations of escaping Lyman Continuum (LyC) radiation from 34 massive star-forming galaxies and 12 weak AGN with reliably measured spectroscopic redshifts at $z$$\simeq$2.3-4.1. We analyzed Hubble Space Telescope Wide Field…

Some cosmological hydrodynamical simulations predict that outflows driven by active galactic nuclei (AGN) play a key role in powering the Ly$\alpha$ nebulae observed around high-redshift quasars. In such simulations, AGN feedback seeded as…