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相关论文: Fluorescent Ly-alpha emission from the high-redshi…

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We use very large cosmological Smoothed-Particle-Hydrodynamics simulations to study the properties of high redshift Lyman-alpha emitters (LAEs). We identify star-forming galaxies at z=3.1 in a cosmological volume of 100 h^-1Mpc on a side.…

宇宙学与河外天体物理 · 物理学 2015-05-27 Ikkoh Shimizu , Naoki Yoshida , Takashi Okamoto

How galaxies acquire material from the circumgalactic medium (CGM) is a key question in galaxy evolution. Recent observations and simulations show that gas recycling could be an important avenue for star formation. This paper presents Keck…

Observations by the Large Area Telescope (LAT) on the \textit{Fermi} mission of diffuse $\gamma$-rays in a mid-latitude region in the third quadrant (Galactic longitude $l$ from $200\arcdeg$ to $260\arcdeg$ and latitude $| b |$ from…

高能天体物理现象 · 物理学 2009-12-04 A. A. Abdo

We investigate Lyman-$\alpha$ transmission spikes at $z > 5$ in synthetic quasar spectra, and discuss their connection to the properties of the intergalactic medium and their ability to constrain reionization models. We use state-of-the-art…

宇宙学与河外天体物理 · 物理学 2019-05-08 Enrico Garaldi , Nickolay Gnedin , Piero Madau

We investigate the large-scale inhomogeneities of the hydrogen ionizing radiation field in the Universe at redshift z=3. Using a raytracing algorithm, we simulate a model in which quasars are the dominant sources of radiation. We make use…

天体物理学 · 物理学 2009-11-10 Rupert A. C. Croft

Several Lyman-alpha (Ly$\alpha$) emitters deep into the reionization era exhibit double-peaked Ly$\alpha$ emission profiles, raising the question of how the intergalactic medium can transmit photons blueward of the Ly$\alpha$ resonance at…

We present an exhaustive census of Lyman alpha (Ly$\alpha$) emission in the general galaxy population at $3<z<4.6$. We use the Michigan/Magellan Fiber System (M2FS) spectrograph to study a stellar mass (M$_*$) selected sample of 625…

星系天体物理 · 物理学 2017-07-17 Grecco A. Oyarzún , Guillermo A. Blanc , Valentino González , Mario Mateo , John I. Bailey

We study the three-dimensional distribution of non virialised matter at z~2 using high resolution spectra of QSO pairs and simulated spectra drawn from cosmological hydrodynamical simulations. We have collected the largest sample of QSO…

天体物理学 · 物理学 2009-11-11 V. D'Odorico , M. Viel , F. Saitta , S. Cristiani , S. Bianchi , B. Boyle , S. Lopez , J. Maza , P. Outram

The intense UV radiation from a highly luminous QSO should excite fluorescent Ly-alpha emission from any nearby neutral hydrogen clouds. We present a very deep narrow-band search for such emission near the z=2.168 quasar PKS 0424-131,…

天体物理学 · 物理学 2011-03-10 Paul J. Francis , Joss Bland-Hawthorn

We present a new model for high redshift Lyman-Alpha Emitters (LAEs) in the cosmological context which takes into account the resonant scattering of Ly-a photons through expanding gas. The GALICS semi-analytic model provides us with the…

宇宙学与河外天体物理 · 物理学 2015-06-04 Thibault Garel , Jérémy Blaizot , Bruno Guiderdoni , Daniel Schaerer , Anne Verhamme , Matthew Hayes

We present an analysis of high-resolution hydrodynamical N-body simulations of coupled dark energy cosmologies which focusses on the statistical properties of the transmitted Lyman-alpha flux in the high-redshift intergalactic medium (IGM).…

宇宙学与河外天体物理 · 物理学 2015-05-19 Marco Baldi , Matteo Viel

This thesis deals with different aspects of a special kind of high redshift galaxy, namely Ly-alpha emitters. Ly-alpha emitters are galaxies found through their Ly-alpha emission, at redshifts larger than z >~ 2 where the emission line has…

天体物理学 · 物理学 2007-11-15 Kim K. Nilsson

Distant luminous Lyman-alpha emitters are excellent targets for detailed observations of galaxies in the epoch of reionisation. Spatially resolved observations of these galaxies allow us to simultaneously probe the emission from young…

星系天体物理 · 物理学 2020-06-10 Jorryt Matthee , David Sobral

Lyman-$\alpha$ (Ly$\alpha$) emitting galaxies are powerful tools to probe the late stages of cosmic reionization. The observed sudden drop in Ly$\alpha$ fraction at $z>6$ is often interpreted as a sign of reionization, since the…

宇宙学与河外天体物理 · 物理学 2021-03-03 Sultan Hassan , Max Gronke

Observations of reionization-era analogs at $z\sim3$ are a powerful tool for constraining reionization. Rest-ultraviolet observations are particularly useful, in which both direct and indirect tracers of ionizing-photon production and…

星系天体物理 · 物理学 2022-06-24 Anthony J. Pahl , Alice Shapley , Charles C. Steidel , Yuguang Chen , Naveen A. Reddy

High-redshift QSO spectra show large spatial fluctuations in the Ly-alpha opacity of the intergalactic medium on surprisingly large scales at z>~5.5. We present a radiative transfer simulation of cosmic reionization driven by galaxies that…

We present results of a deep spectroscopic survey designed to quantify the statistics of the escape of ionizing photons from star-forming galaxies at z~3. We measure the ratio of ionizing to non-ionizing UV flux density <f900/f1500>_obs,…

星系天体物理 · 物理学 2018-12-26 C. C. Steidel , M. Bogosavljevic , A. E. Shapley , N. A. Reddy , G. C. Rudie , M. Pettini , R. F. Trainor , A. L. Strom

(abridged) We present an effective implementation of analytical calculations of the Lyalpha opacity distribution of the Intergalactic Medium (IGM) along multiple lines of sight (LOS) to distant quasars in a cosmological setting. This method…

天体物理学 · 物理学 2009-11-06 M. Viel , S. Matarrese , H. J. Mo , M. G. Haehnelt , Tom Theuns

We report the results of a survey for fluorescent Ly-alpha emission carried out in the field surrounding the z=3.1 quasar QSO0420-388 using the FORS2 instrument on the VLT. We first review the properties expected for fluorescent Ly-alpha…

天体物理学 · 物理学 2008-11-26 Sebastiano Cantalupo , Simon J. Lilly , Cristiano Porciani

We model the spectra and surface brightness distributions for the Lyman alpha (Lya) radiation expected from protogalaxies that are caught in the early stages of their assembly. We use the results of a companion paper to characterize the…

天体物理学 · 物理学 2008-11-26 Mark Dijkstra , Zoltan Haiman , Marco Spaans