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We present spectroscopic properties of 22 Lyman-alpha emitters(LAEs) at z=5.5-6.6 with Lyman-alpha(Lya) luminosity log($L_{Lya}$[$ergs^{-1}$])=42.4-43.5, obtained using VLT/MUSE as part of the Middle Ages Galaxy Properties with Integral…

We present new Chandra observations that complete a sample of seventeen (17) luminous infrared galaxies (LIRGs) with D < 60 Mpc and low Galactic column densities of N_H < 5 X 10^20 cm^-2. The LIRGs in our sample have total infrared…

Cosmology and Nongalactic Astrophysics · Physics 2019-08-19 B. D. Lehmer , D. M. Alexander , F. E. Bauer , W. N. Brandt , A. D. Goulding , L. P. Jenkins , A. Ptak , T. P. Roberts

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…

Starting from a summary of detection statistics of our recent X-shooter campaign, we review the major surveys, both space and ground based, for emission counterparts of high-redshift damped Ly$\alpha$ absorbers (DLAs) carried out since the…

Astrophysics of Galaxies · Physics 2017-06-19 Jens-Kristian Krogager , Palle Møller , Johan P. U. Fynbo , Pasquier Noterdaeme

We present some results from an archival VLA study of ultraluminous X-ray source s (ULXs). These unresolved non-nuclear X-ray sources have luminosities (L_X >= 1 0^39 ergs/sec) which may require somewhat exotic explanations, such as…

Astrophysics · Physics 2007-05-23 Neal A. Miller , Susan G. Neff , Richard F. Mushotzky

We investigate the fraction of z ~ 0.3 Lyman alpha emitting galaxies (LAEs) which host active galactic nucleus activity, which is typically from 1 - 5% at 2 < z < 6. Using optical spectroscopy of 23 LAEs at 0.2 < z < 0.45 selected with…

Cosmology and Nongalactic Astrophysics · Physics 2009-09-24 Steven L. Finkelstein , Seth H. Cohen , Sangeeta Malhotra , James E. Rhoads , Casey Papovich , Zhenya Zheng , Junxian Wang

The origin of the Lyman-${\alpha}$ (Ly${\alpha}$) emission in galaxies is a long-standing issue: despite several processes known to originate this line (e.g. AGN, star formation, cold accretion, shock heating), it is difficult to…

Our aim is to explore the nature of emission line galaxies by combining high-resolution observations obtained in different bands to understand which objects are powered by an Active Galactic Nucleus(AGN). From the spectroscopic Palomar…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-12 B. Balmaverde , A. Capetti

A 10-arcmin field around the HDF(N) contains 92 radio sources >40 uJy, resolved by MERLIN+VLA at 0".2-2".0 resolution. 55 have Chandra X-ray counterparts including 18 with a hard X-ray photon index and high luminosity characteristic of a…

We study the average Ly$\alpha$ emission associated with high-$z$ strong (log $N$(H I) $\ge$ 21) damped Ly$\alpha$ systems (DLAs). We report Ly$\alpha$ luminosities ($L_{\rm Ly\alpha}$) for the full as well as various sub-samples based on…

Astrophysics of Galaxies · Physics 2016-12-14 Ravi Joshi , Raghunathan Srianand , Pasquier Noterdaeme , Patrick Petitjean

We review the imaging and spectroscopic properties of the Lyman alpha emission in starburst galaxies. The Lyman alpha photons escape is largely driven by kinematical and orientation effects related to the presence of large scale expanding…

Astrophysics · Physics 2007-05-23 Daniel Kunth , M. Hayes , G. Ostlin , J. M. Mas-Hesse , C. Leitherer , A. Petrosian

In active galactic nuclei (AGN), fluorescent Fe K$\alpha$ (iron) line emission is generally interpreted as originating from obscuring material around a supermassive black hole (SMBH) on the scale of a few parsecs (pc). However, recent…

Astrophysics of Galaxies · Physics 2021-06-30 Wei Yan , Ryan C. Hickox , Chien-Ting J. Chen , Claudio Ricci , Alberto Masini , Franz E. Bauer , David M. Alexander

X-ray point sources in galaxies are dominated by X-ray binaries (XRBs) that are variables or transients and whether their variability would alter the X-ray luminosity functions (XLF) is still in debate. Here we report on NGC 7331 as an…

High Energy Astrophysical Phenomena · Physics 2019-07-17 Ruolan Jin , Albert K. H. Kong

Using a sample of 92 UV continuum-selected, spectroscopically identified galaxies with <z> = 2.65, all of which have been imaged in the Ly-a line with extremely deep narrow-band imaging, we examine galaxy Ly-a emission profiles to very…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-27 C. C. Steidel , M. Bogosavljević , A. E. Shapley , J. A. Kollmeier , N. A. Reddy , D. K. Erb , M. Pettini

Recent studies of the cosmic X-ray background (XRB) have suggested the possible existence of a population of relatively faint sources with hard X-ray spectra; however, the emission mechanism remains unclear. If the hard X-ray emission is…

Astrophysics · Physics 2007-05-23 Insu Yi , Stephen P. Boughn

We built a grid of photoionization models and compiled already available observational emission line intensities ($\rm 1000 \: < \: \lambda(\AA) \: < \: 2000$) of confirmed star formation regions and Active Galactic Nucleus (AGNs) in order…

Astrophysics of Galaxies · Physics 2018-07-11 O. L. Dors , B. Agarwal , G. F. Hagele , M. V. Cardaci , C. -E. Rydberg , R. A. Riffel , A. S. Oliveira , A. C. Krabbe

The hydrogen Lyman-$\alpha$ (H {\sc i} Ly$\alpha$) emission during solar flares has rarely been studied in spatially resolved images and its physical origin has not been fully understood. In this paper, we present novel Ly$\alpha$ images…

Solar and Stellar Astrophysics · Physics 2022-09-21 Ying Li , Qiao Li , De-Chao Song , Andrea Francesco Battaglia , Hualin Xiao , Säm Krucker , Udo Schühle , Hui Li , Weiqun Gan , M. D. Ding

We analyze 18 sources that were found to show interesting properties of periodicity, very soft spectra and/or large long-term variability in X-rays in our project of classification of sources from the 2XMMi-DR3 catalog but were poorly…

High Energy Astrophysical Phenomena · Physics 2015-06-17 Dacheng Lin , Natalie A. Webb , Didier Barret

We explore the properties of high-redshift Lyman-alpha emitters (LAE), and their link with the Lyman-Break galaxy population (LBG), using a semi-analytic model of galaxy formation that takes into account resonant scattering of Lya photons…

Astrophysics of Galaxies · Physics 2015-06-24 T. Garel , J. Blaizot , B. Guiderdoni , L. Michel-Dansac , M. Hayes , A. Verhamme

We review recent results on populations of compact X-ray sources in normal galaxies. The luminosity distributions of low and high mass X-ray binaries in nearby galaxies appear to be described by the respective ``universal'' luminosity…

Astrophysics · Physics 2008-11-26 M. Gilfanov