Observations of Ly Emitters at High Redshift
arXiv:2012.11645 · doi:10.1007/978-3-662-59623-4_3
Abstract
In this series of lectures, I review our observational understanding of high- Ly emitters (LAEs) and relevant scientific topics. Since the discovery of LAEs in the late 1990s, more than ten (one) thousand(s) of LAEs have been identified photometrically (spectroscopically) at to . These large samples of LAEs are useful to address two major astrophysical issues, galaxy formation and cosmic reionization. Statistical studies have revealed the general picture of LAEs' physical properties: young stellar populations, remarkable luminosity function evolutions, compact morphologies, highly ionized inter-stellar media (ISM) with low metal/dust contents, low masses of dark-matter halos. Typical LAEs represent low-mass high- galaxies, high- analogs of dwarf galaxies, some of which are thought to be candidates of population III galaxies. These observational studies have also pinpointed rare bright Ly sources extended over kpc, dubbed Ly blobs, whose physical origins are under debate. LAEs are used as probes of cosmic reionization history through the Ly damping wing absorption given by the neutral hydrogen of the inter-galactic medium (IGM), which complement the cosmic microwave background radiation and 21cm observations. The low-mass and highly-ionized population of LAEs can be major sources of cosmic reionization. The budget of ionizing photons for cosmic reionization has been constrained, although there remain large observational uncertainties in the parameters. Beyond galaxy formation and cosmic reionization, several new usages of LAEs for science frontiers have been suggested such as the distribution of {\sc Hi} gas in the circum-galactic medium and filaments of large-scale structures. On-going programs and future telescope projects, such as JWST, ELTs, and SKA, will push the horizons of the science frontiers.
arXiv commentLecture notes for `Lyman-alpha as an Astrophysical and Cosmological Tool', Saas-Fee Advanced Course 46. Verhamme, A., North, P., Cantalupo, S., & Atek, H. (eds.) --- 147 pages, 103 figures. Abstract abridged. Link to the lecture program including the video recording and ppt files : https://obswww.unige.ch/Courses/saas-fee-2016/program.cgi
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- Resolving the unresolved cosmic X-ray background in the Chandra Deep Fields
- Linking Ly-alpha and Low-Ionization Transitions at Low Optical Depth
- Clustering of Lyman alpha emitters at z ~ 4.5
- The ionizing photon production efficiency of compact z~0.3 Lyman continuum leakers and comparison with high redshift galaxies
- The Serendipitous Discovery of a Group or Cluster of young Galaxies at z=2.40 in Deep Hubble Space Telescope WFPC2 Images
- Panoramic Survey of Lyman α Emitters at z=3.1
- Initial LOFAR observations of Epoch of Reionization windows: II. Diffuse polarized emission in the ELAIS-N1 field
- Neutral hydrogen optical depth near star-forming galaxies at z~2.4 in the Keck Baryonic Structure Survey
- Statistical Properties of Diffuse Lyman-alpha Halos around Star-forming Galaxies at z~2
- Escape fraction of ionizing photons from galaxies at z=0--6
- Sizing up Lyman-alpha and Lyman Break Galaxies
- Black hole growth in the early Universe is self-regulated and largely hidden from view
- Ly alpha emitting galaxies as early stages in galaxy formation
- The cosmic star formation rate evolution from z=5 to z=0 from the VIMOS VLT Deep Survey
- Nebular Attenuation in Hα-selected Star-forming Galaxies at z=0.8 from the NewHα Survey
- The Faintest X-ray Sources from z=0-8
- Probing the z>6 Universe with the first Hubble Frontier Fields cluster Abell 2744
- The contribution of faint AGNs to the ionizing background at z~4
- Lyman-alpha Emitters and Lyman-break Galaxies at z=3-6 in Cosmological SPH Simulations
- The Discovery of a Large Lyman-alpha+HeII Nebula at z~1.67: A Candidate Low Metallicity Region?
- Probing Galaxy Formation with He II Cooling Lines
- The Polarization of Scattered Lyman Alpha Radiation Around High-Redshift Galaxies
- Filamentary Infall of Cold Gas and Escape of Lyman Alpha and Hydrogen Ionizing Radiation from an Interacting High-Redshift Galaxy
- Reionization, SLOAN, and WMAP: is the Picture Consistent?
- The GC Simulations : Quantifying the Dark Side of the Universe in the Planck Cosmology
- Evolution of N/O Abundance Ratios and Ionization Parameters from z~0 to 2 Investigated by the Direct Temperature Method
- Probing Intergalactic Neutral Hydrogen by the Lyman Alpha Red Damping Wing of Gamma-Ray Burst 130606A Afterglow Spectrum at z = 5.913
- HST Emission Line Galaxies at z ~ 2: Comparing Physical Properties of Lyman Alpha and Optical Emission Line Selected Galaxies
- On the UV compactness and morphologies of typical Lyman-a emitters from z~2 to z~6
- The baryonic mass function of galaxies
- A High Fraction of Ly-alpha-Emitters Among Galaxies with Extreme Emission Line Ratios at z ~ 2
- The luminosity function of Ly-alpha emitters at 2.3 < z < 4.6 from integral-field spectroscopy
- Large-scale clustering of Lyman-alpha emission intensity from SDSS/BOSS
- A Ly-alpha Emitter with an Extremely Large Rest-frame Equivalent Width of ~900A at z=6.5: A Candidate of Population III-dominated Galaxy?
- On the influence of physical galaxy properties on Lyman-alpha escape in star-forming galaxies
- CHORUS II. Subaru/HSC Determination of the Ly Luminosity Function at : Constraints on Cosmic Reionization Model Parameter
- On the nature and physical conditions of the luminous Lya emitter CR7 and its rest-frame UV components
- Intensity mapping with SDSS/BOSS Lyman-alpha emission, quasars and their Lyman-alpha forest
- Spectral Energy Distribution Fitting of HETDEX Pilot Survey Lyman-alpha Emitters in COSMOS and GOODS-N
- Searching for Neutral Hydrogen Halos around z ~ 2.1 and z ~ 3.1 Ly-alpha Emitting Galaxies
- On the Diffuse Lyman-alpha Halo Around Lyman-alpha Emitting Galaxies
- X-Ray Detection of an Obscured Active Galactic Nucleus in a z=3.09 Radio-quiet Ly-alpha Nebula
- Singly-Peaked P-Cygni type Ly from starburst galaxies
- Spatially Resolved Gas Kinematics within a Ly Nebula: Evidence for Large-scale Rotation
- The Diversity of Diffuse Ly Nebulae around Star-Forming Galaxies at High Redshift
- Modelling high redshift Lyman-alpha Emitters
- Dwarf Galaxy Formation Was Suppressed By Cosmic Reionization
- Lyman Alpha Signatures from Direct Collapse Black Holes
- A Lyman alpha emitter at z = 6.5 found with slitless spectroscopy
- No evidence of obscured, accreting black holes in most z=6 star-forming galaxies
- Lyman-alpha blobs: polarization arising from cold accretion
- Exploring 21cm - Lyman Alpha emitter synergies for SKA
- Constraining the Quasar Contribution to the Reionisation of Cosmic Hydrogen
- Evidence for Spatially Compact Lyman Alpha Emission in z=3.1 Lyman-Alpha-Emitting Galaxies
- Constraints on the faint end of the quasar luminosity function at z~5 in the COSMOS field
- Cross-correlation of the cosmic 21-cm signal and Lyman Alpha Emitters during reionization
- HeII emission in Lyman-alpha nebulae: AGN or cooling radiation?
- The reanalysis of spectra of GRB 080913 to estimate the neutral fraction of the IGM at a redshift of 6.7
- Hubble Space Telescope Imaging of Lyman Alpha Emission at z=4.4
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- Magellan/MMIRS near-infrared multi-object spectroscopy of nebular emission from star forming galaxies at 2<z<3
- Fast Identification of Bound Structures in Large N-body Simulations
- The Line Polarization Within a Giant Lyman-alpha Nebula
- Expanding shells of shocked neutral hydrogen around compact HII regions
- First Infrared-based implications for the dust attenuation and star formation of typical Ly emitters
- Understanding the redshift evolution of the luminosity functions of Lyman-alpha emitters
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