Observations of the Lyman- Universe
arXiv:2012.07960 · doi:10.1146/annurev-astro-032620-021859
Abstract
Hydrogen Lyman- (Ly) emission has been one of the major observational probes for the high redshift universe, since the first discoveries of high- Ly emitting galaxies in the late 1990s. Due to the strong Ly emission originated by resonant scattering and recombination of the most-abundant element, Ly observations witness not only HII regions of star formation and AGN but also diffuse HI gas in the circum-galactic medium (CGM) and the inter-galactic medium (IGM). Here we review Ly sources, and present theoretical interpretations reached to date. We conclude that: 1) A typical Ly emitter (LAE) at with a Ly luminosity is a high- counterpart of a local dwarf galaxy, a compact metal-poor star-forming galaxy (SFG) with an approximate stellar (halo) mass and star-formation rate of () and yr, respectively; 2) High- SFGs ubiquitously have a diffuse Ly emitting halo in the CGM extending to the halo virial radius and beyond; 3) Remaining neutral hydrogen at the epoch of reionization makes a strong dimming of Ly emission for galaxies at that suggest the late reionization history. The next generation large telescope projects will combine Ly emission data with HI Ly absorptions and 21cm radio data that map out the majority of hydrogen (HI+HII) gas, uncovering the exchanges of i) matter by outflow/inflow and ii) radiation, relevant to cosmic reionization, between galaxies and the CGM/IGM.
arXiv comment45 pages, 18 figures. Invited review published in Annual Reviews of Astronomy and Astrophysics. See https://www.annualreviews.org/doi/abs/10.1146/annurev-astro-032620-021859 for updated version
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- The MUSE Extremely Deep Field: Classifying the Spectral Shapes of Lya Emitting Galaxies
- Constraining the 21cm brightness temperature of the IGM at =6.6 around LAEs with the Murchison Widefield Array
- Galaxy populations in protoclusters at cosmic noon
- Influence of mergers on LyC escape of high redshift galaxies
- Identifying Lyα emitter candidates with Random Forest: learning from galaxies in CANDELS survey
- Photometric IGM Tomography: Efficiently Mapping Quasar Light Echoes with Deep Narrow Band Imaging
- The miniJPAS Survey: Detection of double-core Lyα morphology of two high-redshift (z>3) QSOs
- Spectroscopy of an extreme [OIII] emitting active galactic nucleus at : implications for the reionisation era
- MUSE Analysis of Gas around Galaxies (MAGG) -- VI. The cool and enriched gas environment of z3 Ly emitters
- Quenching of Galaxies at Cosmic Noon: Understanding the Effect of Environment
- The Role of Dust, UV Luminosity and Large-scale Environment on the Escape of Lya Photons: A Case Study of a Protocluster field at z = 3.1
- Probing the cosmic web in Ly emission over large scales: an Intensity Mapping forecast for DECaLS/BASS and DESI
- Photometric IGM tomography with Subaru/HSC: the large-scale structure of Ly emitters and IGM transmission in the COSMOS field at
- The miniJPAS & J-NEP surveys: Identification and characterization of the Ly Emitter population and the Ly Luminosity Function
- Generation of high circular polarization of interstellar Lyman radiation triggering biological homochirality
- Three-Dimensional Stacking as a Line Intensity Mapping Statistic
- Lyman-alpha at Cosmic Noon I: Ly-alpha Spectral Type Selection of z ~ 2-3 Lyman Break Galaxies with Broadband Imaging
- The Intrinsic Distribution of Lyman- Halos
- Circumgalactic Ly Nebulae in Overdense Quasar Pair Regions Observed with the Palomar Cosmic Web Imager
- The Active Galactic Nuclei in the Hobby-Eberly Telescope Dark Energy Experiment Survey (HETDEX) III. A red quasar with extremely high equivalent widths showing powerful outflows
- Modelling LAEs in the Epoch of Reionization with OBELISK
- The Lyman Alpha Reference Sample. XVI. Global 21cm HI properties of Lyman- emitting galaxies
- Near-IR narrow-band imaging with CIRCE at the Gran Telescopio Canarias: Searching for Ly-emitters at
- Impact of reionization history on constraining primordial gravitational waves in future all-sky cosmic microwave background experiments
- zELDA II: reconstruction of galactic Lyman-alpha spectra attenuated by the intergalactic medium using neural networks
- Impact of redshift distribution uncertainties on Lyman-break galaxy cosmological parameter inference
- Direct correlation of line intensity mapping and CMB lensing from evolution along the lightcone
- Influence of turbulence on Lyman-alpha scattering
- Reionization in Protocluster Environments at with JWST/NIRSpec
- Lyα Intensity Mapping in HETDEX: Galaxy-Lyα Intensity Cross-Power Spectrum
- On the Evidence for Molecular Outflows in High-redshift Dusty Star-forming Galaxies
- The effect of ionizing background fluctuations on the spatial correlations of high redshift Ly-emitting galaxies
- On the Origin of the Strong Optical Variability of Emission-line Galaxies
- HETDEX Public Data Release 1: Source Catalog 2 and Data Cubes from ~90 sq deg of Integral-Field Optical Spectroscopy
- Deep JWST spectroscopy of galaxies in a candidate ionized bubble at : probing reionization at pMpc scales with Ly emission
- Mapping neutral islands during end stages of reionization with photometric intergalactic medium tomography
- A physically-motivated template set for high-z galaxy SED fitting
- Can luminous Lyman alpha emitters at 5.7 and 6.6 suppress star formation?
- Lyman-alpha at Cosmic Noon II: The relationship between kinematics and Lyman-alpha in z~2-3 Lyman Break Galaxies
- ODIN: Using multiplicity of Lyman-Alpha Emitters to assess star formation activity in dark matter halos
- ODIN: A New Lyman Alpha Blob Selection Method, Sample, and Statistical Analysis at
- A Lyman continuum analysis for galaxies at in the Abell 2744 Cluster Field
- Double-Peaked Ly Emission during Reionization Requires Nearby Voids and a Favorable Local Ionizing Background
- Direct Collapse Pre-supermassive Black Hole Objects as Ly Emitters
- A gradient boosting and broadband approach to finding Lyman-α emitting galaxies beyond narrowband surveys
- MUSE Analysis of Gas around Galaxies (MAGG) -- VII. Emission line galaxies near strong blended Ly absorption systems at
- Resolving dust and Lyα emission in a lensed galaxy at the epoch of reionization with JWST/CANUCS
- The ALMA View of High-Redshift Galaxy Formation
- Clustering analysis of medium-band selected high-redshift galaxies
- Resolving circumgalactic gas flows around a z3.6 quasar using MUSE and ALMA
- Bayesian luminosity function estimation in multi-depth datasets with selection effects: A case study for Lyman emitters
- The stellar population of a Ly emitting group associated with a damped Ly absorber
- A Non-parametric Method for the Inference of Halo Occupation Distributions