Results 11 to 20 of about 5,863 (203)
Lyman Alpha Emitting Galaxies in the Nearby Universe [PDF]
AbstractThe Lyman alpha emission line (Lyα) of neutral hydrogen (Hi) is intrinsically the brightest emission feature in the spectrum of astrophysical nebulae, making it a very attractive observational feature with which to survey galaxies. Moreover as an ultraviolet resonance line, Lyα possesses several unique characteristics that make it useful to ...
Hayes, Matthew,
openaire +3 more sources
Chemodynamics of Lyman alpha emitters, Lyman break galaxies and elliptical galaxies [PDF]
We report an ultra-high-resolution simulation that follows evolution from the earliest stages of galaxy formation through the period of dynamical relaxation. The bubble structures of gas revealed in our simulation ($< 3\times 10^8$ years) resemble closely the high-redshift Lyman $α$ emitters (LAEs).
Mori, Masao, Umemura, Masayuki
openaire +3 more sources
Observing Lyman alpha emitters - How does Lyman alpha escape from galaxies?
The Lyman alpha (Lyα) emission line has grown to become one of the most successful tools for finding galaxies at high redshift. At redshifts corresponding to the early cosmic times of reionization and primeval galaxy formation, the wavelength of Lyα is still accessible with ground-based facilities.
Sandberg, Andreas
openaire +2 more sources
The Lensed Lyman-Alpha MUSE Arcs Sample (LLAMAS) : I. Characterisation of extended Lyman-alpha haloes and spatial offsets [PDF]
We present the Lensed Lyman-Alpha MUSE Arcs Sample (LLAMAS) selected from MUSE and HST observations of 17 lensing clusters.
Bacon, Roland +63 more
core +1 more source
Cystic fibrosis year in review 2022
Abstract Remarkable medical advancements have been made for people with cystic fibrosis (CF) in recent years, with an abundance of research continuing to be conducted worldwide. With concern for limitations in access to highly effective CFTR modulators, as well as the recent Coronavirus Disease‐19 pandemic, there has been a consistent effort to ...
Jeeyeon Kim +2 more
wiley +1 more source
PAWS and POCO: NIR Astrophotonic Instruments for Astronomy
Abstract For near‐infrared ground and space‐based astronomy, compact photonic devices can replace the large bulk optical components in spectrographs, frequency combs, beam combiners, and sky subtraction filters, thus saving cost, reducing volume, weight, and power requirements.
Kalaga Madhav +8 more
wiley +1 more source
Characterizing Strongly-Lensed Lyman-Alpha Galaxies at z > 4
Lyman-alpha is one of the most important tools for studying star-forming regions in young galaxies. As Hydrogen's brightest recombination line, it is an excellent tracer for star formation during the Epoch of Reionization.
Navarre, Alexander
core +1 more source
Future Climate Under CMIP6 Solar Activity Scenarios
Abstract Predictions of solar activity in the future are difficult to make due to the chaotic state of solar dynamo and the high nonlinearity of physical processes on the Sun. Therefore, the Climate Intercomparison Project Phase 6 (CMIP6) used a statistical approach and recommended two different solar forcing scenarios for the simulations.
Jan Sedlacek +4 more
wiley +1 more source
Lyman break galaxies and the star formation rate of the Universe at z ~ 6 [PDF]
We determine the space density of UV-luminous starburst galaxies at z≈ 6 using deep HST ACS SDSS-i′ (F775W) and SDSS-z′ (F850LP) and VLT ISAAC J and Ks band imaging of the Chandra Deep Field South.
Stanway, Elizabeth R. +6 more
core +1 more source
Revisiting the emission line source detection problem in integral field spectroscopic data
Abstract We present a 3‐dimensional matched filtering approach for the blind search of faint emission‐line sources in integral‐field spectroscopic datasets. The filter is designed to account for the spectrally rapidly varying background noise due to the telluric air glow spectrum.
Edmund Christian Herenz
wiley +1 more source

