0000000000298923

AUTHOR

Cullan Howlett

showing 2 related works from this author

The Detailed Science Case for the Maunakea Spectroscopic Explorer, 2019 edition

2019

(Abridged) The Maunakea Spectroscopic Explorer (MSE) is an end-to-end science platform for the design, execution and scientific exploitation of spectroscopic surveys. It will unveil the composition and dynamics of the faint Universe and impact nearly every field of astrophysics across all spatial scales, from individual stars to the largest scale structures in the Universe. Major pillars in the science program for MSE include (i) the ultimate Gaia follow-up facility for understanding the chemistry and dynamics of the distant Milky Way, including the outer disk and faint stellar halo at high spectral resolution (ii) galaxy formation and evolution at cosmic noon, via the type of revolutionary…

[PHYS]Physics [physics]Cosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics::Instrumentation and Methods for AstrophysicsFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics - Astrophysics of Galaxies[PHYS] Physics [physics][SDU] Sciences of the Universe [physics][SDU]Sciences of the Universe [physics]Astrophysics of Galaxies (astro-ph.GA)Astrophysics::Earth and Planetary AstrophysicsAstrophysics - Instrumentation and Methods for AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Astrophysics::Galaxy AstrophysicsAstrophysics - Cosmology and Nongalactic Astrophysics
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The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in the Data Release 10 and 11 galaxy…

2014

We present a one per cent measurement of the cosmic distance scale from the detections of the baryon acoustic oscillations in the clustering of galaxies from the Baryon Oscillation Spectroscopic Survey (BOSS), which is part of the Sloan Digital Sky Survey III (SDSS-III). Our results come from the Data Release 11 (DR11) sample, containing nearly one million galaxies and covering approximately $8\,500$ square degrees and the redshift range $0.2<z<0.7$. We also compare these results with those from the publicly released DR9 and DR10 samples. Assuming a concordance $\Lambda$CDM cosmological model, the DR11 sample covers a volume of 13\,Gpc${}^3$ and is the largest region of the Universe ever su…

AstrofísicaCosmology and GravitationCosmology and Nongalactic Astrophysics (astro-ph.CO)[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Cosmic microwave backgroundDark matterFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysicsdistance scaleAstrophysics01 natural sciencesObservacions astronòmiques0103 physical sciencesQB Astronomycosmological parametersdark energy010303 astronomy & astrophysicsQCSTFCAstrophysics::Galaxy AstrophysicsQBPhysics/dk/atira/pure/core/subjects/cosmologyCosmologia010308 nuclear & particles physicsAngular diameter distanceAstrophysics::Instrumentation and Methods for AstrophysicsSpectral densityRCUKAstronomy and AstrophysicsEspectroscòpia de microonesGalaxyRedshiftobservations [cosmology]CosmologyBaryonQC Physics13. Climate actionSpace and Planetary ScienceMicrowave spectroscopyBaryon acoustic oscillationslarge-scale structure of UniverseAstrophysics - Cosmology and Nongalactic AstrophysicsAstronomical observations
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