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Alpha Shape Topology of the Cosmic Web

Astronomy and Astrophysics – Astrophysics – Cosmology and Extragalactic Astrophysics
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AlterBBN: A program for calculating the BBN abundances of the elements in alternative cosmologies

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Alternative diagnostic diagrams and the "forgotten" population of weak line galaxies in the SDSS

Astronomy and Astrophysics – Astrophysics – Cosmology and Extragalactic Astrophysics
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Alternative inflationary scenario due to compact extra dimensions

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Alternatives to dark matter: Modified gravity as an alternative to dark matter

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Ambiguities in second-order cosmological perturbations for non-canonical scalar fields

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Ambiguous Tests of General Relativity on Cosmological Scales

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Ameliorating Systematic Uncertainties in the Angular Clustering of Galaxies: A Study using SDSS-III

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AMiBA Wideband Analog Correlator

Astronomy and Astrophysics – Astrophysics – Cosmology and Extragalactic Astrophysics
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AMiBA: Broadband Heterodyne CMB Interferometry

Astronomy and Astrophysics – Astrophysics – Cosmology and Extragalactic Astrophysics
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AMiBA: scaling relations between the integrated Compton-y and X-ray derived temperature, mass, and luminosity

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AMiBA: Sunyaev-Zel'dovich effect derived properties and scaling relations of massive galaxy clusters

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AMIGA project: Quantification of the isolation of 950 CIG galaxies

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Ammonia (J,K) = (1,1) to (4,4) and (6,6) inversion lines detected in the Seyfert 2 galaxy NGC 1068

Astronomy and Astrophysics – Astrophysics – Cosmology and Extragalactic Astrophysics
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Ammonia as a Temperature Tracer in the Ultraluminous Galaxy Merger Arp220

Astronomy and Astrophysics – Astrophysics – Cosmology and Extragalactic Astrophysics
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Ammonia as a Tracer of Fundamental Constants

Astronomy and Astrophysics – Astrophysics – Cosmology and Extragalactic Astrophysics
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Amplitudes of thermal and kinetic Sunyaev-Zel'dovich signals from small-scale CMB anisotropies

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AMUSE-VIRGO. III: mid-infrared photometry of early-type galaxies and limits on obscured nuclear emission

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An Accounting of the Dust-Obscured Star Formation and Accretion Histories Over the Last ~11~Billion Years

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An accurate measurement of the anisotropies and mean level of the Cosmic Infrared Background at 100 and 160 um

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