output
19992026
most citedThe Supernova Legacy Survey: Measurement of Omega_M, Omega_Lambda and w from the First Year Data Set

2.4k citations

Showing 2017Show all

44 papers · 1 filter

astro-ph.EP2017★ 4 cited

Future Exoplanet Research: Science Questions and How to Address Them

Jean Schneider

Started approximately in the late 1980s, exoplanetology has up to now unveiled the main gross bulk characteristics of planets and planetary systems. In the future it will benefit f…

astro-ph.GA2017★ 151 cited

Diffuse ionized gas in galaxies across the Hubble sequence at the CALIFA resolution

E. A. D. Lacerda, R. Cid Fernandes, G. S. Couto +7

We use spatially resolved spectroscopy from the Calar Alto Legacy Field Area (CALIFA) survey to study the nature of the line emitting gas in galaxies of different Hubble types, foc…

astro-ph.HE2017★ 12 cited

Nonradial and nonpolytropic astrophysical outflows. X. Relativistic MHD rotating spine jets in Kerr metric

L. Chantry, V. Cayatte, C. Sauty +2

High resolution radio imaging of AGN have revealed that some sources present motion of superluminal knots and transverse stratification of their jet. Recent observational projects…

astro-ph.CO2017★ 1 cited

Cosmology with 21cm intensity mapping

Isabella P. Carucci

The nature of the most abundant components of the Universe, dark energy and dark matter, is still to be uncovered. I tackle this subject considering a novel cosmological probe: the…

astro-ph.GA2017★ 13 cited

Exploring the inner parsecs of Active Galactic Nuclei using near-infrared high resolution polarimetric simulations with MontAGN

Lucas Grosset, Daniel Rouan, Damien Gratadour +4

Aims: In this paper, we aim to constrain the properties of dust structures in the central first parsecs of Active Galactic Nuclei (AGN). Our goal is to study the required optical d…

astro-ph.CO2017★ 21 cited

The Linear Point Standard Ruler for galaxy survey data: validation with mock catalogues

Stefano Anselmi, Pier-Stefano Corasaniti, Glenn D. Starkman +2

Due to late time non-linearities, the location of the acoustic peak in the two-point galaxy correlation function is a redshift-dependent quantity, thus it cannot be simply employed…