output
19932026
most citedGaia Data Release 2. Summary of the contents and survey properties

8.6k citations

Showing 2014 · astro-ph.IMShow all

24 papers · 2 filters

astro-ph.IM2014★ 54 cited

Performance characterization of a broadband vector Apodizing Phase Plate coronagraph

G. P. P. L. Otten, F. Snik, M. A. Kenworthy +2

One of the main challenges for the direct imaging of planets around nearby stars is the suppression of the diffracted halo from the primary star. Coronagraphs are angular filters t…

astro-ph.IM2014★ 183 cited

Laboratory formation of fullerenes from PAHs: Top-down interstellar chemistry

Junfeng Zhen, Pablo Castellanos, Daniel M. Paardekooper +2

Interstellar molecules are thought to build up in the shielded environment of molecular clouds or in the envelope of evolved stars. This follows many sequential reaction steps of a…

astro-ph.IM2014★ 73 cited

Measuring a Cherenkov ring in the radio emission from air showers at 110-190 MHz with LOFAR

A. Nelles, P. Schellart, S. Buitink +66

Measuring radio emission from air showers offers a novel way to determine properties of the primary cosmic rays such as their mass and energy. Theory predicts that relativistic tim…

astro-ph.IM2014

On the Reliability of N-body Simulations

Tjarda Boekholt, Simon Portegies Zwart

The general consensus in the N-body community is that statistical results of an ensemble of collisional N-body simulations are accurate, even though individual simulations are not.…

astro-ph.IM2014★ 38 cited

The LOFAR long baseline snapshot calibrator survey

J. Moldón, A. T. Deller, O. Wucknitz +82

Aims. An efficient means of locating calibrator sources for International LOFAR is developed and used to determine the average density of usable calibrator sources on the sky for s…

astro-ph.IM2014★ 201 cited

A scheme for radiation pressure and photon diffusion with the M1 closure in RAMSES-RT

J. Rosdahl, R. Teyssier

We describe and test an updated version of radiation-hydrodynamics (RHD) in the RAMSES code, that includes three new features: i) radiation pressure on gas, ii) accurate treatment…

astro-ph.IM2014★ 107 cited

The Australian Square Kilometre Array Pathfinder: System Architecture and Specifications of the Boolardy Engineering Test Array

A. W. Hotan, J. D. Bunton, L. Harvey-Smith +98

This paper describes the system architecture of a newly constructed radio telescope - the Boolardy Engineering Test Array, which is a prototype of the Australian Square Kilometre A…

astro-ph.IM2014★ 5 cited

The Influence of Social Movements on Space Astronomy Policy

Hannah E. Harris, Pedro Russo

Public engagement (PE) initiatives can lead to a long term public support of science. However most of the real impact of PE initiatives within the context of long-term science poli…

astro-ph.IM2014★ 15 cited

A connected component-based method for efficiently integrating multiscale -body systems

Jürgen Jänes, Federico I. Pelupessy, Simon F. Portegies Zwart

We present a novel method for efficient direct integration of gravitational N-body systems with a large variation in characteristic time scales. The method is based on a recursive…

astro-ph.IM2014★ 3 cited

UVMag: Space UV and visible spectropolarimetry

Martin Pertenais, Coralie Neiner, Laurent Pares +3

UVMag is a project of a space mission equipped with a high-resolution spectropolarimeter working in the UV and visible range. This M-size mission will be proposed to ESA at its M4…

astro-ph.IM2014★ 25 cited

Lunar occultation of the diffuse radio sky: LOFAR measurements between 35 and 80 MHz

H. K. Vedantham, L. V. E. Koopmans, A. G. de Bruyn +91

We present radio observations of the Moon between and MHz to demonstrate a novel technique of interferometrically measuring large-scale diffuse emission extending far bey…

astro-ph.IM2014★ 13 cited

Gaia on-board metrology: basic angle and best focus

A. Mora, M. Biermann, A. G. A. Brown +21

The Gaia payload ensures maximum passive stability using a single material, SiC, for most of its elements. Dedicated metrology instruments are, however, required to carry out two f…

astro-ph.IM2014★ 377 cited

Fundamental limitations of high contrast imaging set by small sample statistics

Dimitri Mawet, Julien Milli, Zahed Wahhaj +9

In this paper, we review the impact of small sample statistics on detection thresholds and corresponding confidence levels (CLs) in high contrast imaging at small angles. When look…

astro-ph.IM2014★ 1 cited

Focal-plane wavefront sensing with high-order adaptive optics systems

Visa Korkiakoski, Christoph U. Keller, Niek Doelman +3

We investigate methods to calibrate the non-common path aberrations at an adaptive optics system having a wavefront-correcting device working at an extremely high resolution (large…

astro-ph.IM2014★ 14 cited

Big Data analytics and Cognitive Computing: future opportunities for Astronomical research

Michael Garrett

The days of the lone astronomer with his optical telescope and photographic plates are long gone: Astronomy in 2025 will not only be multi-wavelength, but multi-messenger, and domi…

astro-ph.IM2014★ 36 cited

Fast & Furious focal-plane wavefront sensing

Visa Korkiakoski, Christoph U. Keller, Niek Doelman +3

We present two complementary algorithms suitable for using focal-plane measurements to control a wavefront corrector with an extremely high spatial resolution. The algorithms use l…

astro-ph.IM2014★ 109 cited

LOFAR Sparse Image Reconstruction

H. Garsden, J. N. Girard, J. L. Starck +77

Context. The LOw Frequency ARray (LOFAR) radio telescope is a giant digital phased array interferometer with multiple antennas distributed in Europe. It provides discrete sets of F…

astro-ph.IM2014★ 76 cited

Deep sea tests of a prototype of the KM3NeT digital optical module

S. Adrián-Martínez, M. Ageron, F. Aharonian +247

The first prototype of a photo-detection unit of the future KM3NeT neutrino telescope has been deployed in the deep waters of the Mediterranean Sea. This digital optical module has…

astro-ph.IM2014★ 5 cited

EFTCAMB/EFTCosmoMC: Numerical Notes v3.0

Bin Hu, Marco Raveri, Noemi Frusciante +1

EFTCAMB/EFTCosmoMC are publicly available patches to the CAMB/CosmoMC codes implementing the effective field theory approach to single scalar field dark energy and modified gravity…

astro-ph.IM2014★ 142 cited

Galaxy And Mass Assembly (GAMA): autoz spectral redshift measurements, confidence and errors

I. K. Baldry, M. Alpaslan, A. E. Bauer +17

The Galaxy And Mass Assembly (GAMA) survey has obtained spectra of over 230000 targets using the Anglo-Australian Telescope. To homogenise the redshift measurements and improve the…

astro-ph.IM2014★ 100 cited

Direct detection of exoplanets in the 3 -- 10 micron range with E-ELT/METIS

Sascha P. Quanz, Ian Crossfield, Michael R. Meyer +2

We quantify the scientific potential for exoplanet imaging with the Mid-infrared E-ELT Imager and Spectrograph (METIS) foreseen as one of the instruments of the European Extremely…

astro-ph.IM2014★ 49 cited

On the minimal accuracy required for simulating self-gravitating systems by means of direct N-body methods

Simon Portegies Zwart, Tjarda Boekholt

The conservation of energy, linear momentum and angular momentum are important drivers for our physical understanding of the evolution of the Universe. These quantities are also co…

astro-ph.IM2014★ 8 cited

Multi-scale and multi-domain computational astrophysics

A. van Elteren, F. I. Pelupessy, S. Portegies Zwart

Astronomical phenomena are governed by processes on all spatial and temporal scales, ranging from days to the age of the Universe (13.8,Gyr) as well as from km size up to the size…

astro-ph.IM2014★ 5 cited

Determination of the position angle of stellar spin axes

Anna-Lea Lesage, Guenter Wiedemann

Measuring the stellar position angle provides valuable information on binary stellar formation or stellar spin axis evolution. We aim to develop a method for determining the absolu…