output
19922026
most citedThe SIESTA method for ab initio order-N materials simulation

12k citations

Showing 2017 · astro-ph.IMShow all

8 papers · 2 filters

astro-ph.IM2017★ 40 cited

Supervised detection of exoplanets in high-contrast imaging sequences

Carlos Alberto Gomez Gonzalez, Olivier Absil, Marc van Droogenbroeck

Post-processing algorithms play a key role in pushing the detection limits of high-contrast imaging (HCI) instruments. State-of-the-art image processing approaches for HCI enable t…

astro-ph.IM2017★ 20 cited

An H-band Vector Vortex Coronagraph for the Subaru Coronagraphic Extreme-Adaptive Optics System

Jonas Kühn, Eugene Serabyn, Julien Lozi +11

The vector vortex is a coronagraphic imaging mode of the recently commissioned Subaru Coronagraphic Extreme-Adaptive Optics (SCExAO) platform on the 8-m Subaru Telescope. This mult…

astro-ph.IM2017★ 39 cited

A New Standard for Assessing the Performance of High Contrast Imaging Systems

Rebecca Jensen-Clem, Dimitri Mawet, Carlos A. Gomez Gonzalez +8

As planning for the next generation of high contrast imaging instruments (e.g. WFIRST, HabEx, and LUVOIR, TMT-PFI, EELT-EPICS) matures, and second-generation ground-based extreme a…

astro-ph.IM2017★ 22 cited

SPECULOOS exoplanet search and its prototype on TRAPPIST

Artem Burdanov, Laetitia Delrez, Michaël Gillon +1

One of the most significant goals of modern science is establishing whether life exists around other suns. The most direct path towards its achievement is the detection and atmosph…

astro-ph.IM2017★ 3 cited

Redshift determination through weighted phase correlation: a linearithmic implementation

L. Delchambre

We present a new algorithm having a time complexity of O(N log N) and designed to retrieve the phase at which an input signal and a set of not necessarily orthogonal templates matc…

astro-ph.IM2017★ 6 cited

K-shell photoabsorption and photoionization of trace elements. II. Isoelectronic sequences with electron number

C. Mendoza, M. A. Bautista, P. Palmeri +3

We are concerned with improving the diagnostic potential of the K lines and edges of elements with low cosmic abundances that are observed in the X-ray spectra of supernova remnant…