Alexander, Samuel Hibbard, Bill
Published in
Journal of Artificial General Intelligence
In 2011, Hibbard suggested an intelligence measure for agents who compete in an adversarial sequence prediction game. We argue that Hibbard’s idea should actually be considered as two separate ideas: first, that the intelligence of such agents can be measured based on the growth rates of the runtimes of the competitors that they defeat; and second,...
Thiébaut, Éric Tallon, Michel Thé, Samuel Denis, Loïc
The FRiM fractal operator belongs to a family of operators, called ASAP, defined by an ordered selection of nearest neighbors. This generalization provides means to improve upon the good properties of FRiM. We propose a fast algorithm to build an ASAP operator mimicking the fractal structure of FRiM for pupils of any size and geometry and to learn ...
Thiébaut, Éric Tallon, Michel Tallon-Bosc, Isabelle Gelly, Bernard Douet, Richard Langlois, Maud Moretto, Gil
We have taken advantage of the implementation of an adaptive optics system on the Themis solar telescope to implement innovative strategies based on an inverse problem formulation for the control loop. Such an approach encompassing the whole system implies the estimation of the pixel variances of the Shack-Hartmann wavefront sensor, a novel real-ti...
Aksoy, Nurbanu Ravikumar, Nishant Frangi, Alejandro F.
Medical image interpretation is central to most clinical applications such as disease diagnosis, treatment planning, and prognostication. In clinical practice, radiologists examine medical images (e.g. chest x-rays, computed tomography images, etc.) and manually compile their findings into reports, which can be a time-consuming process. Automated a...
Le Graët, J. Secroun, A. Barbier, R. Gillard, W. Clémens, J.-C. Conseil, S. Escoffier, S. Ferriol, S. Fourmanoit, N. Kajfasz, E.
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Euclid is a major ESA mission scheduled for launch in 2023-2024 to map the geometry of the dark Universe using two primary probes, weak gravitational lensing and galaxy clustering. Euclid’s instruments, a visible imager (VIS) and an infrared spectrometer and photometer (NISP) have both been designed and built by Euclid Consortium teams. The NISP in...
Zhu, Wenbo
With the rapid transformation of computer hardware and algorithms, mobile networking has evolved from low datacarrying capacity and high latency to better-optimized networks, either by enhancing the digital network or using different approaches to reduce network traffic. This paper discusses the big data applications and scheduling in the distribut...
Medinaceli, E. Valenziano, L. Auricchio, N. Franceschi, E. Gianotti, F. Battaglia, P. Farinelli, R. Balestra, A. Dusini, S. Sirignano, C.
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ESA’s mission Euclid while undertaking its final integration stage is fully qualified. Euclid will perform an extra galactic survey (0
Reynolds, Christopher S. Kara, Erin A. Mushotzky, Richard F. Ptak, Andrew Koss, Michael J. Williams, Brian J. Allen, Steven W. Bauer, Franz E. Bautz, Marshall Bogadhee, Arash
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The Advanced X-ray Imaging Satellite (AXIS) is a Probe-class concept that will build on the legacy of the Chandra x-ray Observatory by providing low-background, arcsecond-resolution in the 0.3-10 keV band across a 450 arcminute2 field of view, with an order of magnitude improvement in sensitivity. AXIS utilizes breakthroughs in the construction of ...
Lovis, Christophe Blind, Nicolas Chazelas, Bruno Kühn, Jonas G. Genolet, Ludovic Hughes, Ian Sordet, Michaël Schnell, Robin Turbet, Martin Fusco, Thierry
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RISTRETTO is a visible high-resolution spectrograph fed by an extreme adaptive optics (AO) system, to be proposed as a visitor instrument on ESO VLT. The main science goal of RISTRETTO is the detection and atmospheric characterisation of exoplanets in reflected light, in particular the temperate rocky planet Proxima b. RISTRETTO will be able to mea...
Bestha, Manjunath Hasan, Amirul Divakar, Devika Surya, Arun Sriram, S. Sivarani, T. Prakash, Ajin M., Parvathy Yadav, Sudharshan
Highly multiplexed spectroscopic surveys have changed the astronomy landscape in recent years. However, these surveys are limited to low and medium spectral resolution. High spectral resolution spectroscopy is often photon starved and will benefit from a large telescope aperture. Multiplexed high-resolution surveys require a wide field of view and ...