output
19922026
most citedSciPy 1.0--Fundamental Algorithms for Scientific Computing in Python

40.2k citations

Showing 2017 · astro-ph.IMShow all

23 papers · 2 filters

astro-ph.IM2017★ 68 cited

Deep learning Approach for Classifying, Detecting and Predicting Photometric Redshifts of Quasars in the Sloan Digital Sky Survey Stripe 82

Johanna Pasquet-Itam, Jérôme Pasquet

We apply a convolutional neural network (CNN) to classify and detect quasars in the Sloan Digital Sky Survey Stripe 82 and also to predict the photometric redshifts of quasars. The…

astro-ph.IM2017★ 12 cited

The NIKA2 instrument at 30-m IRAM telescope: performance and results

A. Catalano, R. Adam, P. A. R. Ade +84

The New IRAM KID Arrays 2 (NIKA2) consortium has just finished installing and commissioning a millimetre camera on the IRAM 30 m telescope. It is a dual-band camera operating with…

astro-ph.IM2017★ 4 cited

Capabilities of ACAD-OSM, an active method for the correction of aperture discontinuities

Johan Mazoyer, Laurent Pueyo, Mamadou N'Diaye +4

The increasing complexity of the aperture geometry of the future space- and ground based-telescopes will limit the performance of the next generation of coronagraphic instruments f…

astro-ph.IM2017★ 12 cited

A fast, wide-field and distortion-free telescope with curved detectors for surveys at ultra-low surface brightness

Eduard Muslimov, David Valls-Gabaud, Gérard Lemaître +6

We present the design of an all-reflective, bi-folded Schmidt telescope aimed at surveys of extended astronomical objects with extremely-low surface brightness. The design leads to…

astro-ph.IM2017★ 6 cited

Deformable mirror interferometric analysis for the direct imagery of exoplanets

Johan Mazoyer, Raphaël Galicher, Pierre Baudoz +3

Direct imaging of exoplanet systems requires the use of coronagraphs to reach high contrast levels (10^-8 to 10^-11) at small angular separations (0.1"). However, the performance o…

astro-ph.IM2017★ 23 cited

Performance of the extreme-AO instrument VLT/SPHERE and dependence on the atmospheric conditions

J. Milli, D. Mouillet, T. Fusco +10

SPHERE is the high-contrast exoplanet imager and spectrograph installed at the Unit Telescope 3 of the Very Large Telescope. After more than two years of regular operations, we ana…

astro-ph.IM2017★ 10 cited

Optimal correction of distortion for High Angular Resolution images. Application to GeMS data

A. Bernard, B. Neichel, L. M. Mugnier +1

Whether is ground-based or space-based, any optical instrument suffers from some amount of optical geometric distortion. Recently, the diffraction-limited image quality afforded by…

astro-ph.IM2017★ 21 cited

Active correction of aperture discontinuities - optimized stroke minimization I: a new adaptive interaction matrix algorithm

J. Mazoyer, L. Pueyo, M. N'Diaye +7

Future searches for biomarkers on habitable exoplanets will rely on telescope instruments that achieve extremely high contrast at small planet-to-star angular separations. Coronagr…

astro-ph.IM2017★ 3 cited

CFHQSIR: a Y-band extension of the CFHTLS-Wide survey

S. Pipien, S. Basa, J. -G. Cuby +6

The Canada-France-Hawaii Telescope Legacy Survey (CFHTLS) has been conducted over a five-year period at the CFHT with the MegaCam instrument, totaling 450 nights of observations. T…

astro-ph.IM2017★ 27 cited

Data Acquisition Architecture and Online Processing System for the HAWC gamma-ray observatory

HAWC collaboration, A. U. Abeysekara, R. Alfaro +105

The High Altitude Water Cherenkov observatory (HAWC) is an air shower array devised for TeV gamma-ray astronomy. HAWC is located at an altitude of 4100 m a.s.l. in Sierra Negra, Me…

astro-ph.IM2017★ 10 cited

SCALA: In-situ calibration for Integral Field Spectrographs

S. Lombardo, D. Küsters, M. Kowalski +39

The scientific yield of current and future optical surveys is increasingly limited by systematic uncertainties in the flux calibration. This is the case for Type Ia supernova (SN I…

astro-ph.IM2017★ 35 cited

Disproval of the validated planets K2-78b, K2-82b, and K2-92b

J. Cabrera, S. C. C. Barros, D. Armstrong +13

Transiting super-Earths orbiting bright stars in short orbital periods are interesting targets for the study of planetary atmospheres. While selecting super-Earths suitable for fur…

astro-ph.IM2017★ 16 cited

Quantifying telescope phase discontinuities external to AO-systems by use of Phase Diversity and Focal Plane Sharpening

Masen Lamb, Carlos Correia, Jean-Francois Sauvage +7

We propose and apply two methods to estimate pupil plane phase discontinuities for two realistic scenarios on VLT and Keck. The methods use both Phase Diversity and a form of image…

astro-ph.IM2017★ 160 cited

The NIKA2 large field-of-view millimeter continuum camera for the 30-m IRAM telescope

Remi Adam, Amar Adane, P. A. R. Ade +45

Millimeter-wave continuum astronomy is today an indispensable tool for both general Astrophysics studies and Cosmology. General purpose, large field-of-view instruments are needed…

astro-ph.IM2017★ 124 cited

Exploring Cosmic Origins with CORE: Survey requirements and mission design

J. Delabrouille, P. de Bernardis, F. R. Bouchet +200

Future observations of cosmic microwave background (CMB) polarisation have the potential to answer some of the most fundamental questions of modern physics and cosmology. In this p…

astro-ph.IM2017★ 6 cited

Automated reliability assessment for spectroscopic redshift measurements

S. Jamal, V. Le Brun, O. Le Fèvre +7

We present a new approach to automate the spectroscopic redshift reliability assessment based on machine learning (ML) and characteristics of the redshift probability density funct…

astro-ph.IM2017★ 32 cited

An Application of Multi-band Forced Photometry to One Square Degree of SERVS: Accurate Photometric Redshifts and Implications for Future Science

Kristina Nyland, Mark Lacy, Anna Sajina +7

We apply The Tractor image modeling code to improve upon existing multi-band photometry for the Spitzer Extragalactic Representative Volume Survey (SERVS). SERVS consists of post-c…

astro-ph.IM2017★ 3 cited

Advanced modelling of a moderate-resolution holographic spectrograph

Eduard Muslimov, Gennady Valyavin, Sergei Fabrika +1

In the present article we consider an accurate modeling of spectrograph with cascade of volume-phase holographic gratings. The proposed optical scheme allows to detect spectra in a…

astro-ph.IM2017★ 84 cited

Deep Convolutional Neural Networks as strong gravitational lens detectors

C. Schaefer, M. Geiger, T. Kuntzer +1

Future large-scale surveys with high resolution imaging will provide us with a few new strong galaxy-scale lenses. These strong lensing systems however will be contained in…

astro-ph.IM2017★ 36 cited

Fine cophasing of segmented aperture telescopes with ZELDA, a Zernike wavefront sensor in the diffraction-limited regime

Pierre Janin-Potiron, Mamadou N'Diaye, Patrice Martinez +3

Segmented aperture telescopes require an alignment procedure with successive steps from coarse alignment to monitoring process in order to provide very high optical quality images…

astro-ph.IM2017★ 1.1k cited

The Hyper Suprime-Cam SSP Survey: Overview and Survey Design

H. Aihara, N. Arimoto, R. Armstrong +139

Hyper Suprime-Cam (HSC) is a wide-field imaging camera on the prime focus of the 8.2m Subaru telescope on the summit of Maunakea in Hawaii. A team of scientists from Japan, Taiwan…

astro-ph.IM2017★ 22 cited

An analytic expression for coronagraphic imaging through turbulence. Application to on-sky coronagraphic phase diversity

Olivier Herscovici-Schiller, Laurent M. Mugnier, Jean-François Sauvage

The ultimate performance of coronagraphic high contrast exoplanet imaging systems such as SPHERE or GPI is limited by quasi-static aberrations. These aberrations produce speckles t…

astro-ph.IM2017★ 9 cited

The Euclid Data Processing Challenges

Pierre Dubath, Nikolaos Apostolakos, Andrea Bonchi +37

Euclid is a Europe-led cosmology space mission dedicated to a visible and near infrared survey of the entire extra-galactic sky. Its purpose is to deepen our knowledge of the dark…