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The KM3NeT Collaboration is currently constructing a multi-site high-energy neutrino telescope in the Mediterranean Sea consisting of matrices of pressure-resistant glass spheres, each holding a set of 31 small-area photomultipliers. The…

天体物理仪器与方法 · 物理学 2022-07-27 S. Aiello , A. Albert , M. Alshamsi , S. Alves Garre , Z. Aly , A. Ambrosone , F. Ameli , M. Andre , G. Androulakis , M. Anghinolfi , M. Anguita , M. Ardid , S. Ardid , J. Aublin , C. Bagatelas , B. Baret , S. Basegmez du Pree , M. Bendahman , F. Benfenati , E. Berbee , A. M. van den Berg , V. Bertine , S. Biagi , M. Boettcher , M. Bou Cabo , J. Boumaaza , M. Bouta , M. Bouwhuis , C. Bozza , H. Branza , R. Bruijn , J. Brunner , R. Bruno , E. Buis , R. Buompane , J. Busto , B. Caiffi , D. Calvo , S. Campion , A. Capone , V. Carretero , P. Castaldi , S. Celli , M. Chabab , N. Chau , A. Chena , S. Cherubini , V. Chiarella , T. Chiarusi , M. Circella , R. Cocimano , J. A. B. Coelho , A. Coleiro , M. Colomer Molla , R. Coniglione , P. Coyle , A. Creusot , A. Cruza , G. Cuttone , R. Dalliera , B. De Martino , I. Di Palma , A. F. Diaz , D. Diego Tortosa , C. Distefano , A. Domi , C. Donzau , D. Dornic , M. Dorra , D. Drouhin , T. Eberla , A. Eddyamoui , T. van Eeden , D. van Eijk , I. El Bojaddaini , S. El Hedri , A. Enzenhofer , V. Espinosa , P. Fermani , G. Ferrara , M. D. Filipovic , F. Filippini , L. A. Fusco , T. Gala , J. Garcia Mendez , F. Garufi , Y. Gatelet , C. Gatius Oliver , N. Geisselbrecht , L. Gialanella , E. Giorgio , S. R. Gozzini , R. Gracia , K. Grafa , G. Grella , D. Guderian , C. Guidi , B. Guillon , M. Gutierrez , J. Haefner , S. Hallmann , H. Hamdaoui , H. van Harena , A. Heijboer , A. Hekaloa , L. Henniga , J. J. Hernandez-Rey , J. Hofestadt , F. Huang , W. Idrissi Ibnsalih , G. Illuminati , C. W. James , D. Janezashvili , M. de Jong , P. de Jong , B. J. Jung , P. Kalaczynski , O. Kalekin , U. F. Katz , N. R. Khan Chowdhury , G. Kistauri , F. van der Knaap , P. Kooijman , A. Kouchner , V. Kulikovskiy , M. Labalme , R. Lahmann , M. Lamoureux , G. Larosa , C. Lastori , A. Lazo , R. Le Breton , S. Le Stum , G. Lehaut , O. Leonardi , F. Leone , E. Leonora , N. Lessing , G. Levi , M. Lincetto , M. Lindsey Clark , T. Lipreau , C. LLorens Alvarez , F. Longhitano , D. Lopez-Coto , L. Maderer , J. Majumdar , J. Manczak , A. Margiotta , A. Marinelli , C. Markou , L. Martina , J. A. Martinez-Mora , A. Martini , F. Marzaioli , S. Mastroianni , K. W. Melis , G. Miele , P. Migliozzi , E. Migneco , P. Mijakowski , L. S. Miranda , C. M. Mollo , M. Moser , A. Moussa , R. Muller , M. Musumeci , L. Nauta , S. Navas , C. A. Nicolau , B. Nkosi , B. OFearraigh , M. OSullivan , M. Organokov , A. Orlando , J. Palacios Gonzalez , G. Papalashvilia , R. Papaleo , A. M. Paun , G. E. Pavala , C. Pellegrino , M. Perrin-Terrin , V. Pestel , P. Piattelli , C. Pieterse , O. Pisanti , C. Poire , V. Popa , T. Pradier , I. Probsta , S. Pulvirenti , G. Quemenera , N. Randazzo , S. Razzaquea , D. Real , S. Recka , G. Riccobene , A. Romanov , A. Rovelli , F. Salesa Greus , D. F. E. Samtlebe , A. Sanchez Losa , M. Sanguineti , D. Santonocito , P. Sapienza , J. Schnabel , M. F. Schneidera , J. Schumann , H. M. Schutte , J. Seneca , I. Sgura , R. Shanidze , A. Sharma , A. Sinopoulou , B. Spisso , M. Spurio , D. Stavropoulos , S. M. Stellaccian , M. Taiutik , Y. Tayalati , H. Thiersen , S. Tingay , S. Tsagkli , V. Tsourapis , E. Tzamariudaki , D. Tzanetatos , V. Van Elewyck , G. Vasileiadis , F. Versari , D. Vivolo , G. de Wasseige , J. Wilmsa , R. Wojaczynski , E. de Wolf , T. Yousfi , S. Zavatarelli , A. Zegarelli , D. Zito , J. D. Zornoza , J. Zuniga , N. Zywucka

The effect of satellite constellations on observations in the visible and IR domains is estimated, considering 18 constellations in development by SpaceX, Amazon, OneWeb, and others, with over 26,000 satellites, constituting a…

天体物理仪器与方法 · 物理学 2021-08-06 Olivier R. Hainaut , Adrew P. Williams

Astronomical observations in the X-ray band are subject to atmospheric attenuation and have to be performed in the space. CubeSats offer a cost effective means for space-based X-ray astrophysics but allow only limited mass and volume. In…

天体物理仪器与方法 · 物理学 2023-04-05 Hua Feng , Philip Kaaret

The number of satellites in low-Earth orbit is increasing rapidly, and many tens of thousands of them are expected to be launched in the coming years. There is a strong concern among the astronomical community about the contamination of…

天体物理仪器与方法 · 物理学 2022-01-19 C. G. Bassa , O. R. Hainaut , D. Galadi-Enriquez

We describe the design, performance and scientific objectives of the NASA-funded ALICE instrument aboard the ESA Rosetta asteroid flyby/comet rendezvous mission. ALICE is a lightweight, low-power, and low-cost imaging spectrograph optimized…

EAGLE is the multi-object, spatially-resolved, near-IR spectrograph instrument concept for the E-ELT, relying on a distributed Adaptive Optics, so-called Multi Object Adaptive Optics. This paper presents the results of a phase A study.…

The Euclid, Rubin/LSST and Roman (WFIRST) projects will undertake flagship optical/near-infrared surveys in the next decade. By mapping thousands of square degrees of sky and covering the electromagnetic spectrum between 0.3 and 2 microns…

A fleet of nanosatellites using precise timing synchronization provided by the Global Positioning System is a new concept for monitoring the gamma-ray sky that can achieve both all-sky coverage and good localization accuracy. We are…

The article is a short overview of a proposal of a CubeSat type nanosatellite designed to conduct biopharmaceutical tests on the low earth orbit. Motivations behind the emerging demand for such solution nowadays and in the close future are…

生物物理 · 物理学 2018-02-13 Anna Kornakiewicz , Jakub Mielczarek , Adam Zadrozny

New micro-satellite constellations enable unprecedented systematic monitoring applications thanks to their wide coverage and short revisit capabilities. However, the large volumes of images that they produce have uneven qualities, creating…

计算机视觉与模式识别 · 计算机科学 2019-04-22 Jérémy Anger , Carlo de Franchis , Gabriele Facciolo

The Wide-Field InfraRed Space Telescope (WFIRST) will be capable of delivering precise astrometry for faint sources over the enormous field of view of its main camera, the Wide-Field Imager (WFI). This unprecedented combination will be…

In preparation for James Webb Space Telescope (JWST), a set of cross calibration programs with HST and Spitzer for suitable primary photometric standards and astrometric fields were developed. NICMOS/HST and IRAC/Spitzer photometry…

天体物理学 · 物理学 2007-05-23 Rosa I. Diaz-Miller

Orbital monitoring of exoplanetary and stellar systems is fundamental for analysing their architecture, dynamical stability and evolution, and mechanisms of formation. Current high-contrast extreme-adaptive optics imagers like SPHERE, GPI,…

This paper presents initial flight results for distributed optical angles-only navigation of a swarm of small spacecraft, conducted during the Starling Formation-Flying Optical Experiment (StarFOX). StarFOX is a core payload of the NASA…

机器人学 · 计算机科学 2024-06-12 Justin Kruger , Soon S. Hwang , Simone D'Amico

GAIA astrometric mission of ESA will be very efficient in discovering binary and multiple stars with any orbital period, from minutes to millions of years. Main parameters of the revised mission design are presented. Next we estimate the…

天体物理学 · 物理学 2007-05-23 Tomaz Zwitter , Ulisse Munari

We present a coordinated campaign of observations to monitor the brightness of the James Webb Space Telescope (JWST) as it travels toward the second Earth-Sun Lagrange point and unfolds using the network ofUnistellar digital telescopes.…

The Balloon-borne Large Aperture Submillimeter Telescope (BLAST) is a sub-orbital experiment designed to study the process of star formation in local galaxies (including the Milky Way) and in galaxies at cosmological distances. Using a 2-m…