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ANTARES is a project aiming at the operation of an underwater detector at a depth of 2.5 km close to Toulon in the South of France. The detector is expected to be completed at the beginning of 2007. The main purpose of the experiment is the…

High Energy Physics - Experiment · Physics 2019-08-14 Teresa Montaruli

KM3NeT is a future research infrastructure in the Mediterranean Sea, hosting a multi-cubic-kilometre neutrino telescope and nodes for Earth and Sea sciences. In this report we shortly summarise the genesis of the KM3NeT project and present…

High Energy Astrophysical Phenomena · Physics 2019-08-14 Ulrich F. Katz

We present a short review of GRB studies performed for many years by Ioffe Institute experiments onboard a number of space missions. The first breakthrough in the studies of GRB was made possible by four Konus experiments carried out by the…

High Energy Astrophysical Phenomena · Physics 2012-06-26 R. L. Aptekar , S. V. Golenetskii , D. D. Frederiks , E. P. Mazets , V. D. Palshin

The ANTARES project aims to build a deep underwater Cherenkov neutrino telescope in the Mediterranean Sea. Currently the experiment is in the construction phase and has recently achieved two important milestones. The electro-optical cable…

Astrophysics · Physics 2019-08-14 I. Sokalski

In this paper we present an overview of the Telescope designed for ESA's mission dedicated to map the Cosmic Microwave Background Anisotropies and Polarization. Two instruments, LFI and HFI, operate in an overall frequency range between 25…

We present the distance priors from the finally released $Planck~ \textrm{TT,TE,EE}+\textrm{lowE}$ data in 2018. The uncertainties are around $40\%$ smaller than those from $Planck$ 2015 TT$+$lowP. In order to check the validity of these…

Cosmology and Nongalactic Astrophysics · Physics 2019-02-27 Lu Chen , Qing-Guo Huang , Ke Wang

An extremely sensitive all-sky survey will be carried out in the millimetre/submillimetre waveband by the forthcoming ESA mission Planck Surveyor. The main scientific goal of the mission is to make very accurate measurements of the spatial…

Astrophysics · Physics 2009-10-30 Andrew W. Blain

High altitude scientific balloons offer unique opportunities to carry scientific payloads to stratospheric altitudes at a cost several orders of magnitude lower than corresponding satellite missions. Balloon-borne payloads are easy to…

Instrumentation and Methods for Astrophysics · Physics 2021-03-23 D. Anand , B. Suneel Kumar , Devendra Ojha

The Atomic Clocks Ensemble in Space (ACES/PHARAO mission), which will be installed on board the International Space Station (ISS), uses a dedicated two-way Micro-Wave Link (MWL) in order to compare the timescale generated on board with…

Space Physics · Physics 2012-06-28 P. Delva , F. Meynadier , P. Wolf , C. Le Poncin-Lafitte , P. Laurent

Starting from 1960s, a great number of missions and experiments have been performed for the study of the high--energy sky. This review gives a wide vision of the most important space missions and balloon experiments that have operated in…

Instrumentation and Methods for Astrophysics · Physics 2019-05-06 Erica Cavallari , Filippo Frontera

EUSO-Balloon is a pathfinder mission for the Extreme Universe Space Observatory onboard the Japanese Experiment Module (JEM-EUSO). It was launched on the moonless night of the 25$^{th}$ of August 2014 from Timmins, Canada. The flight ended…

Instrumentation and Methods for Astrophysics · Physics 2018-08-09 G. Abdellaoui , S. Abe , J. H. Adams , A. Ahriche , D. Allard , L. Allen , G. Alonso , L. Anchordoqui , A. Anzalone , Y. Arai , K. Asano , R. Attallah , H. Attoui , M. Ave Pernas , S. Bacholle , M. Bakiri , P. Baragatti , P. Barrillon , S. Bartocci , J. Bayer , B. Beldjilali , T. Belenguer , N. Belkhalfa , R. Bellotti , A. Belov , K. Belov , K. Benmessai , M. Bertaina , P. L. Biermann , S. Biktemerova , F. Bisconti , N. Blanc , J. Błȩcki , S. Blin-Bondil , P. Bobik , M. Bogomilov , E. Bozzo , A. Bruno , K. S. Caballero , F. Cafagna , D. Campana , J-N. Capdevielle , F. Capel , A. Caramete , L. Caramete , P. Carlson , R. Caruso , M. Casolino , C. Cassardo , A. Castellina , C. Catalano O. Catalano , A. Cellino , M. Chikawa , G. Chiritoi , M. J. Christl , V. Connaughton , L. Conti , G. Cordero , G. Cotto , H. J. Crawford , R. Cremonini , S. Csorna , A. Cummings , S. Dagoret-Campagne , C. De Donato , C. de la Taille , C. De Santis , L. del Peral , M. Di Martino , A. Diaz Damian , T. Djemil , I. Dutan , A. Ebersoldt , T. Ebisuzaki , R. Engel , J. Eser , F. Fenu , S. Fernández-González , J. Fernández-Soriano , S. Ferrarese , M. Flamini , C. Fornaro , M. Fouka , A. Franceschi , S. Franchini , C. Fuglesang , T. Fujii , J. Fujimoto , M. Fukushima , P. Galeotti , E. García-Ortega , G. Garipov , E. Gascón , J. Genci , G. Giraudo , C. González Alvarado , P. Gorodetzky , R. Greg , F. Guarino , A. Guzmán , Y. Hachisu , M. Haiduc , B. Harlov , A. Haungs , J. Hernández Carretero , W. Hidber Cruz , D. Ikeda , N. Inoue , S. Inoue , F. Isgrò , Y. Itow , T. Jammer , S. Jeong , E. Joven , E. G. Judd , A. Jung , J. Jochum , F. Kajino , T. Kajino , S. Kalli , I. Kaneko , Y. Karadzhov , J. Karczmarczyk , K. Katahira , K. Kawai , Y. Kawasaki , A. Kedadra , H. Khales , B. A. Khrenov , Jeong-Sook Kim , Soon-Wook Kim , M. Kleifges , P. A. Klimov , D. Kolev , H. Krantz , I. Kreykenbohm , K. Kudela , Y. Kurihara , A. Kusenko , E. Kuznetsov , A. La Barbera , C. Lachaud , H. Lahmar , F. Lakhdari , R. Larson , O. Larsson , J. Lee , J. Licandro , L. López Campano , M. C. Maccarone , S. Mackovjak , M. Mahdi , D. Maravilla , L. Marcelli , J. L. Marcos , A. Marini , W. Marszał , K. Martens , Y. Martín , O. Martinez , M. Martucci , G. Masciantonio , K. Mase , M. Mastafa , R. Matev , J. N. Matthews , N. Mebarki , G. Medina-Tanco , M. A. Mendoza , A. Menshikov , A. Merino , J. Meseguer , S. S. Meyer , J. Mimouni , H. Miyamoto , Y. Mizumoto , A. Monaco , J. A. Morales de los Ríos , C. Moretto S. Nagataki , S. Naitamor , T. Napolitano , W. Naslund , R. Nava , A. Neronov , K. Nomoto , T. Nonaka , T. Ogawa , S. Ogio , H. Ohmori , A. V. Olinto , P. Orleański , G. Osteria , A. Pagliaro , W. Painter , M. I. Panasyuk , B. Panico , G. Pasqualino , E. Parizot , I. H. Park , B. Pastircak , T. Patzak , T. Paul , I. Pérez-Grande , F. Perfetto , T. Peter , P. Picozza , S. Pindado , L. W. Piotrowski , S. Piraino , L. Placidi , Z. Plebaniak , S. Pliego , A. Pollini , Z. Polonski , E. M. Popescu , P. Prat , G. Prévôt , H. Prieto , G. Puehlhofer , M. Putis , J. Rabanal , A. A. Radu , M. Reyes , M. Rezazadeh , M. Ricci , M. D. Rodríguez Frías , M. Rodencal , F. Ronga , G. Roudil , I. Rusinov , M. Rybczyński , M. D. Sabau , G. Sáez Cano , H. Sagawa , Z. Sahnoune , A. Saito , N. Sakaki , H. Salazar , J. C. Sanchez Balanzar , J. L. Sánchez , A. Santangelo , A. Sanz-Andrés , M. Sanz Palomino , O. Saprykin , F. Sarazin , M. Sato , T. Schanz , H. Schieler , V. Scotti , S. Selmane , D. Semikoz , M. Serra , S. Sharakin , H. M. Shimizu , K. Shinozaki , T. Shirahama , B. Spataro , I. Stan , T. Sugiyama , D. Supanitsky , M. Suzuki , B. Szabelska , J. Szabelski , N. Tajima , T. Tajima , Y. Takahashi , H. Takami , M. Takeda , Y. Takizawa , M. C. Talai , C. Tenzer , S. B. Thomas , O. Tibolla , L. Tkachev , H. Tokuno , T. Tomida , N. Tone , S. Toscano , M. Traïche , R. Tsenov , Y. Tsunesada , K. Tsuno , J. Tubbs , S. Turriziani , Y. Uchihori , O. Vaduvescu , J. F. Valdés-Galicia , P. Vallania , G. Vankova , C. Vigorito , L. Villaseñor , B. Vlcek , P. von Ballmoos , M. Vrabel , S. Wada , J. Watanabe , J. Watts , M. Weber , R. Weigand Muñoz , A. Weindl , L. Wiencke , M. Wille , J. Wilms , Z. Włodarczyk , T. Yamamoto , J. Yang , H. Yano , I. V. Yashin , D. Yonetoku , S. Yoshida , R. Young , I. S Zgura , M. Yu. Zotov , A. Zuccaro Marchi

We use model selection forecasting to assess the ability of the Planck satellite to make a positive detection of spectral index running. We simulate Planck data for a range of assumed cosmological parameter values, and carry out a three-way…

Astrophysics · Physics 2008-11-26 Cédric Pahud , Andrew R. Liddle , Pia Mukherjee , David Parkinson

The emergence of the ISR project at CERN is described in the light of the situation at CERN at the end of the 1950s when the CERN Proton Synchrotron (PS) was still under construction. The discussions leading to the project are put into…

Accelerator Physics · Physics 2012-06-19 Kurt Hubner

Hipparcos, the first ever experiment of global astrometry, was launched by ESA in 1989 and its results published in 1997 (Perryman et al., Astron. Astrophys. 323, L49, 1997; Perryman & ESA (eds), The Hipparcos and Tycho catalogues, ESA…

Instrumentation and Methods for Astrophysics · Physics 2015-06-04 Catherine Turon , Xavier Luri , Eduard Masana

Radio pulsars have been responsible for many astonishing astrophysical and fundamental physics breakthroughs since their discovery 50 years ago. In this review I will discuss many of the highlights, most of which were only possible because…

Instrumentation and Methods for Astrophysics · Physics 2018-08-22 Matthew Bailes

PICARD is a CNES micro-satellite launched in June 2010 (Thuillier at al. 2006). Its main goal is to measure the solar shape, total and spectral irradiance during the ascending phase of the activity cycle. The SODISM telescope onboard PICARD…

The scientific success of the SVOM mission will rely on the rapid transmission of alert messages from the satellite to the scientific community, and in particular to the ground-based instruments supporting the mission. In this paper, we…

Instrumentation and Methods for Astrophysics · Physics 2026-04-28 B. Cordier , L. Jeannin , Ph. Lafabrie , G. Chavanas , S. Crepaldi , N. Dagoneau , A. Formica , V. Garcia , L. Jolivet , S. Lacour , H. Louvin , E. Sabatier

Pluto's first known moon, Charon, was discovered in 1978 (Christy 1978) and has a diameter about half that of Pluto (Buie 1992,Young 1994, Sicardy 2005), which makes it larger relative to its primary than any other moon in the Solar System.…

A pulsar timing system has been operating in the 18-cm band at the Urumqi Astronomical Observatory 25-m telescope since mid-1999. Frequency resolution allowing dedispersion of the pulsar signals is provided by a 2X128X2.5 MHz…

Astrophysics · Physics 2009-11-07 N. Wang , R. N. Manchester , J. Zhang , X. J. Wu , A. Yusup , A. G. Lyne , K. S. Cheng , M. Z. Chen

We show that results from the Planck satellite reported in 2013 are consistent with the simplest cyclic models for natural parameter ranges i.e., order unity dimensionless coefficients, assuming the standard entropic mechanism for…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-15 Jean-Luc Lehners , Paul J. Steinhardt