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A major goal of modern astrophysics is to understand the processes by which the universe evolved from its initial simplicity, as seen in measurements of the Cosmic Microwave Background, to the universe we see today, with complexity on all…

A convergence of ideas, observations and technology have led to the greatest period of cosmological discovery yet. Over the past three years we have determined the basic features of our Universe. We are now challenged to make sense of what…

Astrophysics · Physics 2007-05-23 Michael S. Turner

The James Webb Space Telescope (JWST), as the largest space-based astronomical observatory with near- and mid-infrared instrumentation, will elucidate many mysterious aspects of comets. We summarize four cometary science themes especially…

With the discovery of a high-energy neutrino flux in the 0.1 PeV to PeV range from beyond the Earth's atmosphere with the IceCube detector, neutrino astronomy has achieved a major breakthrough in the exploration of the high-energy universe.…

High Energy Astrophysical Phenomena · Physics 2019-08-13 A. Kappes

Neutrino astrophysics offers new perspectives on the Universe investigation: high energy neutrinos, produced by the most energetic phenomena in our Galaxy and in the Universe, carry complementary (if not exclusive) information about the…

High Energy Astrophysical Phenomena · Physics 2010-02-11 T. Chiarusi , M. Spurio

Over the last decades, observations with increasing quality have revolutionized our understanding of the general properties of the Universe. Questions posed for millenia by mankind about the origin, evolution and structure of the cosmos…

Cosmology and Nongalactic Astrophysics · Physics 2020-07-22 Ricardo T. Génova-Santos

Cosmological discoveries over the past century have completely changed our picture of our place in the universe. New observations have a realistic chance of probing nature on heretofore unimaginable scales, and as a result are changing the…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-18 Lawrence M. Krauss

Sky surveys represent a fundamental data basis for astronomy. We use them to map in a systematic way the universe and its constituents, and to discover new types of objects or phenomena. We review the subject, with an emphasis on the…

Instrumentation and Methods for Astrophysics · Physics 2015-05-20 S. G. Djorgovski , A. A. Mahabal , A. J. Drake , M. J. Graham , C. Donalek

Recent advances in astronomical observations have ushered in an era of remarkable discoveries. We now probe the Universe through multi-messenger signals, image the sky with unprecedented depth and resolution, and investigate individual…

Instrumentation and Methods for Astrophysics · Physics 2026-05-12 Zheng Cai , Song Huang , Yu Liu , Cheng Zhao , Lei Huang

Small satellite platforms with high performance avionics are becoming more affordable. So far, with a few exceptions, small satellites have been mainly dedicated to earth observation. However, astronomy is a fascinating field with a history…

Instrumentation and Methods for Astrophysics · Physics 2020-06-29 Pol Ribes-Pleguezuelo , Fanny Keller , Matteo Taccola

The advent of the Spitzer Space Telescope has revolutionized our understanding of the history of star formation and galaxy mass assembly in the Universe. The tremendous leap in sensitivity from previous mid-to-far IR missions has allowed…

Cosmology and Nongalactic Astrophysics · Physics 2009-05-08 Isaac Roseboom , Seb Oliver , Duncan Farrah , Mark Frost

Neutrino telescopes provide a unique observational gateway to the high-energy universe, enabling the study of cosmic accelerators and extreme environments that remain inaccessible to the other high-energy messengers. Although they share…

High Energy Astrophysical Phenomena · Physics 2026-03-24 Aya Ishihara

The discovery of cosmic acceleration is one of the most important developments in modern cosmology. The observation, thirteen years ago, that type Ia supernovae appear dimmer that they would have been in a decelerating universe followed by…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-04 Pierre Astier , Reynald Pain

Since its inception six decades ago, astrobiology has diversified immensely to encompass several scientific questions including the origin and evolution of Terran life, the organic chemical composition of extraterrestrial objects, and the…

Magnetic field is ubiquitous in the Universe and it plays essential roles in various astrophysical phenomena, yet its real origin and evolution are poorly known. This article reviews current understanding of magnetic fields in the…

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

Radio astronomy provides a unique window on the universe, allowing us to study: non-thermal processes (galactic nuclei, quasars, pulsars) at the highest angular resolution using VLBI, with low opacity. It is the most interesting wave band…

Astrophysics · Physics 2007-05-23 R D Ekers , J F Bell

This is the report of the Ultraviolet-Optical Working Group (UVOWG) commissioned by NASA to study the scientific rationale for new missions in ultraviolet/optical space astronomy approximately ten years from now, when the Hubble Space…

Doing astronomy with photons of energies in excess of a GeV has turned out to be extremely challenging. Efforts are underway to develop instruments that may push astronomy to wavelengths smaller than $10^{-14}$~cm by mapping the sky in high…

High Energy Physics - Phenomenology · Physics 2009-10-28 F. Halzen

The advanced interferometer network will herald a new era in observational astronomy. There is a very strong science case to go beyond the advanced detector network and build detectors that operate in a frequency range from 1 Hz-10 kHz,…

General Relativity and Quantum Cosmology · Physics 2012-06-05 B. Sathyaprakash , M. Abernathy , F. Acernese , P. Ajith , B. Allen , P. Amaro-Seoane , N. Andersson , S. Aoudia , K. Arun , P. Astone , B. Krishnan , L. Barack , F. Barone , B. Barr , M. Barsuglia , M. Bassan , R. Bassiri , M. Beker , N. Beveridge , M. Bizouard , C. Bond , S. Bose , L. Bosi , S. Braccini , C. Bradaschia , M. Britzger , F. Brueckner , T. Bulik , H. J. Bulten , O. Burmeister , E. Calloni , P. Campsie , L. Carbone , G. Cella , E. Chalkley , E. Chassande-Mottin , S. Chelkowski , A. Chincarini , A. Di. Cintio , J. Clark , E. Coccia , C. N. Colacino , J. Colas , A. Colla , A. Corsi , A. Cumming , L. Cunningham , E. Cuoco , S. Danilishin , K. Danzmann , E. Daw , R. De. Salvo , W. Del. Pozzo , T. Dent , R. De. Rosa , L. Di. Fiore , M. Di. Paolo. Emilio , A. Di. Virgilio , A. Dietz , M. Doets , J. Dueck , M. Edwards , V. Fafone , S. Fairhurst , P. Falferi , M. Favata , V. Ferrari , F. Ferrini , F. Fidecaro , R. Flaminio , J. Franc , F. Frasconi , A. Freise , D. Friedrich , P. Fulda , J. Gair , M. Galimberti , G. Gemme , E. Genin , A. Gennai , A. Giazotto , K. Glampedakis , S. Gossan , R. Gouaty , C. Graef , W. Graham , M. Granata , H. Grote , G. Guidi , J. Hallam , G. Hammond , M. Hannam , J. Harms , K. Haughian , I. Hawke , D. Heinert , M. Hendry , I. Heng , E. Hennes , S. Hild , J. Hough , D. Huet , S. Husa , S. Huttner , B. Iyer , D. I. Jones , G. Jones , I. Kamaretsos , C. Kant Mishra , F. Kawazoe , F. Khalili , B. Kley , K. Kokeyama , K. Kokkotas , S. Kroker , R. Kumar , K. Kuroda , B. Lagrange , N. Lastzka , T. G. F. Li , M. Lorenzini , G. Losurdo , H. Lück , E. Majorana , V. Malvezzi , I. Mandel , V. Mandic , S. Marka , F. Marin , F. Marion , J. Marque , I. Martin , D. Mc. Leod , D. Mckechan , M. Mehmet , C. Michel , Y. Minenkov , N. Morgado , A. Morgia , S. Mosca , L. Moscatelli , B. Mours , H. Müller-Ebhardt , P. Murray , L. Naticchioni , R. Nawrodt , J. Nelson , R. O'. Shaughnessy , C. D. Ott , C. Palomba , A. Paoli , G. Parguez , A. Pasqualetti , R. Passaquieti , D. Passuello , M. Perciballi , F. Piergiovanni , L. Pinard , M. Pitkin , W. Plastino , M. Plissi , R. Poggiani , P. Popolizio , E. Porter , M. Prato , G. Prodi , M. Punturo , P. Puppo , D. Rabeling , I. Racz , P. Rapagnani , V. Re , J. Read , T. Regimbau , H. Rehbein , S. Reid , F. Ricci , F. Richard , C. Robinson , A. Rocchi , R. Romano , S. Rowan , A. Rüdiger , A. Samblowski , L. Santamaría , B. Sassolas , R. Schilling , P. Schmidt , R. Schnabel , B. Schutz , C. Schwarz , J. Scott , P. Seidel , A. M. Sintes , K. Somiya , C. F. Sopuerta , B. Sorazu , F. Speirits , L. Storchi , K. Strain , S. Strigin , P. Sutton , S. Tarabrin , B. Taylor , A. Thürin , K. Tokmakov , M. Tonelli , H. Tournefier , R. Vaccarone , H. Vahlbruch , J. F. J. van. den. Brand , C. Van. Den. Broeck , S. van. der. Putten , M. van. Veggel , A. Vecchio , J. Veitch , F. Vetrano , A. Vicere , S. Vyatchanin , P. Weßels , B. Willke , W. Winkler , G. Woan , A. Woodcraft , K. Yamamoto
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