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We present here a new robotic telescope called TRAPPIST (TRAnsiting Planets and PlanetesImals Small Telescope). Equipped with a high-quality CCD camera mounted on a 0.6 meter light weight optical tube, TRAPPIST has been installed in April…

地球与行星天体物理 · 物理学 2015-05-27 M. Gillon , E. Jehin , P. Magain , V. Chantry , D. Hutsemekers , J. Manfroid , D. Queloz , S. Udry

As one of the options, the Cherenkov Telescope Array (CTA) Consortium is considering the possibility to install its Southern array in Chile, in the Atacama Desert. The envisaged site is situated about 5 km from the future European Extremely…

天体物理仪器与方法 · 物理学 2019-08-14 Markus Gaug , Michele Doro

The European Large Area ISO Survey (ELAIS) has surveyed 12 square degrees of the sky at 15 and 90 microns, and subsets of this area at 6.75 and 175 microns, using the Infrared Space Observatory (ISO). This project was the largest single…

We present some recent results from the European Large Area ISO Survey (ELAIS). This survey was the largest non-serendipitous ISO field survey. A preliminary reduction has recently been completed and catalogues of sources released to the…

Observatory end-to-end science operations is the overall process starting with a scientific question, represented by a proposal requesting observing time, and ending with the analysis of observation data addressing that question, and…

The Simons Observatory (SO) is a ground-based cosmic microwave background survey experiment that consists of three 0.5 m small-aperture telescopes and one 6 m large-aperture telescope, sited at an elevation of 5200 m in the Atacama Desert…

天体物理仪器与方法 · 物理学 2022-07-20 Lauren J. Saunders , Matthew Hasselfield , Brian J. Koopman , Laura Newburgh

The Simons Observatory (SO) is a cosmic microwave background (CMB) observatory consisting of three small aperture telescopes and one large aperture telescope. SO is located in the Atacama Desert in Chile at an elevation of 5180m.…

This overview article describes the legacy prospect and discovery potential of the Dark Energy Survey (DES) beyond cosmological studies, illustrating it with examples from the DES early data. DES is using a wide-field camera (DECam) on the…

宇宙学与河外天体物理 · 物理学 2016-11-18 Dark Energy Survey Collaboration , T. Abbott , F. B. Abdalla , J. Aleksic , S. Allam , A. Amara , D. Bacon , E. Balbinot , M. Banerji , K. Bechtol , A. Benoit-Levy , G. M. Bernstein , E. Bertin , J. Blazek , C. Bonnett , S. Bridle , D. Brooks , R. J. Brunner , E. Buckley-Geer , D. L. Burke , G. B. Caminha , D. Capozzi , J. Carlsen , A. Carnero-Rosell , M. Carollo , M. Carrasco-Kind , J. Carretero , F. J. Castander , L. Clerkin , T. Collett , C. Conselice , M. Crocce , C. E. Cunha , C. B. D'Andrea , L. N. da Costa , T. M. Davis , S. Desai , H. T. Diehl , J. P. Dietrich , S. Dodelson , P. Doel , A. Drlica-Wagner , J. Estrada , J. Etherington , A. E. Evrard , J. Fabbri , D. A. Finley , B. Flaugher , R. J. Foley , P. Rosalba , J. Frieman , J. Garcia-Bellido , E. Gaztanaga , D. W. Gerdes , T. Giannantonio , D. A. Goldstein , D. Gruen , R. A. Gruendl , P. Guarnieri , G. Gutierrez , W. Hartley , K. Honscheid , B. Jain , D. J. James , T. Jeltema , S. Jouvel , R. Kessler , A. King , D. Kirk , R. Kron , K. Kuehn , N. Kuropatkin , O. Lahav , T. S. Li , M. Lima , H. Lin , M. A. G. Maia , M. Makler , M. Manera , C. Maraston , J. L. Marshall , P. Martini , R. G. McMahon , P. Melchior , A. Merson , C. J. Miller , R. Miquel , J. J. Mohr , X. Morice-Atkinson , K. Naidoo , E. Neilsen , R. C. Nichol , B. Nord , R. Ogando , F. Ostrovski , A. Palmese , A. Papadopoulos , H. Peiris , J. Peoples , W. J. Percival , A. A. Plazas , S. L. Reed , A. Refregier , A. K. Romer , A. Roodman , A. Ross , E. Rozo , E. S. Rykoff , I. Sadeh , M. Sako , C. Sanchez , E. Sanchez , B. Santiago , V. Scarpine , M. Schubnell , I. Sevilla-Noarbe , E. Sheldon , M. Smith , R. C. Smith , M. Soares-Santos , F. Sobreira , M. Soumagnac , E. Suchyta , M. Sullivan , M. Swanson , G. Tarle , J. Thaler , D. Thomas , R. C. Thomas , D. Tucker , J. D. Vieira , V. Vikram , A. R. Walker , R. H. Wechsler , J. Weller , W. Wester , L. Whiteway , H. Wilcox , B. Yanny , Y. Zhang , J. Zuntz

The proposed next generation Event Horizon Telescope (ngEHT) concept envisions the imaging of various astronomical sources on scales of microarcseconds in unprecedented detail with at least two orders of magnitude improvement in the image…

天体物理仪器与方法 · 物理学 2022-12-20 Kazunori Akiyama , Jens Kauffmann , Lynn D. Matthews , Kotaro Moriyama , Shoko Koyama , Kazuhiro Hada

The EAGLE instrument is a Multi-Object Adaptive Optics (MOAO) fed, multiple Integral Field Spectrograph (IFS), working in the Near Infra-Red (NIR), on the European Extremely Large Telescope (E-ELT). A Phase A design study was delivered to…

Dedicated to spectroscopic and imaging observations of the ultraviolet sky, the World Space Observatory for Ultraviolet Project is a Russia led international collaboration presently involving also China, Germany, Italy, Spain and Ukraine.…

天体物理学 · 物理学 2020-08-05 I. Pagano , M. Sachkov , A. I. Gomez de Castro , M. Huang , N. Kappelmann , S. Scuderi , B. Shustov , K. Werner , G. Zhao

Ground-based gamma-ray astronomy is now well established as a key observational approach to address critical topics at the frontiers of astroparticle physics and high-energy astrophysics. Whilst the field of TeV astronomy was once dominated…

高能天体物理现象 · 物理学 2025-06-26 SWGO Collaboration , P. Abreu , R. Alfaro , A. Alfonso , M. Andrade , E. O. Angüner , E. A. Anita-Rangel , O. Aquines-Gutiérrez , C. Arcaro , R. Arceo , J. C. Arteaga-Velázquez , P. Assis , H. A. Ayala Solares , A. Bakalova , E. M. Bandeira , P. Bangale , U. Barres de Almeida , P. Batista , I. Batković , J. Bazo , E. Belmont , J. Bennemann , S. Y. BenZvi , A. Bernal , W. Bian , C. Bigongiari , E. Bottacini , R. Branada , P. Brogueira , A. M. Brown , T. Bulik , K. S. Caballero-Mora , P. Camarri , W. Cao , Z. Cao , Z. Cao , T. Capistrán , M. Cardillo , C. Casentini , C. Castromonte , P. M. Chadwick , J. Chanamé , J. Chang , S. Chen , A. Chiavassa , L. Chytka , R. Colalillo , R. Conceição , G. Consolati , R. Cordero , P. J. Costa , R. Covarelli , X. Cui , X. Cui , A. De Angelis , E. de Gouveia Dal Pino , R. de Menezes , P. Desiati , N. Di Lalla , F. Di Pierro , G. Di Sciascio , J. C. Díaz Vélez , C. Dib , B. Dingus , J. Djuvsland , C. Dobrigkeit , L. M. Domingues Mendes , T. Dorigo , M. Doro , A. C. dos Reis , M. Du Vernois , D. Elsaesser , K. Engel , T. Ergin , M. Errando , K. Fang , A. Fazzi , C. Feng , M. Feroci , C. N. Ferreira , N. Fraija , S. Fraija , A. Franceschini , G. F. Franco , S. Funk , R. Galleguillos , B. Gao , C. Gao , A. M. Garcia Reyes , S. Garcia , F. Garfias , G. Giacinti , L. Gibilisco , B. Giovanni , J. Glombitza , H. Goksu , G. Gong , B. S. González , M. M. González , J. Goodman , V. M. Grieco , M. Gu , F. Guarino , G. P. Guedes , J. Gyeong , F. Haist , G. Han , P. Hansen , J. P. Harding , S. Hernandez Cadena , I. Herzog , J. Hinton , W. Hofmann , C. Hou , Hou C. , K. Hu , D. Huang , P. Huentemeyer , A. Iriarte , J. Isaković , A. Jardin-Blicq , L. I. Junoy , J. Juryšek , S. Kaci , B. Khelifi , D. Kieda , F. La Monaca , G. La Mura , R. G. Lang , J. S. Lapington , R. Laspiur , L. Lavitola , J. Lee , F. Leitl , M. Lemoine-Goumard , L. Lessio , T. Lewis , C. Li , J. Li , K. Li , T. Li , B. Liberti , S. Lin , R. A. Lineros , D. Liu , J. Liu , R. Liu , F. Longo , Y. Luo , J. Lv , E. Macerata , G. Magugliani , K. Malone , A. Mancilla , D. Mandat , M. Manganaro , M. Mariani , A. Mariazzi , M. Mariotti , T. Marrodan , H. Martínez-Huerta , I. Martins , S. Medina , D. Melo , L. F. Mendes , E. Meza , R. Micali , D. Miceli , S. Miozzi , L. S. Miranda , P. E. Mirón Enriquez , A. Mitchell , A. Molinario , A. Montero , O. G. Morales-Olivares , A. Morselli , E. Mossini , M. Mostafá , F. Muleri , F. Nardi , A. P. Nayak , A. Negro , L. Nellen , M. Nisa , V. Novotny , L. Olivera-Nieto , N. Omodei , E. Orlando , S. Ortolani , M. Osorio-Archila , T. Ota , L. Otiniano , Z. Ou , A. Paoloni , I. M. Pepe , R. Perca , M. Peresano , Y. Pérez Araujo , T. Petrosillo-Lago , G. Piano , D. Piccolo , A. Pichel , M. Pimenta , M. Pirke , A. Porcelli , T. Porter , E. Prandini , A. Pratts , R. Pretsch , A. Qi , J. Qin , S. Rainò , L. Recabarren , M. Regeard , A. Reisenegger , Q. Remy , H. X. Ren , F. Rescic , B. Reville , M. Reyes , C. D. Rho , M. Riquelme , J. I. Rivadeneira , G. Rodriguez Fernandez , B. Rossi , A. C. Rovero , A. Ruina , E. Ruiz-Velasco , G. Salazar , C. Salotto , F. Sanchez , A. Sandoval , F. Sansone , M. Santander , R. Santonico , G. L. P. Santos , A. Santos-Guevara , D. Sartirana , M. Schneider , M. Schneider , H. Schoorlemmer , F. G. Schröder , F. Schussler , H. Schutte , J. Serna-Franco , M. Shoaib , A. Smith , A. J. Smith , Y. Son , O. Soto , S. T. Spencer , R. W. Springer , J. Stewart , L. A. Stuani , H. Sun , M. Tambone , R. Tang , Z. Tang , S. Tapia , M. Tavani , R. Terrier , T. Terzić , K. Tollefson , B. Tomé , I. Torres , R. Torres-Escobedo , G. C. Trinchero , R. Turner , P. Ulloa , L. Valore , C. van Eldik , J. Vega , I. D. Vergara Quispe , A. Viana , J. Vícha , C. F. Vigorito , V. Vittorini , B. Wang , L. Wang , X. Wang , X. Wang , X. Wang , Z. Wang , Z. Wang , M. Waqas , I. J. Watson , F. Werner , R. White , C. Wiebusch , F. Wohlleben , S. Xi , G. Xiao , H. Xiao , H. Xiao , L. Yang , R. Yang , Z. Yang , Z. Yang , R. Yanyachi , Z. Yao , D. Zavrtanik , H. Zhang , H. Zhang , J. Zhang , J. Zhang , S. Zhang , S. Zhang , X. Zhang , Y. Zhang , Y. Zhang , Y. Zhang , J. Zhao , L. Zhao , H. Zhou , C. Zhu , H. Zhu , H. Zhu , P. Zhu , X. Zuo , P. Zyla

The ESO Slice Project (ESP) is a galaxy redshift survey we have recently completed as an ESO Key-Project. The ESP covers 23.3 square degrees in a region close to the South Galactic Pole. The survey is nearly complete (85%) to the limiting…

Ground-based gamma-ray astronomy has experienced a major breakthrough in the last decade thanks to the advent of new generation instruments such as H.E.S.S., MAGIC, Milagro and VERITAS. A large variety of cosmic particle accelerators has…

高能天体物理现象 · 物理学 2011-10-11 Jürgen Knödlseder

(abridged) The Atacama Large Millimeter/submillimeter Array (ALMA) was the top-ranked priority for a new ground-based facility in the 2000 Canadian Long Range Plan. Ten years later, at the time of LRP2010, ALMA construction was well…

The Simons Observatory (SO) is a group of modern telescopes dedicated to observing the polarized cosmic microwave background (CMB), transients, and more. The Observatory consists of four telescopes and instruments, with over 60,000…

The Herschel ATLAS is the largest open-time key project that will be carried out on the Herschel Space Observatory. It will survey 510 square degrees of the extragalactic sky, four times larger than all the other Herschel surveys combined,…

In October 1997, the Italian and Dutch GRB teams started a collaboration on ESO optical follow-up of rapidly and accurately localized GRBs. Subsequently, starting April 1, 2000, this collaboration was extended to astronomers from other…

天体物理学 · 物理学 2007-05-23 Nicola Masetti