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The Southern Wide-field Gamma-ray Observatory (SWGO) is an R&D project to plan and design the next observatory to detect gamma rays in the Southern hemisphere. The experiment, planned to be placed at an altitude greater than 4400 m, is…

High Energy Physics - Experiment · Physics 2023-09-12 Ruben Conceição

The scientific potential of a wide field-of-view, and very-high duty cycle, ground-based gamma-ray detector has been demonstrated by the current generation of instruments, such as HAWC and ARGO, and will be further extended in the Northern…

Instrumentation and Methods for Astrophysics · Physics 2021-03-31 Ulisses Barres de Almeida

The Southern Wide-field Gamma-ray Observatory (SWGO) is a proposed ground-based gamma-ray detector that will be located in the Southern Hemisphere and is currently in its design phase. In this contribution, we will outline the prospects for…

High Energy Astrophysical Phenomena · Physics 2022-05-11 R. López-Coto , A. Mitchell , E. O. Angüner , G. Giacinti

The Southern Wide-field Gamma-ray Observatory (SWGO) is a project by scientists and engineers from 14 countries and 78 institutions to design and build the first wide-field, ground-based gamma-ray observatory in the Southern Hemisphere,…

We describe plans for the development of the Southern Wide-field Gamma-ray Observatory (SWGO), a next-generation instrument with sensitivity to the very-high-energy (VHE) band to be constructed in the Southern Hemisphere. SWGO will provide…

The very-high-energy gamma-ray sky can be surveyed on a daily basis by particle-detector arrays at high (mountain) elevation. In the northern hemisphere the survey recently conducted by the HAWC gamma-ray observatory significantly enriched…

High Energy Astrophysical Phenomena · Physics 2019-08-26 Harm Schoorlemmer

We outline the science motivation for SGSO, the Southern Gamma-Ray Survey Observatory. SGSO will be a next-generation wide field-of-view gamma-ray survey instrument, sensitive to gamma-rays in the energy range from 100 GeV to hundreds of…

High Energy Astrophysical Phenomena · Physics 2019-02-25 A. Albert , R. Alfaro , H. Ashkar , C. Alvarez , J. Álvarez , J. C. Arteaga-Velázquez , H. A. Ayala Solares , R. Arceo , J. A. Bellido , S. BenZvi , T. Bretz , C. A. Brisbois , A. M. Brown , F. Brun , K. S. Caballero-Mora , A. Carosi , A. Carramiñana , S. Casanova , P. M. Chadwick , G. Cotter , S. Coutiño De León , P. Cristofari , S. Dasso , E. de la Fuente , B. L. Dingus , P. Desiati , F. de O. Salles , V. de Souza , D. Dorner , J. C. Díaz-Vélez , J. A. García-González , M. A. DuVernois , G. Di Sciascio , K. Engel , H. Fleischhack , N. Fraija , S. Funk , J-F. Glicenstein , J. Gonzalez , M. M. González , J. A. Goodman , J. P. Harding , A. Haungs , J. Hinton , B. Hona , D. Hoyos , P. Huentemeyer , A. Iriarte , A. Jardin-Blicq , V. Joshi , S. Kaufmann , K. Kawata , S. Kunwar , J. Lefaucheur , J. -P. Lenain , K. Link , R. López-Coto , V. Marandon , M. Mariotti , J. Martínez-Castro , H. Martínez-Huerta , M. Mostafá , A. Nayerhoda , L. Nellen , E. de Oña Wilhelmi , R. D. Parsons , B. Patricelli , A. Pichel , Q. Piel , E. Prandini , E. Pueschel , S. Procureur , A. Reisenegger , C. Rivière , J. Rodriguez , A. C. Rovero , G. Rowell , E. L. Ruiz-Velasco , A. Sandoval , M. Santander , T. Sako , T. K. Sako , K. Satalecka , H. Schoorlemmer , F. Schüssler , M. Seglar-Arroyo , A. J. Smith , S. Spencer , P. Surajbali , E. Tabachnick , A. M. Taylor , O. Tibolla , I. Torres , B. Vallage , A. Viana , J. J. Watson , T. Weisgarber , F. Werner , R. White , R. Wischnewski , R. Yang , A. Zepeda , H. Zhou

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…

High Energy Astrophysical Phenomena · Physics 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 Southern Wide-field Gamma-ray Observatory (SWGO) is an international collaboration working on realizing a next-generation observatory located in the Southern hemisphere, which offers a privileged view of our galactic center. We are…

The hybrid detection approach in astroparticle physics has been successfully employed in cosmic-ray experiments and is currently being explored by gamma-ray observatories like LHAASO. We present a study on the hybrid detection concept for…

The focus of this presentation is to go through some of the remarkable observations concerning gamma-ray cosmic accelerators and diffuse emissions. Additionally, I will cover the status of the new generation of gamma-ray groundbased…

High Energy Astrophysical Phenomena · Physics 2019-02-28 Teresa Montaruli

I provide a personal perspective on the future of the field of ground-based gamma-ray astronomy, on the occasion of the 2024 {\it Gamma} conference in Milan. I discuss some of the scientific motivations for new instrumentation and the major…

Instrumentation and Methods for Astrophysics · Physics 2025-12-19 Jim Hinton

The operation of the next generation of gamma-ray observatories will lead to a great advance in dark matter searches. In this paper, we use the hidden sectors hypothesis within the so-called secluded models to calculate the capabilities of…

High Energy Astrophysical Phenomena · Physics 2025-01-20 Micael Andrade , Juan Fagiani , Clarissa Siqueira , Vitor de Souza , Aion Viana

In recent years, ground-based gamma-ray observatories have made a number of important astrophysical discoveries which have attracted the attention of the wider scientific community. The Division of Astrophysics of the American Physical…

Several projects planned or proposed can significantly expand our knowledge of the high-energy Universe in gamma rays. Construction of the Cherenkov telescope array CTA is started, and other detectors are planned which will use the…

Instrumentation and Methods for Astrophysics · Physics 2016-10-27 Alesandro De Angelis

The World Space Observatory is an unconventional space project proceeding via distributed studies. The present design, verified for feasibilty, consists of a 1.7-meter telescope operating at the second Largangian point of the Earth-Sun…

This paper reports on the current status of the World Space Observatory WSO-UV, a space mission for UV astronomy, planned for launch at the beginning of next decade. It is based on a 1.7 m telescope, with focal plane instruments including…

Gamma-ray astronomy holds a great potential for Astrophysics, Particle Physics and Cosmology. The CTA is an inter- national initiative to build the next generation of ground-based gamma-ray observatories, which will represent a factor of…

Instrumentation and Methods for Astrophysics · Physics 2019-08-14 Ulisses Barres de Almeida

The Cherenkov Telescope Array (CTA) is the major ground-based gamma-ray observatory planned for the next decade and beyond. Consisting of two large atmospheric Cherenkov telescope arrays (one in the southern hemisphere and one in the…

High Energy Astrophysical Phenomena · Physics 2019-06-12 The CTA Consortium , represented by Rene A. Ong
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