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With the advent of the Large Array Telescope (LAT) on board the Fermi satellite, a new window on the Universe has been opened. Publicly available, the Fermi-LAT data come together with an analysis software named ScienceTools (ST,…

Instrumentation and Methods for Astrophysics · Physics 2013-07-19 D. A. Sanchez , C. Deil

The AGILE satellite, in orbit since 2007, localized up to October 2009 about 1 Gamma Ray Burst (GRB) per month with the hard X-ray imager SuperAGILE (18 - 60 keV) (with a rate reduced by a factor 2-3 in spinning mode) and is detecting…

High Energy Astrophysical Phenomena · Physics 2019-08-13 F. Longo , G. Barbiellini , E. Del Monte , M. Marisaldi , F. Fuschino , A. Giuliani

The Advanced GAmma Tracking Array (AGATA) is a European project to develop and operate the next generation gamma-ray spectrometer. AGATA is based on the technique of gamma-ray energy tracking in electrically segmented high-purity germanium…

Instrumentation and Detectors · Physics 2012-09-18 S. Akkoyun , A. Algora , B. Alikhani , F. Ameil , G. de Angelis , L. Arnold , A. Astier , A. Ataç , Y. Aubert , C. Aufranc , A. Austin , S. Aydin , F. Azaiez , S. Badoer , D. L. Balabanski , D. Barrientos , G. Baulieu , R. Baumann , D. Bazzacco , F. A. Beck , T. Beck , P. Bednarczyk , M. Bellato , M. A. Bentley , G. Benzoni , R. Berthier , L. Berti , R. Beunard , G. Lo Bianco , B. Birkenbach , P. G. Bizzeti , A. M. Bizzeti-Sona , F. Le Blanc , J. M. Blasco , N. Blasi , D. Bloor , C. Boiano , M. Borsato , D. Bortolato , A. J. Boston , H. C. Boston , P. Bourgault , P. Boutachkov , A. Bouty , A. Bracco , S. Brambilla , I. P. Brawn , A. Brondi , S. Broussard , B. Bruyneel , D. Bucurescu , I. Burrows , A. Bürger , S. Cabaret , B. Cahan , E. Calore , F. Camera , A. Capsoni , F. Carrió , G. Casati , M. Castoldi , B. Cederwall , J. -L. Cercus , V. Chambert , M. El Chambit , R. Chapman , L. Charles , J. Chavas , E. Clément , P. Cocconi , S. Coelli , P. J. Coleman-Smith , A. Colombo , S. Colosimo , C. Commeaux , D. Conventi , R. J. Cooper , A. Corsi , A. Cortesi , L. Costa , F. C. L. Crespi , J. R. Cresswell , D. M. Cullen , D. Curien , A. Czermak , D. Delbourg , R. Depalo , T. Descombes , P. Désesquelles , P. Detistov , C. Diarra , F. Didierjean , M. R. Dimmock , Q. T. Doan , C. Domingo-Pardo , M. Doncel , F. Dorangeville , N. Dosme , Y. Drouen , G. Duchêne , B. Dulny , J. Eberth , P. Edelbruck , J. Egea , T. Engert , M. N. Erduran , S. Ertürk , C. Fanin , S. Fantinel , E. Farnea , T. Faul , M. Filliger , F. Filmer , Ch. Finck , G. de France , A. Gadea , W. Gast , A. Geraci , J. Gerl , R. Gernhäuser , A. Giannatiempo , A. Giaz , L. Gibelin , A. Givechev , N. Goel , V. González , A. Gottardo , X. Grave , J. Grȩbosz , R. Griffiths , A. N. Grint , P. Gros , L. Guevara , M. Gulmini , A. Görgen , H. T. M. Ha , T. Habermann , L. J. Harkness , H. Harroch , K. Hauschild , C. He , A. Hernández-Prieto , B. Hervieu , H. Hess , T. Hüyük , E. Ince , R. Isocrate , G. Jaworski , A. Johnson , J. Jolie , P. Jones , B. Jonson , P. Joshi , D. S. Judson , A. Jungclaus , M. Kaci , N. Karkour , M. Karolak , A. Kaşkaş , M. Kebbiri , R. S. Kempley , A. Khaplanov , S. Klupp , M. Kogimtzis , I. Kojouharov , A. Korichi , W. Korten , Th. Kröll , R. Krücken , N. Kurz , B. Y. Ky , M. Labiche , X. Lafay , L. Lavergne , I. H. Lazarus , S. Leboutelier , F. Lefebvre , E. Legay , L. Legeard , F. Lelli , S. M. Lenzi , S. Leoni , A. Lermitage , D. Lersch , J. Leske , S. C. Letts , S. Lhenoret , R. M. Lieder , D. Linget , J. Ljungvall , A. Lopez-Martens , A. Lotodé , S. Lunardi , A. Maj , J. van der Marel , Y. Mariette , N. Marginean , R. Marginean , G. Maron , A. R. Mather , W. Mȩczyński , V. Mendéz , P. Medina , B. Melon , R. Menegazzo , D. Mengoni , E. Merchan , L. Mihailescu , C. Michelagnoli , J. Mierzejewski , L. Milechina , B. Million , K. Mitev , P. Molini , D. Montanari , S. Moon , F. Morbiducci , R. Moro , P. S. Morrall , O. Möller , A. Nannini , D. R. Napoli , L. Nelson , M. Nespolo , V. L. Ngo , M. Nicoletto , R. Nicolini , Y. Le Noa , P. J. Nolan , M. Norman , J. Nyberg , A. Obertelli , A. Olariu , R. Orlandi , D. C. Oxley , C. Özben , M. Ozille , C. Oziol , E. Pachoud , M. Palacz , J. Palin , J. Pancin , C. Parisel , P. Pariset , G. Pascovici , R. Peghin , L. Pellegri , A. Perego , S. Perrier , M. Petcu , P. Petkov , C. Petrache , E. Pierre , N. Pietralla , S. Pietri , M. Pignanelli , I. Piqueras , Z. Podolyak , P. Le Pouhalec , J. Pouthas , D. Pugnére , V. F. E. Pucknell , A. Pullia , B. Quintana , R. Raine , G. Rainovski , L. Ramina , G. Rampazzo , G. La Rana , M. Rebeschini , F. Recchia , N. Redon , M. Reese , P. Reiter , P. H. Regan , S. Riboldi , M. Richer , M. Rigato , S. Rigby , G. Ripamonti , A. P. Robinson , J. Robin , J. Roccaz , J. -A. Ropert , B. Rossé , C. Rossi Alvarez , D. Rosso , B. Rubio , D. Rudolph , F. Saillant , E. Şahin , F. Salomon , M. -D. Salsac , J. Salt , G. Salvato , J. Sampson , E. Sanchis , C. Santos , H. Schaffner , M. Schlarb , D. P. Scraggs , D. Seddon , M. Şenyiğit , M. -H. Sigward , G. Simpson , J. Simpson , M. Slee , J. F. Smith , P. Sona , B. Sowicki , P. Spolaore , C. Stahl , T. Stanios , E. Stefanova , O. Stézowski , J. Strachan , G. Suliman , P. -A. Söderström , J. L. Tain , S. Tanguy , S. Tashenov , Ch. Theisen , J. Thornhill , F. Tomasi , N. Toniolo , R. Touzery , B. Travers , A. Triossi , M. Tripon , K. M. M. Tun-Lanoë , M. Turcato , C. Unsworth , C. A. Ur , J. J. Valiente-Dobon , V. Vandone , E. Vardaci , R. Venturelli , F. Veronese , Ch. Veyssiere , E. Viscione , R. Wadsworth , P. M. Walker , N. Warr , C. Weber , D. Weisshaar , D. Wells , O. Wieland , A. Wiens , G. Wittwer , H. J. Wollersheim , F. Zocca , N. V. Zamfir , M. Ziȩbliński , A. Zucchiatti

Axions and axion-like particles (ALPs) are hypothetical particles that occur in extensions of the Standard Model and are candidates for cold dark matter. They could be detected through their oscillations into photons in the presence of…

High Energy Astrophysical Phenomena · Physics 2022-09-21 Manuel Meyer , James Davies , Julian Kuhlmann

We report the results of an extensive search in the AGILE data for a gamma-ray counterpart of the LIGO gravitational wave event GW150914. Currently in spinning mode, AGILE has the potential of covering with its gamma-ray instrument 80 % of…

The scientific goals of the AMIGA project are based on the analysis of a significant amount of spectroscopic 3D data. In order to perform this work we present an initiative to develop a new VO compliant package, including present core…

Instrumentation and Methods for Astrophysics · Physics 2009-01-21 J. E. Ruiz , J. D. Santander-Vela , V. Espigares , L. Verdes-Montenegro , J. M. van der Hulst

GPUs are critical for compute-intensive applications, yet emerging workloads such as recommender systems, graph analytics, and data analytics often exceed GPU memory capacity. Existing solutions allow GPUs to use CPU DRAM or SSDs as…

Distributed, Parallel, and Cluster Computing · Computer Science 2025-08-27 Zhuoping Yang , Jinming Zhuang , Xingzhen Chen , Alex K. Jones , Peipei Zhou

DIETER is an open-source power sector model designed to analyze future settings with very high shares of variable renewable energy sources. It minimizes overall system costs, including fixed and variable costs of various generation,…

Computers and Society · Computer Science 2021-09-23 Carlos Gaete-Morales , Martin Kittel , Alexander Roth , Wolf-Peter Schill

Explainable artificial intelligence (XAI) is an emerging new domain in which a set of processes and tools allow humans to better comprehend the decisions generated by black box models. However, most of the available XAI tools are often…

Machine Learning · Computer Science 2021-07-22 Zoumpolia Dikopoulou , Serafeim Moustakidis , Patrik Karlsson

During the first 3 years of operation the Gamma-Ray Imaging Detector onboard the AGILE satellite detected several blazars in a high gamma-ray activity: 3C 279, 3C 454.3, PKS 1510-089, S5 0716+714, 3C 273, W Comae, Mrk 421, PKS 0537-441 and…

We present ZodiPy, a modern and easy-to-use Python package for modeling the zodiacal emission seen by an arbitrary Solar System observer, which can be used for the removal of both thermal emission and scattered sunlight from interplanetary…

Earth and Planetary Astrophysics · Physics 2022-10-19 M. San , D. Herman , G. B. Erikstad , M. Galloway , D. Watts

ASTRA is a Python package that provides a modular, instrument-independent interface for working with high-resolution stellar spectra. Designed to support data from multiple spectrographs, including ESPRESSO (Pepe et al., 2021), HARPS (Mayor…

Instrumentation and Methods for Astrophysics · Physics 2026-01-16 André M. Silva , J. P. Faria , N. C. Santos , S. G. Sousa , P. T. P. Viana , J. H. C. Martins

Exploratory visual data analysis tools empower data analysts to efficiently and intuitively explore data insights throughout the entire analysis cycle. However, the gap between common programmatic analysis (e.g., within computational…

Human-Computer Interaction · Computer Science 2025-01-08 Yue Yu , Leixian Shen , Fei Long , Huamin Qu , Hao Chen

AOtools is a Python package which is open-source and aimed at providing tools for adaptive optics users and researchers. We present version 1.0 which contains tools for adaptive optics processing, including analysing data in the pupil…

Instrumentation and Methods for Astrophysics · Physics 2020-01-08 M. J. Townson , O. J. D. Farley , G. Orban de Xivry , J. Osborn , A. P. Reeves

In the multi-messenger era, astronomical projects share information about transients phenomena issuing science alerts to the Scientific Community through different communications networks. This coordination is mandatory to understand the…

Instrumentation and Methods for Astrophysics · Physics 2023-02-08 N. Parmiggiani , A. Bulgarelli , D. Beneventano , V. Fioretti , L. Baroncelli , A. Addis , M. Tavani

Raman spectroscopy is a non-destructive and label-free chemical analysis technique, which plays a key role in the analysis and discovery cycle of various branches of science. Nonetheless, progress in Raman spectroscopic analysis is still…

Spectropolarimetry, the observation of polarization and intensity as a function of wavelength, is a powerful tool in stellar astrophysics. It is particularly useful for characterizing stars and circumstellar material, and for tracing the…

During more than 17 years of operation in space INTEGRAL telescope has accumulated large data set that contains records of hard X-ray and soft gamma-ray astronomical sources. These data can be re-used in the context of multi-wavelength or…

Instrumentation and Methods for Astrophysics · Physics 2021-07-28 A. Neronov , V. Savchenko , A. Tramacere , M. Meharga , C. Ferrigno , S. Paltani
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