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Related papers: The ANTARES Astronomical Time-Domain Event Broker

200 papers

ANTARES is the largest high-energy neutrino telescope in the Northern Hemisphere. A search for neutrinos in coincidence with gamma-ray bursts using ANTARES data from late 2007 to 2011 is presented here. An extended maximum likelihood ratio…

High Energy Astrophysical Phenomena · Physics 2013-11-19 Julia Schmid

The Angstrom Project is undertaking an optical survey of stellar microlensing events across the bulge region of the Andromeda Galaxy (M31) using a distributed network of two-meter class telescopes. The Angstrom Project Alert System (APAS)…

Time-domain astronomy is entering an era of unprecedented discovery driven by wide-field, high-cadence surveys such as LSST, Roman, Euclid, SKA, and PLATO. While some of these facilities will generate enormous photometric alert streams, the…

This paper reports a search for spatial clustering of the arrival directions of high energy muon neutrinos detected by the ANTARES neutrino telescope. An improved two-point correlation method is used to study the autocorrelation of 3058…

High Energy Astrophysical Phenomena · Physics 2014-05-08 S. Adrián-Martínez , A. Albert , M. André , G. Anton , M. Ardid , J. -J. Aubert , B. Baret , J. Barrios-Martí , S. Basa , V. Bertin , S. Biagi , C. Bogazzi , R. Bormuth , M. Bou-Cabo , M. C. Bouwhuis , R. Bruijn , J. Brunner , J. Busto , A. Capone , L. Caramete , J. Carr , S. Cecchini , T. Chiarusi , M. Circella , R. Coniglione , L. Core , H. Costantini , P. Coyle , A. Creusot , C. Curtil , G. De Rosa , I. Dekeyser , A. Deschamps , G. De Bonis , C. Donzaud , D. Dornic , Q. Dorosti , D. Drouhin , A. Dumas , T. Eberl , D. Elsässer , A. Enzenhöfer , S. Escoffier , K. Fehn , I. Felis , P. Fermani , F. Folger , L. A. Fusco , S. Galatà , P. Gay , S. Geißelsöder , K. Geyer , V. Giordano , A. Gleixner , J. P. Gómez-González , K. Graf , G. Guillard , H. van Haren , A. J. Heijboer , Y. Hello , J. J. Hernández-Rey , B. Herold , A. Herrero , J. Hößl , J. Hofestädt , C. Hugon , C. W James , M. de Jong , M. Kadler , O. Kalekin , U. Katz , D. Kießling , P. Kooijman , A. Kouchner , I. Kreykenbohm , V. Kulikovskiy , R. Lahmann , E. Lambard , G. Lambard , D. Lattuada , D. Lefèvre , E. Leonora , H. Loehner , S. Loucatos , S. Mangano , M. Marcelin , A. Margiotta , J. A. Martínez-Mora , S. Martini , A. Mathieu , T. Michael , P. Migliozzi , C. Mueller , M. Neff , E. Nezri , D. Palioselitis , G. E. Pavalas , C. Perrina , P. Piattelli , V. Popa , T. Pradier , C. Racca , G. Riccobene , R. Richter , K. Roensch , A. Rostovtsev , M. Saldaña , D. F. E. Samtleben , A. Sánchez-Losa , M. Sanguineti , J. Schmid , J. Schnabel , S. Schulte , F. Schüssler , T. Seitz , C. Sieger , A. Spies , M. Spurio , J. J. M. Steijger , Th. Stolarczyk , M. Taiuti , C. Tamburini , Y. Tayalati , A. Trovato , B. Vallage , C. Vallée , V. Van Elewyck , E. Visser , D. Vivolo , S. Wagner , J. Wilms , E. de Wolf , K. Yatkin , H. Yepes , J. D. Zornoza , J. Zúñiga

High-energy neutrinos could be produced in the interaction of charged cosmic rays with matter or radiation surrounding astrophysical sources. To look for transient sources associated with neutrino emission, a follow-up program of neutrino…

High Energy Astrophysical Phenomena · Physics 2024-02-27 A. Albert , S. Alves , M. André , M. Ardid , S. Ardid , J. -J. Aubert , J. Aublin , B. Baret , S. Basa , Y. Becherini , B. Belhorma , M. Bendahman , F. Benfenati , V. Bertin , S. Biagi , M. Bissinger , J. Boumaaza , M. Bouta , M. C. Bouwhuis , H. Brânzas , R. Bruijn , J. Brunner , J. Busto , B. Caiffi , D. Calvo , S. Campion , A. Capone , L. Caramete , F. Carenini , J. Carr , V. Carretero , S. Celli , L. Cerisy , M. Chabab , R. Cherkaoui El Moursli , T. Chiarusi , M. Circella , J. A. B. Coelho , A. Coleiro , R. Coniglione , P. Coyle , A. Creusot , A. S. M. Cruz , A. F. Díaz , B. De Martino , C. Distefano , I. Di Palma , C. Donzaud , D. Dornic , D. Drouhin , T. Eberl , T. van Eeden , D. van Eijk , S. El Hedri , N. El Khayati , A. Enzenhöfer , P. Fermani , G. Ferrara , F. Filippini , L. Fusco , S. Gagliardini , J. García , C. Gatius Oliver , P. Gay , N. Geißelbrecht , H. Glotin , R. Gozzini , R. Gracia Ruiz , K. Graf , C. Guidi , L. Haegel , S. Hallmann , H. van Haren , A. J. Heijboer , Y. Hello , L. Hennig , J. J. Hernández-Rey , J. Hößl , J. Hofestädt , F. Huang , G. Illuminati , C. W. James , B. Jisse-Jung , M. de Jong , P. de Jong , M. Kadler , O. Kalekin , U. Katz , A. Kouchner , I. Kreykenbohm , V. Kulikovskiy , R. Lahmann , M. Lamoureux , A. Lazo , D. Lefèvre , E. Leonora , G. Levi , S. Le Stum , S. Loucatos , L. Maderer , J. Manczak , M. Marcelin , A. Margiotta , A. Marinelli , J. A. Martínez-Mora , P. Migliozzi , A. Moussa , R. Muller , S. Navas , E. Nezri , B. Ó Fearraigh , E. Oukacha , A. Pāun , G. E. Pāvālas , S. Peña-Martínez , M. Perrin-Terrin , P. Piattelli , V. Popa , T. Pradier , N. Randazzo , D. Real , G. Riccobene , A. Romanov , A. Sánchez-Losa , A. Saina , F. Salesa Greus , D. F. E. Samtleben , M. Sanguineti , P. Sapienza , J. Schnabel , J. Schumann , F. Schüssler , J. Seneca , M. Spurio , Th. Stolarczyk , M. Taiuti , Y. Tayalati , S. J. Tingay , B. Vallage , G. Vannoye , V. Van Elewyck , S. Viola , D. Vivolo , J. Wilms , S. Zavatarelli , A. Zegarelli , J. D. Zornoza , J. Zúñiga , V. Lipunov , G. Antipov , P. Balanutsa , D. Buckley , N. Budnev , A. Chasovnikov , D. Cheryasov , C. Francile , A. Gabovich , E. Gorbovskoy , I. Gorbunov , O. Gress , V. Kornilov , A. Kuznetsov , A. Iyudin , R. Podesta , F. Podesta , R. Rebolo Lopez , V. Senik , M. Sierra-Rucart , S. Svertilov , N. Tiurina , D. Vlasenko , I. Yashin , K. Zhirkov , S. Croft , D. L. Kaplan , G. E. Anderson , A. Williams , D. Dobie , K. W. Bannister , P. J. Hancock , P. A. Evans , J. A. Kennea , J. P. Osborne , S. B. Cenko , S. Antier , J. L. Atteia , M. Boër , A. Klotz , S. Chaty , K. Hodapp , V. Savchenko

The study of flaring astrophysical events in the multi-messenger approach requires instantaneous follow-up observations to better understand the nature of these events through complementary observational data. We present Astro-COLIBRI as a…

Instrumentation and Methods for Astrophysics · Physics 2023-01-31 P. Reichherzer , F. Schüssler , V. Lefranc , J. Becker Tjus , J. Mourier , A. K. Alkan

Observations of transient phenomena, such as GRBs, FRBs, novae/supernovae explosions, coupled with the detection of cosmic messengers like high-energy neutrinos and gravitational waves, have transformed astrophysics. Maximizing the…

Instrumentation and Methods for Astrophysics · Physics 2024-06-05 Fabian Schüssler , A. Kaan Alkan , M. de Bony de Lavergne , J. Mourier

EMBERS is an anticipatory intelligence system forecasting population-level events in multiple countries of Latin America. A deployed system from 2012, EMBERS has been generating alerts 24x7 by ingesting a broad range of data sources…

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

Observability in cloud infrastructure is critical for service providers, driving the widespread adoption of anomaly detection systems for monitoring metrics. However, existing systems often struggle to simultaneously achieve explainability,…

Machine Learning · Computer Science 2025-01-27 Yile Gu , Yifan Xiong , Jonathan Mace , Yuting Jiang , Yigong Hu , Baris Kasikci , Peng Cheng

Cloud computing is ubiquitous: more and more companies are moving the workloads into the Cloud. However, this rise in popularity challenges Cloud service providers, as they need to monitor the quality of their ever-growing offerings…

Distributed, Parallel, and Cluster Computing · Computer Science 2021-08-04 Mohammad Saiful Islam , William Pourmajidi , Lei Zhang , John Steinbacher , Tony Erwin , Andriy Miranskyy

The plethora of space-borne and ground-based observatories has provided astrophysicists with an unprecedented volume of data, which can only be processed at scale using advanced computing algorithms. Consequently, ensuring the quality of…

Machine Learning · Computer Science 2025-09-19 Mahsa Khazaei , Azim Ahmadzadeh , Alexei Pevtsov , Luca Bertello , Alexander Pevtsov

We describe the development of a system for an automated, iterative, real-time classification of transient events discovered in synoptic sky surveys. The system under development incorporates a number of Machine Learning techniques, mostly…

Instrumentation and Methods for Astrophysics · Physics 2011-10-24 S. G. Djorgovski , C. Donalek , A. Mahabal , B. Moghaddam , M. Turmon , M. Graham , A. Drake , N. Sharma , Y. Chen

Both multi-messenger astronomy and new high-throughput wide-field surveys require flexible tools for the selection and analysis of astrophysical transients. We here introduce the Alert Management, Photometry and Evaluation of Lightcurves…

The expansion of exoplanet observations has created a need for flexible, accessible, and user-friendly workflows. Transmission spectroscopy has become a key technique for probing atmospheric composition of transiting exoplanets. The…

Earth and Planetary Astrophysics · Physics 2026-03-31 Emilie Panek , Alexander Roman , Gaurav Shukla , Leonardo Pagliaro , Katia Matcheva , Konstantin Matchev

In this study, we address one of the challenges of developing NER models for scholarly domains, namely the scarcity of suitable labeled data. We experiment with an approach using predictions from a fine-tuned LLM model to aid non-domain…

Computation and Language · Computer Science 2024-05-07 Julia Evans , Sameer Sadruddin , Jennifer D'Souza

Skyalert.org is a web application to collect and disseminate observations about time-critical astronomical transients, and to add annotations and intelligent machine-learning to those observations. The information is "pushed" to…

Instrumentation and Methods for Astrophysics · Physics 2009-06-12 R. D. Williams , S. G. Djorgovski , A. J. Drake , M. J. Graham , A. Mahabal

In time-domain astronomy, STLF (Short-Timescale and Large Field-of-view) sky survey is the latest way of sky observation. Compared to traditional sky survey who can only find astronomical phenomena, STLF sky survey can even reveal how short…

Databases · Computer Science 2018-11-28 Chen Yang , Xiaofeng Meng , Zhihui Du , JiaMing Qiu , Kenan Liang , Yongjie Du , Zhiqiang Duan , Xiaobin Ma , Zhijian Fang

The ANTARES collaboration is building a deep sea neutrino telescope in the Mediterranean Sea. This detector will cover a sensitive area of typically 0.1 km-squared and will be equipped with about 1000 optical modules. Each of these optical…

Astrophysics · Physics 2012-08-27 The ANTARES Collaboration

An automated, rapid classification of transient events detected in the modern synoptic sky surveys is essential for their scientific utility and effective follow-up using scarce resources. This presents some unusual challenges: the data are…

Instrumentation and Methods for Astrophysics · Physics 2016-11-17 S. G. Djorgovski , A. A. Mahabal , C. Donalek , M. J. Graham , A. J. Drake , B. Moghaddam , M. Turmon