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相关论文: Spectroscopic Alerts for the Time-Domain Era

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Space-based time-domain telescopes such as CoRoT, Kepler/K2 and TESS have profoundly impacted astrophysics over the past two decades. Continuous light curves with high cadence and high photometric precision are now available for millions of…

太阳与恒星天体物理 · 物理学 2025-12-12 Daniel Huber

The advent of new observational facilities in the last two decades has allowed the rapid discovery and high-resolution optical imaging of many strong lens systems from galaxy to cluster scales, as well as their spectroscopic follow-up.…

天体物理学 · 物理学 2009-11-10 L. V. E. Koopmans , I. W. A. Browne , N. J. Jackson

Spiking Neural Networks (SNNs) promise efficient and dynamic spatio-temporal data processing. This paper reformulates a significant challenge in radio astronomy, Radio Frequency Interference (RFI) detection, as a time-series segmentation…

神经与进化计算 · 计算机科学 2026-01-23 Nicholas J. Pritchard , Andreas Wicenec , Mohammed Bennamoun , Richard Dodson

In this work, we propose a deep learning-based classification model of astronomical objects using alerts reported by the Zwicky Transient Facility (ZTF) survey. The model takes as inputs sequences of stamp images and metadata contained in…

天体物理仪器与方法 · 物理学 2024-05-27 Daniel Neira O. , Pablo A. Estévez , Francisco Förster

The EXTraS project (Exploring the X-ray Transient and variable Sky) will harvest the hitherto unexplored temporal domain information buried in the serendipitous data collected by the European Photon Imaging Camera (EPIC) instrument onboard…

高能天体物理现象 · 物理学 2019-08-15 A. De Luca , R. Salvaterra , A. Tiengo , D. D'Agostino , M. G. Watson , F. Haberl , J. Wilms

High-energy neutrinos could be produced in the interaction of charged cosmic rays with matter or radiation surrounding astrophysical sources. Even with the recent detection of extraterrestrial high-energy neutrinos by the IceCube…

高能天体物理现象 · 物理学 2016-03-16 S. Adrian-Martinez , M. Ageron , A. Albert , I. Al Samarai , M. Andre , G. Anton , M. Ardid , J. -J. Aubert , B. Baret , J. Barrios-Marti , 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 , T. Chiarusi , M. Circella , R. Coniglione , H. Costantini , P. Coyle , A. Creusot , I. Dekeyser , A. Deschamps , G. De Bonis , C. Distefano , C. Donzaud , D. Dornic , D. Drouhin , A. Dumas , T. Eberl , D. Elsasser , A. Enzenhofer , K. Fehn , I. Felis , P. Fermani , F. Folger , L. A. Fusco , S. Galata , P. Gay , S. Geißelsoder , K. Geyer , V. Giordano , A. Gleixner , R. Gracia-Ruiz , K. Graf , H. van Haren , A. J. Heijboer , Y. Hello , J. J. Hernandez-Rey , A. Herrero , J. Hoßl , J. Hofestadt , 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 , G. Lambard , D. Lattuada , D. Lefevre , E. Leonora , S. Loucatos , S. Mangano , M. Marcelin , A. Margiotta , J. A. Martinez-Mora , S. Martini , A. Mathieu , T. Michael , P. Migliozzi , A. Moussa , C. Mueller , M. Neff , E. Nezri , G. E. Pavalas , C. Pellegrino , C. Perrina , P. Piattelli , V. Popa , T. Pradier , C. Racca , G. Riccobene , R. Richter , K. Roensch , A. Rostovtsev , M. Saldana , D. F. E. Samtleben , M. Sanguineti , P. Sapienza , J. Schmid , J. Schnabel , S. Schulte , F. Schüssler , T. Seitz , C. Sieger , M. Spurio , J. J. M. Steijger , Th. Stolarczyk , A. Sanchez-Losa , M. Taiuti , C. Tamburini , A. Trovato , M. Tselengidou , C. Tonnis , D. Turpin , B. Vallage , C. Vallee , V. Van Elewyck , M. Vecchi , E. Visser , D. Vivolo , S. Wagner , J. Wilms , J. D. Zornoza , J. Zuniga , A. Klotz , M. Boer , A. Le Van Suu , C. Akerlof , W. Zheng , P. Evans , N. Gehrels , J. Kennea , J. P. Osborne , D. M. Coward

This work describes the context and approach for the detection of spectroscopic signatures from planets in the habitable zone of nearby stars. By understanding the limitations of current observatories, future telescopes can be understood,…

地球与行星天体物理 · 物理学 2026-04-13 Vincent Kofman

A next generation of space-based observatories aims to detect and characterize potentially Earth-like exoplanets around Sun-like stars using reflected light spectroscopy. However, it remains unclear how such direct imaging…

地球与行星天体物理 · 物理学 2025-10-28 Arnaud Salvador , Tyler D. Robinson

In the last decade a new generation of telescopes and sensors has allowed the production of a very large amount of data and astronomy has become, a data-rich science; this transition is often labeled as: "data revolution" and "data…

天体物理仪器与方法 · 物理学 2013-04-25 Stefano Cavuoti

Over the past decade, neutrino astronomy has emerged as a new window into the extreme and hidden universe. Current-generation experiments have detected high-energy neutrinos of astrophysical origin and identified the first sources, opening…

高能物理 - 实验 · 物理学 2025-06-25 C. A. Argüelles , F. Halzen , N. Kurahashi

Neutral hydrogen pervades the infant Universe, and its redshifted 21-cm signal allows one to chart the Universe. This signal allows one to probe astrophysical processes such as the formation of the first stars, galaxies, (super)massive…

The investigation of the emergence of life is a major endeavour of science. Astronomy is contributing to it in three fundamental manners: (1) by measuring the chemical enrichment of the Universe, (2) by investigating planet formation and…

The next generation of observatories will facilitate the discovery of new types of astrophysical transients. The detection of such phenomena, whose characteristics are presently poorly constrained, will hinge on the ability to perform blind…

高能天体物理现象 · 物理学 2019-02-15 Iftach Sadeh

Large sets of objects with spectroscopic redshift measurements will be needed for imaging dark energy experiments to achieve their full potential, serving two goals:_training_, i.e., the use of objects with known redshift to develop and…

Astronomy is entering a new era of discovery, coincident with the establishment of new facilities for observation and simulation that will routinely generate petabytes of data. While an increasing reliance on automated data analysis is…

天体物理仪器与方法 · 物理学 2015-05-27 Amr Hassan , Christopher J. Fluke

The changes in brightness of an astronomical source as a function of time are key probes into that source's physics. Periodic and quasi-periodic signals are indicators of fundamental time (and length) scales in the system, while stochastic…

天体物理仪器与方法 · 物理学 2023-08-08 Matteo Bachetti , Daniela Huppenkothen

The next generation of observatories will facilitate the discovery of new types of astrophysical transients. The detection of such phenomena, whose characteristics are presently poorly constrained, will hinge on the ability to perform blind…

高能天体物理现象 · 物理学 2019-08-06 Iftach Sadeh

Multimessenger astronomy seeks to uncover the origins of cosmic rays and neutrinos. The IceCube Neutrino Observatory plays a key role in monitoring the sky for revealing high energy neutrinos and neutrino time clusters possibly associated…

高能天体物理现象 · 物理学 2025-07-10 Caterina Boscolo Meneguolo , Elisa Bernardini , Jean-Pierre Jonckheere , Sarah Mancina

The primary challenge in the study of explosive astrophysical transients is their detection and characterisation using multiple messengers. For this purpose, we have developed a new data-driven discovery framework, based on deep learning.…

高能天体物理现象 · 物理学 2020-05-14 Iftach Sadeh