English
Related papers

Related papers: A systematically-selected sample of luminous, long…

200 papers

We present the discovery that ATLAS18mlw was a tidal disruption event (TDE) in the galaxy WISEA J073544.83+663717.3, at a luminosity distance of 334 Mpc. Initially discovered by the Asteroid Terrestrial Impact Last Alert System (ATLAS) on…

Long Period Transients (LPTs) are a recently identified class of sources characterized by periodic radio bursts lasting seconds to minutes, with flux densities that might reach several tens of Jy. These radio bursts repeat with periodicity…

High Energy Astrophysical Phenomena · Physics 2026-02-11 Nanda Rea , Natasha Hurley-Walker , Manisha Caleb

For decades optical time-domain searches have been tuned to find ordinary supernovae, which rise and fall in brightness over a period of weeks. Recently, supernova searches have improved their cadences and a handful of fast-evolving…

Using a filter in the GROWTH Marshal based on color and the amplitude and the timescale of variability, we have identified 372 objects as known or candidate cataclysmic variables (CVs) during the second year of operation of the Zwicky…

AM CVn systems are ultra-compact, helium-rich, accreting binaries with degenerate or semi-degenerate donors. We report the discovery of five new eclipsing AM CVn systems with orbital periods of 61.5, 55.5, 53.3, 37.4, and 35.4 minutes.…

The Galactic center has some of the highest stellar densities in the Galaxy and a range of interstellar scattering properties that may aid in the detection of new radio-selected transient events. Here we describe a search for radio…

High Energy Astrophysical Phenomena · Physics 2016-12-14 Anirudh Chiti , Shami Chatterjee , Robert Wharton , James Cordes , T. Joseph W. Lazio , David L. Kaplan , Geoffrey C. Bower , Steve Croft

ANTARES, a neutrino detector located in the depths of the Mediterranean Sea, operated successfully for over 15 years before being decommissioned in 2022. The telescope offered an ideal vantage view of the Southern Sky and benefited from…

High Energy Astrophysical Phenomena · Physics 2025-11-11 ANTARES Collaboration , A. Albert , S. Alves , M. André , M. Ardid , S. Ardid , J. J. Aubert , J. Aublin , B. Baret , S. Basa , Y. Becherini , B. Belhorma , F. Benfenati , V. Bertin , S. Biagi , J. Boumaaza , M. Bouta , M. C. Bouwhuis , H. Brânzaş , R. Bruijn , J. Brunner , J. Busto , B. Caiffi , D. Calvo , S. Campion , A. Capone , F. Carenini , J. Carr , V. Carretero , T. Cartraud , 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. F. Díaz , B. De Martino , C. Distefano , I. Di Palma , C. Donzaud , D. Dornic , D. Drouhin , T. Eberl , A. Eddymaoui , 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 , F. Huang , G. Illuminati , 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 , 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. M. Păun , G. E. Păvălaş , S. Peña-Martínez , M. Perrin-Terrin , P. Piattelli , C. Poirè , 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 , F. Schüssler , J. Seneca , M. Spurio , Th. Stolarczyk , M. Taiuti , Y. Tayalati , B. Vallage , G. Vannoye , V. Van Elewyck , S. Viola , D. Vivolo , J. Wilms , S. Zavatarelli , A. Zegarelli , J. D. Zornoza , J. Zúñiga

We present optical/UV photometric and spectroscopic observations, as well as X-ray and radio follow-up, of the extraordinary event AT2019cmw. With a peak bolometric luminosity of ~$\mathrm{10^{45.6}\,erg\,s^{-1}}$, it is one of the most…

Jetted Active Galactic Nuclei (AGN) exhibit variability across a wide range of time scales. Traditionally, this variability can often be modeled well as a stochastic process. However, in certain cases, jetted AGN variability displays…

High Energy Astrophysical Phenomena · Physics 2025-01-03 P. Penil , A. Domínguez , S. Buson , M. Ajello , S. Adhikari , A. Rico

The Weizmann Fast Astronomical Survey Telescope (W-FAST) is a 55cm optical survey telescope with a high cadence (25Hz) monitoring of the sky over a wide field of view (~7deg^2). The high frame rate allows detection of sub-second transients…

Instrumentation and Methods for Astrophysics · Physics 2021-05-26 Guy Nir , Eran O. Ofek , Sagi Ben-Ami , Noam Segev , David Polishook , Ilan Manulis

The fast blue optical transients (FBOTs) are a new population of extragalactic transients of unclear physical origin. A variety of mechanisms have been proposed including failed supernova explosion, shock interaction with a dense medium,…

Two X-ray sources were recently discovered by Irwin et al. in compact companions to elliptical galaxies to show ultra-luminous flares with fast rise (~ minute) and decay (~ hour), and with a peak luminosity ~10^{40-41} erg/s. Together with…

High Energy Astrophysical Phenomena · Physics 2019-02-05 Rong-Feng Shen

Wide-field survery have recently detected recurring optical and X-ray sources near galactic nuclei, with period spanning hours to years. These phenomena could result from repeated partial tidal disruptions of stars by supermassive black…

High Energy Astrophysical Phenomena · Physics 2023-11-10 Itai Linial , Eliot Quataert

Almost all Galactic black hole binaries with low mass donor stars are transient X-ray sources; we expect most of the X-ray transients observed in external galaxies to be black hole binaries also. Obtaining period estimates for…

High Energy Astrophysical Phenomena · Physics 2015-06-04 R. Barnard , J. L. Galache , M. Garcia , N. Nooraee , P. J. Callanan , A. Zezas , S. S. Murray

Changing-look (CL) AGN are unique probes of accretion onto supermassive black holes (SMBHs), especially when simultaneous observations in complementary wavebands allow investigations into the properties of their accretion flows. We present…

The James Webb Space Telescope (JWST) has opened up a new window to study highly reddened explosive transients. We present results from late-time (1421 days post-explosion) JWST follow-up spectroscopic observations with NIRSpec and MIRI LRS…

Solar and Stellar Astrophysics · Physics 2024-07-31 Sam Rose , Ryan M. Lau , Jacob E. Jencson , Mansi M. Kasliwal , Kishalay De , Michael E. Ressler , Ori D. Fox , Matthew J. Hankins

We report the automatic detection of 11 transients (7 possible supernovae and 4 active galactic nuclei candidates) within the Zwicky Transient Facility fourth data release (ZTF DR4), all of them observed in 2018 and absent from public…

Instrumentation and Methods for Astrophysics · Physics 2022-06-01 P. D. Aleo , K. L. Malanchev , M. V. Pruzhinskaya , E. E. O. Ishida , E. Russeil , M. V. Kornilov , V. S. Korolev , S. Sreejith , A. A. Volnova , G. S. Narayan

We construct a menu of objects that can give rise to bright flares when disrupted by massive black holes (BHs), ranging from planets to evolved stars. Through their tidal disruption, main sequence and evolved stars can effectively probe the…

High Energy Astrophysical Phenomena · Physics 2022-07-26 Jamie Law-Smith , Morgan MacLeod , James Guillochon , Phillip Macias , Enrico Ramirez-Ruiz

Luminous red novae (LRNe) are transients characterized by low luminosities and expansion velocities, and are associated with mergers or common envelope ejections in stellar binaries. Intermediate-luminosity red transients (ILRTs) are an…

‹ Prev 1 8 9 10 Next ›