Search Results - "Prieto, J. L"
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Generation of coherent spin-wave modes in yttrium iron garnet microdiscs by spin–orbit torque
Published in Nature communications (27-01-2016)“…In recent years, spin–orbit effects have been widely used to produce and detect spin currents in spintronic devices. The peculiar symmetry of the spin Hall…”
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2
Full control of the spin-wave damping in a magnetic insulator using spin-orbit torque
Published in Physical review letters (07-11-2014)“…It is demonstrated that the threshold current for damping compensation can be reached in a 5 μm diameter YIG(20 nm)|Pt(7 nm) disk. The demonstration rests…”
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3
Giant sharp and persistent converse magnetoelectric effects in multiferroic epitaxial heterostructures
Published in Nature materials (01-05-2007)“…Magnetoelectric coupling between magnetic and electrical properties presents valuable degrees of freedom for applications. The two most promising scenarios are…”
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4
Six months of multiwavelength follow-up of the tidal disruption candidate ASASSN-14li and implied TDE rates from ASAS-SN
Published in Monthly notices of the Royal Astronomical Society (21-01-2016)“…We present ground-based and Swift photometric and spectroscopic observations of the candidate tidal disruption event (TDE) ASASSN-14li, found at the centre of…”
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5
ASASSN-18tb: a most unusual Type Ia supernova observed by TESS and SALT
Published in Monthly notices of the Royal Astronomical Society (01-08-2019)“…ABSTRACT We present photometric and spectroscopic observations of the unusual Type Ia supernova ASASSN-18tb, including a series of Southern African Large…”
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6
High tide: a systematic search for ellipsoidal variables in ASAS-SN
Published in Monthly notices of the Royal Astronomical Society (01-10-2021)“…ABSTRACT The majority of non-merging stellar mass black holes are discovered by observing high energy emission from accretion processes. Here, we pursue the…”
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7
The Luminous and Carbon-rich Supernova 2006gz: A Double Degenerate Merger?
Published in The Astrophysical journal (01-11-2007)“…Spectra and light curves of SN 2006gz show the strongest signature of unburned carbon and one of the slowest fading light curves ever seen in a Type Ia event […”
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8
First Resolution of Microlensed Images
Published in The Astrophysical journal (20-01-2019)“…Abstract We employ Very Large Telescope Interferometer GRAVITY to resolve, for the first time, the two images generated by a gravitational microlens. The…”
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9
Nutation Spectroscopy of a Nanomagnet Driven into Deeply Nonlinear Ferromagnetic Resonance
Published in Physical review. X (19-11-2019)“…Strongly out-of-equilibrium regimes in magnetic nanostructures exhibit novel properties, linked to the nonlinear nature of magnetization dynamics, which are of…”
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10
ASASSN-15lh: A highly super-luminous supernova
Published in Science (American Association for the Advancement of Science) (15-01-2016)“…We report the discovery of ASASSN-15lh (SN 2015L), which we interpret as the most luminous supernova yet found. At redshift z = 0.2326, ASASSN-15lh reached an…”
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The relative specific Type Ia supernovae rate from three years of ASAS-SN
Published in Monthly notices of the Royal Astronomical Society (11-04-2019)“…ABSTRACT We analyse the 476 SN Ia host galaxies from the All-Sky Automated Survey for Supernova (ASAS-SN) Bright Supernova Catalogues to determine the observed…”
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12
High-efficiency control of spin-wave propagation in ultra-thin yttrium iron garnet by the spin-orbit torque
Published in Applied physics letters (25-04-2016)“…We study experimentally with submicrometer spatial resolution the propagation of spin waves in microscopic waveguides based on the nanometer-thick yttrium iron…”
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13
The Largest M Dwarf Flares from ASAS-SN
Published in The Astrophysical journal (10-05-2019)“…The All-sky Automated Survey for Supernovae (ASAS-SN) is the only project in existence to scan the entire sky in optical light approximately every day,…”
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14
Cataclysmic variables from the Catalina Real-time Transient Survey
Published in Monthly notices of the Royal Astronomical Society (21-06-2014)“…We present 855 cataclysmic variable candidates detected by the Catalina Real-time Transient Survey (CRTS) of which at least 137 have been spectroscopically…”
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15
Cool, Luminous, and Highly Variable Stars in the Magellanic Clouds from ASAS-SN: Implications for Thorne–Żytkow Objects and Super-asymptotic Giant Branch Stars
Published in The Astrophysical journal (01-10-2020)“…Abstract Stars with unusual properties can provide a wealth of information about rare stages of stellar evolution and exotic physics. However, determining the…”
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SN 2007bg: the complex circumstellar medium around one of the most radio-luminous broad-lined Type Ic supernovae
Published in Monthly notices of the Royal Astronomical Society (11-01-2013)“…In this paper we present the results of the radio light curve and X-ray observations of broad-lined Type Ic (Ic-BL) SN 2007bg. The light curve shows three…”
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THE YOUNG AND BRIGHT TYPE IA SUPERNOVA ASASSN-14lp: DISCOVERY, EARLY-TIME OBSERVATIONS, FIRST-LIGHT TIME, DISTANCE TO NGC 4666, AND PROGENITOR CONSTRAINTS
Published in The Astrophysical journal (01-08-2016)“…ABSTRACT On 2014 December 9.61, the All-sky Automated Survey for SuperNovae (ASAS-SN or "Assassin") discovered ASASSN-14lp just ∼2 days after first light using…”
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Beryllium detection in the very fast nova ASASSN-16kt (V407 Lupi)
Published in Monthly notices of the Royal Astronomical Society (01-08-2018)“…Abstract We present high-resolution spectroscopic observations of the fast nova ASASSN-16kt (V407 Lup). A close inspection of spectra obtained at early stages…”
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The ALMA early science view of FUor/EXor objects – II. The very wide outflow driven by HBC 494
Published in Monthly notices of the Royal Astronomical Society (21-04-2017)“…Abstract We present Atacama Large Millimeter/sub-millimeter Array Cycle-2 observations of the HBC 494 molecular outflow and envelope. HBC 494 is an FU Ori-like…”
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The unexpected, long-lasting, UV rebrightening of the superluminous supernova ASASSN-15lh
Published in Monthly notices of the Royal Astronomical Society (01-04-2017)“…Given its peak luminosity and early-time spectra, ASASSN-15lh was classified as the most luminous supernova ever discovered. Here, we report a UV rebrightening…”
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