809 citations · 28.2k across the 927 of their papers we have counts for
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Bright polariton OLEDs operating in the ultra-strong coupling regime
Armando Genco, Alessandro Ridolfo, Salvatore Savasta +3
The generation and control of exotic phenomena in organic electroluminescent microcavities, such as polariton lasing and non-linear optical effects, operating in strong and ultra-s…
Atomic adsorption on pristine graphene along the Periodic Table of Elements - From PBE to non-local functionals
Igor A. Pašti, Aleksandar Jovanović, Ana S. Dobrota +3
The understanding of atomic adsorption on graphene is of high importance for many advanced technologies. Here we present a complete database of the atomic adsorption energies for t…
Performance of a First Microhexcavity Plasma Panel Detector with Muons
Alexis Mulski, Yan Benhamou, Erez Etzion +6
The microhexcavity plasma panel detector is a type of gaseous particle detector consisting of a close-packed array of millimeter-size hexagonal cells. The cells are biased to opera…
XMM-Newton imaging of V1818 Ori: a young stellar group on the eastern edge of the Kappa Ori ring
I. Pillitteri, S. J. Wolk, S. T. Megeath
We present the results of a 40 ks XMM-Newton observation centered on the variable star V1818 Ori. Using a combination of the XMM-Newton and AllWISE catalog data, we identify a grou…
Fe I oscillator strengths for transitions from high-lying odd-parity levels
M. T. Belmonte, J. C. Pickering, M. P. Ruffoni +4
We report new experimental Fe I oscillator strengths obtained by combining measurements of branching fractions measured with a Fourier Transform spectrometer and time-resolved lase…
Forming spectroscopic massive proto-binaries by disk fragmentation
D. M. -A. Meyer, R. Kuiper, W. Kley +2
The surroundings of massive protostars constitute an accretion disc which has numerically been shown to be subject to fragmentation and responsible for luminous accretion-driven ou…
CO emission tracing a warp or radial flow within 100 au in the HD 100546 protoplanetary disk
Catherine Walsh, Cail Daley, Stefano Facchini +1
We present spatially resolved ALMA images of CO J=3-2 emission from the protoplanetary disk around HD100546. We model the spatially-resolved kinematic structure of the CO emission.…
Galaxy And Mass Assembly (GAMA): The Consistency of GAMA and WISE Derived Mass-to-Light Ratios
T. Kettlety, J. Hesling, S. Phillipps +11
Recent work has suggested that mid-IR wavelengths are optimal for estimating the mass-to-light ratios of stellar populations and hence the stellar masses of galaxies. We compare st…
Theoretical oscillation frequencies for solar-type dwarfs from stellar models with -atmospheres
Andreas Christ Sølvsten Jørgensen, Achim Weiss, Jakob Rørsted Mosumgaard +2
We present a new method for replacing the outermost layers of stellar models with interpolated atmospheres based on results from 3D simulations, in order to correct for structural…
Microhexcavity Plasma Panel Detectors
Alexis Mulski, Daniel S. Levin, Yan Benhamou +8
Plasma panel detectors are a variant of micropattern detectors that are sensitive to ionizing radiation. They are motivated by the design and operation of plasma display panels. Th…
Orbital Dynamics of Candidate Transitional Millisecond Pulsar 3FGL J1544.6-1125: An unusually face-on system
Christopher T. Britt, Jay Strader, Laura Chomiuk +4
We present the orbital solution for the donor star of the candidate transitional millisecond pulsar 3FGL J1544.6-1125, currently observed as an accreting low-mass X-ray binary. The…
MAGIC Contributions to the 35th International Cosmic Ray Conference (ICRC2017)
MAGIC Collaboration, M. L. Ahnen, S. Ansoldi +143
MAGIC (Major Atmospheric Gamma Imaging Cherenkov) is a system of two 17 m diameter, F/1.03 Imaging Atmospheric Cherenkov Telescopes (IACT). They are dedicated to the observation of…
Short-wavelength out-of-band EUV emission from Sn laser-produced plasma
F. Torretti, R. Schupp, D. Kurilovich +5
We present the results of spectroscopic measurements in the extreme ultraviolet (EUV) regime (7-17 nm) of molten tin microdroplets illuminated by a high-intensity 3-J, 60-ns Nd:YAG…
Asteroseismic masses of retired planet-hosting A-stars using SONG
D. Stello, D. Huber, F. Grundahl +9
To better understand how planets form, it is important to study planet occurrence rates as a function of stellar mass. However, estimating masses of field stars is often difficult.…
Discovery of a radio relic in the low mass, merging galaxy cluster PLCK G200.9-28.2
Ruta Kale, Daniel R. Wik, Simona Giacintucci +5
Radio relics at the peripheries of galaxy clusters are tracers of the elusive cluster merger shocks. We report the discovery of a single radio relic in the galaxy cluster PLCK G200…
Simulations for 21 cm radiation lensing at EoR redshifts
Alessandro Romeo, R. Benton Metcalf, Alkistis Pourtsidou
We introduce simulations aimed at assessing how well weak gravitational lensing of 21cm radiation from the Epoch of Reionization () can be measured by an SKA-like radio t…
The Magellanic Inter-Cloud Project (MAGIC) III: First spectroscopic evidence of a dwarf stripping a dwarf
Ricardo Carrera, Blair C. Conn, Noelia E. D. Noël +2
The Magellanic Bridge (MB) is a gaseous stream that links the Large (LMC) and Small (SMC) Magellanic Clouds. Current simulations suggest that the MB forms from a recent interaction…
Comprehensive study of the dynamics of a classical Kitaev spin liquid
A. M. Samarakoon, A. Banerjee, S. -S. Zhang +5
We study the spin- Kitaev model in the classical () limit using Monte Carlo simulations combined with semi-classical spin dynamics. We discuss differences and simi…
Testing and improving shear viscous phase space correction models
Mridula Damodaran, Denes Molnar, Gergely Gábor Barnaföldi +2
Comparison of hydrodynamic calculations with experimental data inevitably requires a model for converting the fluid to particles. In this work, nonlinear kinetic theory is…
Stellar laboratories. IX. New Se V, Sr IV - VII, Te VI, and I VI oscillator strengths and the Se, Sr, Te, and I abundances in the hot white dwarfs G191-B2B and RE 0503-289
T. Rauch, P. Quinet, M. Knoerzer +4
To analyze spectra of hot stars, advanced non-local thermodynamic equilibrium (NLTE) model-atmosphere techniques are mandatory. Reliable atomic data is for the calculation of such…
High resolution spectroscopy of the extended narrow-line region of IC 5063 and NGC 7212
E. Congiu, M. Contini, S. Ciroi +6
We studied the properties of the gas of the extended narrow line region (ENLR) of two Seyfert 2 galaxies: IC 5063 and NGC 7212. We analysed high resolution spectra to investigate h…
Finding bright Lyman- emitters with lensing: prospects for Euclid
Lucia Marchetti, Stephen Serjeant, Mattia Vaccari
We model the Ly luminosity function to estimate the number of lensed high Ly emitters that may be detected by the Euclid Deep Survey. To span the whole range…
A novel JEAnS analysis of the Fornax dwarf using evolutionary algorithms: mass follows light with signs of an off-centre merger
Foivos I. Diakogiannis, Geraint F. Lewis, Rodrigo A. Ibata +4
Dwarf galaxies, among the most dark matter dominated structures of our universe, are excellent test-beds for dark matter theories. Unfortunately, mass modelling of these systems su…
15N Fractionation in Infrared-Dark Cloud Cores
S. Zeng, I. Jimenez-Serra, G. Cosentino +6
Nitrogen is one of the most abundant elements in the Universe and its 14N/15N isotopic ratio has the potential to provide information about the initial environment in which our Sun…