activity
19952024
most citedBinary Population and Spectral Synthesis Version 2.1: construction, observational verification and new results

953 citations · 10.8k across the 245 of their papers we have counts for

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Showing 2018Show all

23 papers · 1 filter

astro-ph.GA2018

The host galaxies of luminous type 2 AGN at 0.3-0.4

J. J. Urbano-Mayorgas, M. Villar Martín, F. Buitrago +7

We study the morphological and structural properties of the host galaxies associated with 57 optically-selected luminous type 2 AGN at 0.3-0.4: 16 high-luminosity Seyfert 2…

astro-ph.GA2018

Local disc model in view of Gaia DR1 and RAVE data

K. Sysoliatina, A. Just, I. Koutsouridou +8

We test the performance of the semi-analytic self-consistent Just-Jahreiß disc model (JJ model) with the astrometric data from the Tycho-Gaia Astrometric Solution (TGAS) sub-catalo…

astro-ph.GA2018

Dust spectrum and polarisation at 850 um in the massive IRDC G035.39-00.33

Mika Juvela, Vincent Guillet, Tie Liu +18

The dust sub-millimetre polarisation of star-forming clouds carries information on dust and the role of magnetic fields in cloud evolution. With observations of a dense filamentary…

astro-ph.HE2018

LOFAR discovery of a 23.5-second radio pulsar

C. M. Tan, C. G. Bassa, S. Cooper +16

We present the discovery of PSR J0250+5854, a radio pulsar with a spin period of 23.5 s. This is the slowest-spinning radio pulsar known. PSR J0250+5854 was discovered by the LOFAR…

astro-ph.HE2018

The 1989 and 2015 outbursts of V404 Cygni: a global study of wind-related optical features

D. Mata Sánchez, T. Muñoz-Darias, J. Casares +19

The black hole transient V404 Cygni exhibited a bright outburst in June 2015 that was intensively followed over a wide range of wavelengths. Our team obtained high time resolution…

nucl-ex2018

Production cross section and decay study of Es and Md

R. Briselet, Ch. Theisen, M. Vandebrouck +42

In the study of the odd-, even- nuclei Es and Md, performed at the University of Jyväskylä, the fusion-evaporation reactions Au(Ca,2)$^{243}…