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19962007
most citedA new code for automatic determination of equivalent widths: Automatic Routine for line Equivalent widths in stellar Spectra (ARES)

328 citations · 348 across the 5 of their papers we have counts for

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astro-ph2007328 cited

A new code for automatic determination of equivalent widths: Automatic Routine for line Equivalent widths in stellar Spectra (ARES)

S. G. Sousa, N. C. Santos, G. Israelian +2

We present a new automatic code (ARES) for determining equivalent widths of the absorption lines present in stellar spectra. We also describe its use for determining fundamental sp…

astro-ph200720 cited

Radio observations of the CDF-South: a possible link between radio emission and star formation in X-ray selected AGN

E. Rovilos, A. Georgakakis, I. Georgantopoulos +4

We explore the nature of the radio emission of X-ray selected AGN by combining deep radio (1.4GHz; 60micro-Jy) and X-ray data with multiwavelength (optical, mid-infrared) observati…

astro-ph2006

Multi-band Astronomy with LISA

G. Branduardi-Raymont, G. Ramsay, C. Wang +2

We discuss astrophysical scenarios relevant to the generation of gravitational waves (GW) and effects expected to arise from the interaction of GW and electromagnetic (EM) radiatio…

astro-ph2005

The Phoenix Deep Survey: The star-formation rates and the stellar masses of EROs

A. Georgakakis, A. M. Hopkins, J. Afonso +3

We estimate the star-formation rates and the stellar masses of the Extremely Red objects (EROs) detected in a 180arcmin2 Ks-band survey (Ks~20mag). This sample is complemented by s…

astro-ph2005

Cold Dust in (Some) High z Supernova Host Galaxies

D. L. Clements, D. Farrah, M. Rowan-Robinson +3

We present deep submillimetre photometry for 14 galaxies at z=0.5 that are hosts of type 1a supernovae, with the aim of examining the evolution of dust mass and extinction in norma…

astro-ph2004

The Phoenix Deep Survey: the radio properties of the hard X-ray selected sample

A. Georgakakis, A. M. Hopkins, J. Afonso +3

The radio properties of hard (2-8keV) X-ray selected sources are explored by combining a single 50ks XMM-Newton pointing with the ultra-deep and homogeneous Phoenix radio (1.4GHz)…