Search Publications

The behaviour of dark matter associated with four bright cluster galaxies in the 10 kpc core of Abell 3827
DOI: 10.1093/mnras/stv467 Bibcode: 2015MNRAS.449.3393M

Richard, Johan; Hilton, Matt; Massey, Richard +20 more

Galaxy cluster Abell 3827 hosts the stellar remnants of four almost equally bright elliptical galaxies within a core of radius 10 kpc. Such corrugation of the stellar distribution is very rare, and suggests recent formation by several simultaneous mergers. We map the distribution of associated dark matter, using new Hubble Space Telescope imaging …

2015 Monthly Notices of the Royal Astronomical Society
eHST 158
The Herschel Comprehensive (U)LIRG Emission Survey (HERCULES): CO Ladders, Fine Structure Lines, and Neutral Gas Cooling
DOI: 10.1088/0004-637X/801/2/72 Bibcode: 2015ApJ...801...72R

Veilleux, S.; Sanders, D. B.; Isaak, K. G. +27 more

(Ultra) luminous infrared galaxies ((U)LIRGs) are objects characterized by their extreme infrared (8-1000 µm) luminosities (L LIRG > 1011 L and L ULIRG > 1012 L ). The Herschel Comprehensive ULIRG Emission Survey (PI: van der Werf) presents a representative flux-limit…

2015 The Astrophysical Journal
Herschel 157
The far-infrared/radio correlation and radio spectral index of galaxies in the SFR-M plane up to z~2
DOI: 10.1051/0004-6361/201424937 Bibcode: 2015A&A...573A..45M

Berta, S.; Magnelli, B.; Nordon, R. +21 more

We study the evolution of the radio spectral index and far-infrared/radio correlation (FRC) across the star-formation rate - stellar masse (i.e. SFR-M) plane up to z ~ 2. We start from a stellar-mass-selected sample of galaxies with reliable SFR and redshift estimates. We then grid the SFR-M plane in several redshift ranges…

2015 Astronomy and Astrophysics
Herschel 156
A new catalogue of Strömgren-Crawford uvbyβ photometry
DOI: 10.1051/0004-6361/201526413 Bibcode: 2015A&A...580A..23P

Paunzen, E.

Context. The uvbyβ photometric system is widely used for the study of various Galactic and extragalactic objects. It measures the colour due to temperature differences, the Balmer discontinuity, and blanketing absorption due to metals.
Aims: A new all-sky catalogue of all available uvbyβ measurements from the literature was generated.
Me…

2015 Astronomy and Astrophysics
Hipparcos 154
Regional surface morphology of comet 67P/Churyumov-Gerasimenko from Rosetta/OSIRIS images
DOI: 10.1051/0004-6361/201525723 Bibcode: 2015A&A...583A..26E

Jorda, L.; Lamy, P. L.; Lara, L. M. +51 more


Aims: The OSIRIS camera onboard the Rosetta spacecraft has been acquiring images of the comet 67P/Churyumov-Gerasimenko (67P)'s nucleus at spatial resolutions down to ~0.17 m/px ever since Aug. 2014. These images have yielded unprecedented insight into the morphological diversity of the comet's surface. This paper presents an overview of the …

2015 Astronomy and Astrophysics
Rosetta 154
Relativistic boost as the cause of periodicity in a massive black-hole binary candidate
DOI: 10.1038/nature15262 Bibcode: 2015Natur.525..351D

Haiman, Zoltán; Schiminovich, David; D'Orazio, Daniel J.

Because most large galaxies contain a central black hole, and galaxies often merge, black-hole binaries are expected to be common in galactic nuclei. Although they cannot be imaged, periodicities in the light curves of quasars have been interpreted as evidence for binaries, most recently in PG 1302-102, which has a short rest-frame optical period …

2015 Nature
eHST 154
Warm-hot baryons comprise 5-10 per cent of filaments in the cosmic web
DOI: 10.1038/nature16058 Bibcode: 2015Natur.528..105E

Richard, Johan; Massey, Richard; Kneib, Jean-Paul +8 more

Observations of the cosmic microwave background indicate that baryons account for 5 per cent of the Universe’s total energy content. In the local Universe, the census of all observed baryons falls short of this estimate by a factor of two. Cosmological simulations indicate that the missing baryons have not condensed into virialized haloes, but res…

2015 Nature
XMM-Newton eHST 154
NuSTAR Spectroscopy of Multi-component X-Ray Reflection from NGC 1068
DOI: 10.1088/0004-637X/812/2/116 Bibcode: 2015ApJ...812..116B

Hailey, Charles J.; Brandt, William N.; Comastri, Andrea +26 more

We report on high-energy X-ray observations of the Compton-thick Seyfert 2 galaxy NGC 1068 with NuSTAR, which provide the best constraints to date on its >10 keV spectral shape. The NuSTAR data are consistent with those from past and current instruments to within cross-calibration uncertainties, and we find no strong continuum or line variabili…

2015 The Astrophysical Journal
XMM-Newton 153
X-shooter reveals powerful outflows in z ∼ 1.5 X-ray selected obscured quasi-stellar objects
DOI: 10.1093/mnras/stu2117 Bibcode: 2015MNRAS.446.2394B

Lutz, D.; Maiolino, R.; Salvato, M. +20 more

We present X-shooter at Very Large Telescope observations of a sample of 10 luminous, X-ray obscured quasi-stellar objects (QSOs) at z ∼ 1.5 from the XMM-COSMOS survey, expected to be caught in the transitioning phase from starburst to active galactic nucleus (AGN)-dominated systems. The main selection criterion is X-ray detection at bright fluxes…

2015 Monthly Notices of the Royal Astronomical Society
eHST 153
Gaia FGK benchmark stars: abundances of α and iron-peak elements
DOI: 10.1051/0004-6361/201526604 Bibcode: 2015A&A...582A..81J

Gilmore, G.; Montes, D.; Recio-Blanco, A. +26 more

Context. In the current era of large spectroscopic surveys of the Milky Way, reference stars for calibrating astrophysical parameters and chemical abundances are of paramount importance.
Aims: We determine elemental abundances of Mg, Si, Ca, Sc, Ti, V, Cr, Mn, Co, and Ni for our predefined set of Gaia FGK benchmark stars.
Methods: By ana…

2015 Astronomy and Astrophysics
Gaia 152