Search Publications

The progenitors of the Milky Way stellar halo: big bricks favoured over little bricks.
DOI: 10.1093/mnrasl/slv001 Bibcode: 2015MNRAS.448L..77D

Belokurov, V.; Deason, A. J.; Weisz, D. R.

We present a census of blue horizontal branch (BHB) and blue straggler (BS) stars belonging to dwarf galaxies and globular clusters, and compare these counts to that of the Milky Way stellar halo. We find, in agreement with earlier studies, that the ratio of BS-to-BHB stars in these satellite populations is dependent on stellar mass. Dwarf galaxie…

2015 Monthly Notices of the Royal Astronomical Society
eHST 58
Elemental Depletions in the Magellanic Clouds and the Evolution of Depletions with Metallicity
DOI: 10.1088/0004-637X/811/2/78 Bibcode: 2015ApJ...811...78T

Meixner, Margaret; Seale, Jonathan; Dwek, Eli +4 more

We present a study of the composition of gas and dust in the Large and Small Magellanic Clouds (LMC and SMC) using UV absorption spectroscopy. We measure P ii and Fe ii along 84 spatially distributed sightlines toward the MCs using archival Far Ultraviolet Spectroscopic Explorer observations. For 16 of those sightlines, we also measure Si ii, Cr i…

2015 The Astrophysical Journal
eHST 58
The VLT SINFONI Mg II Program for Line Emitters (SIMPLE). II. Background Quasars Probing Z ~ 1 Galactic Winds
DOI: 10.1088/0004-637X/804/2/83 Bibcode: 2015ApJ...804...83S

Finley, Hayley; Bouché, Nicolas; Contini, Thierry +3 more

The physical properties of galactic winds are of paramount importance for our understanding of galaxy formation. Fortunately, they can be constrained using background quasars passing near star-forming galaxies (SFGs). From the 14 quasar-galaxy pairs in our Very Large Telescope (VLT)/SINFONI Mg ii Program for Line Emitters sample, we reobserved the…

2015 The Astrophysical Journal
eHST 58
A survey of stellar X-ray flares from the XMM-Newton serendipitous source catalogue: HIPPARCOS-Tycho cool stars
DOI: 10.1051/0004-6361/201526217 Bibcode: 2015A&A...581A..28P

Rosen, S.; Pye, J. P.; Schröder, A. C. +1 more

Context. The X-ray emission from flares on cool (i.e. spectral-type F-M) stars is indicative of very energetic, transient phenomena, associated with energy release via magnetic reconnection.
Aims: We present a uniform, large-scale survey of X-ray flare emission. The XMM-Newton Serendipitous Source Catalogue and its associated data products pr…

2015 Astronomy and Astrophysics
Hipparcos XMM-Newton 58
The radio relic in Abell 2256: overall spectrum and implications for electron acceleration
DOI: 10.1051/0004-6361/201423972 Bibcode: 2015A&A...575A..45T

Lovisari, L.; Dallacasa, D.; Bonafede, A. +5 more

Context. Radio relics are extended synchrotron sources thought to be produced by shocks in the outskirts of merging galaxy clusters. The cluster Abell 2256 hosts one of the most intriguing examples in this class of sources. It has been found that this radio relic has a rather flat integrated spectrum at low frequencies that would imply an injectio…

2015 Astronomy and Astrophysics
Planck XMM-Newton 58
New light on Galactic post-asymptotic giant branch stars - I. First distance catalogue
DOI: 10.1093/mnras/stu2383 Bibcode: 2015MNRAS.447.1673V

Parker, Quentin A.; Vickers, Shane B.; Frew, David J. +1 more

We have commenced a detailed analysis of the known sample of Galactic post-asymptotic giant branch (PAGB) objects compiled in the Toruń catalogue of Szczerba et al., and present, for the first time, homogeneously derived distance determinations for the 209 likely and 87 possible catalogued PAGB stars from that compilation. Knowing distances are es…

2015 Monthly Notices of the Royal Astronomical Society
AKARI Herschel ISO IUE 58
Spectroscopic Confirmation of an Ultra Massive and Compact Galaxy at z = 3.35: a Detailed Look at an Early Progenitor of Local Giant Ellipticals
DOI: 10.1088/0004-637X/801/2/133 Bibcode: 2015ApJ...801..133M

van Dokkum, Pieter G.; Muzzin, Adam; Labbé, Ivo +10 more

We present the first spectroscopic confirmation of an ultramassive galaxy at redshift z\gt 3 using data from Keck-NIRSPEC, VLT-X-shooter, and GTC-Osiris. We detect strong [O iii] and Lyα emission, and weak [O ii], C iv, and He ii, placing C1-23152 at a spectroscopic redshift of {{z}spec}=3.351. The modeling of the emission-line-correcte…

2015 The Astrophysical Journal
eHST 57
Broadband Radio Polarimetry and Faraday Rotation of 563 Extragalactic Radio Sources
DOI: 10.1088/0004-637X/815/1/49 Bibcode: 2015ApJ...815...49A

Gaensler, B. M.; Franzen, T. M. O.; Anderson, C. S. +1 more

We present a broadband spectropolarimetric survey of 563 discrete, mostly unresolved radio sources between 1.3 and 2.0 GHz using data taken with the Australia Telescope Compact Array. We have used rotation-measure synthesis to identify Faraday-complex polarized sources, those objects whose frequency-dependent polarization behavior indicates the pr…

2015 The Astrophysical Journal
Planck 57
Non-local gravity and comparison with observational datasets
DOI: 10.1088/1475-7516/2015/04/044 Bibcode: 2015JCAP...04..044D

Kunz, Martin; Pettorino, Valeria; Dirian, Yves +2 more

We study the cosmological predictions of two recently proposed non-local modifications of General Relativity. Both models have the same number of parameters as ΛCDM, with a mass parameter m replacing the cosmological constant. We implement the cosmological perturbations of the non-local models into a modification of the CLASS Boltzmann code, and w…

2015 Journal of Cosmology and Astroparticle Physics
Planck 57
HST Rotational Spectral Mapping of Two L-type Brown Dwarfs: Variability in and out of Water Bands indicates High-altitude Haze Layers
DOI: 10.1088/2041-8205/798/1/L13 Bibcode: 2015ApJ...798L..13Y

Metchev, Stanimir; Showman, Adam P.; Apai, Dániel +13 more

We present time-resolved near-infrared spectroscopy of two L5 dwarfs, 2MASS J18212815+1414010 and 2MASS J15074759-1627386, observed with the Wide Field Camera 3 instrument on the Hubble Space Telescope (HST). We study the wavelength dependence of rotation-modulated flux variations between 1.1 µm and 1.7 µm. We find that the water absor…

2015 The Astrophysical Journal
eHST 57