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QUIJOTE scientific results - II. Polarisation measurements of the microwave emission in the Galactic molecular complexes W43 and W47 and supernova remnant W44
DOI: 10.1093/mnras/stw2503 Bibcode: 2017MNRAS.464.4107G

Lasenby, A.; Martínez-González, E.; Rebolo, R. +11 more

We present Q-U-I JOint TEnerife (QUIJOTE) intensity and polarisation maps at 10-20 GHz covering a region along the Galactic plane 24° ≲ l ≲ 45°, |b| ≲ 8°. These maps result from 210 h of data, have a sensitivity in polarisation of ≈40 µK beam-1 and an angular resolution of ≈1°. Our intensity data are crucial to confirm the presenc…

2017 Monthly Notices of the Royal Astronomical Society
Planck 61
The Gaia DR1 mass-radius relation for white dwarfs
DOI: 10.1093/mnras/stw2854 Bibcode: 2017MNRAS.465.2849T

Gänsicke, B. T.; Jordan, S.; Tremblay, P. -E. +9 more

The Gaia Data Release 1 (DR1) sample of white dwarf parallaxes is presented, including six directly observed degenerates and 46 white dwarfs in wide binaries. This data set is combined with spectroscopic atmospheric parameters to study the white dwarf mass-radius relationship (MRR). Gaia parallaxes and G magnitudes are used to derive model atmosph…

2017 Monthly Notices of the Royal Astronomical Society
Gaia eHST 61
The HST large programme on ω Centauri - I. Multiple stellar populations at the bottom of the main sequence probed in NIR-Optical
DOI: 10.1093/mnras/stx836 Bibcode: 2017MNRAS.469..800M

Apai, D.; Anderson, J.; Milone, A. P. +7 more

As part of a large investigation with Hubble Space Telescope to study the faintest stars within the globular cluster ω Centauri, in this work we present early results on the multiplicity of its main sequence (MS) stars, based on deep optical and near-infrared observations. By using appropriate colour-magnitude diagrams, we have identified, for the…

2017 Monthly Notices of the Royal Astronomical Society
eHST 61
Comparative analysis of Debrecen sunspot catalogues
DOI: 10.1093/mnras/stw2667 Bibcode: 2017MNRAS.465.1259G

Ludmány, A.; Baranyi, T.; Győri, L.

Sunspot area data are important for studying solar activity and its long-term variations. At the Debrecen Heliophysical Observatory, we compiled three sunspot catalogues: the Debrecen Photoheliographic Data (DPD), the SDO/HMI Debrecen Data (HMIDD) and the SOHO/MDI Debrecen Data. For comparison, we also compiled an additional sunspot catalogue, the…

2017 Monthly Notices of the Royal Astronomical Society
SOHO 61
Revealing the ultrafast outflow in IRAS 13224-3809 through spectral variability
DOI: 10.1093/mnras/stx945 Bibcode: 2017MNRAS.469.1553P

Fabian, A. C.; Reynolds, C. S.; Pinto, C. +6 more

We present an analysis of the long-term X-ray variability of the extreme narrow-line Seyfert 1 galaxy IRAS 13224-3809 using principal component analysis (PCA) and fractional excess variability (Fvar) spectra to identify model-independent spectral components. We identify a series of variability peaks in both the first PCA component and F…

2017 Monthly Notices of the Royal Astronomical Society
XMM-Newton 61
Nature of the absorbing gas associated with a galaxy group at z∼0.4
DOI: 10.1093/mnras/stw2444 Bibcode: 2017MNRAS.464.2053P

Pettini, Max; York, Donald G.; Husemann, Bernd +6 more

We present new Multi Unit Spectroscopic Explorer observations of quasar field Q2131-1207 with a log N(H I} = 19.50 ± 0.15 sub-damped Lyman α at zabs = 0.42980. We detect four galaxies at a redshift consistent with that of the absorber where only one was known before this study. Two of these are star-forming galaxies, while the ones furt…

2017 Monthly Notices of the Royal Astronomical Society
eHST 61
The metallicity of the intracluster medium over cosmic time: further evidence for early enrichment
DOI: 10.1093/mnras/stx2200 Bibcode: 2017MNRAS.472.2877M

Allen, Steven W.; Simionescu, Aurora; Werner, Norbert +4 more

We use Chandra X-ray data to measure the metallicity of the intracluster medium (ICM) in 245 massive galaxy clusters selected from X-ray and Sunyaev-Zel'dovich (SZ) effect surveys, spanning redshifts 0 < z < 1.2. Metallicities were measured in three different radial ranges, spanning cluster cores through their outskirts. We explore trends in…

2017 Monthly Notices of the Royal Astronomical Society
Planck 61
The Galaxy End Sequence
DOI: 10.1093/mnras/stw2875 Bibcode: 2017MNRAS.465.3125E

Smith, Matthew W. L.; Eales, Stephen; Ciesla, Laure +4 more

A common assumption is that galaxies fall in two distinct regions of a plot of specific star formation rate (SSFR) versus galaxy stellar mass: a star-forming galaxy main sequence (GMS) and a separate region of 'passive' or 'red and dead galaxies'. Starting from a volume-limited sample of nearby galaxies designed to contain most of the stellar mass…

2017 Monthly Notices of the Royal Astronomical Society
Herschel 61
A population of faint low surface brightness galaxies in the Perseus cluster core
DOI: 10.1093/mnras/stx1229 Bibcode: 2017MNRAS.470.1512W

Wittmann, Carolin; Kotulla, Ralf; Lisker, Thorsten +7 more

We present the detection of 89 low surface brightness (LSB), and thus low stellar density galaxy candidates in the Perseus cluster core, of the kind named 'ultra-diffuse galaxies', with mean effective V-band surface brightnesses 24.8-27.1 mag arcsec-2, total V-band magnitudes -11.8 to -15.5 mag, and half-light radii 0.7-4.1 kpc. The can…

2017 Monthly Notices of the Royal Astronomical Society
eHST 59
The Gaia ultracool dwarf sample - I. Known L and T dwarfs and the first Gaia data release
DOI: 10.1093/mnras/stx800 Bibcode: 2017MNRAS.469..401S

Caballero, J. A.; Sarro, L. M.; Marocco, F. +5 more

We identify and investigate known ultracool stars and brown dwarfs that are being observed or indirectly constrained by the Gaia mission. These objects will be the core of the Gaia ultracool dwarf sample composed of all dwarfs later than M7 that Gaia will provide direct or indirect information on. We match known L and T dwarfs to the Gaia first da…

2017 Monthly Notices of the Royal Astronomical Society
Gaia 59