Search Publications

WISDOM project - V. Resolving molecular gas in Keplerian rotation around the supermassive black hole in NGC 0383
DOI: 10.1093/mnras/stz2598 Bibcode: 2019MNRAS.490..319N

Williams, Thomas G.; Sarzi, Marc; Cappellari, Michele +7 more

As part of the mm-Wave Interferometric Survey of Dark Object Masses (WISDOM), we present a measurement of the mass of the supermassive black hole (SMBH) in the nearby early-type galaxy NGC 0383 (radio source 3C 031). This measurement is based on Atacama Large Millimeter/sub-millimeter Array (ALMA) cycle 4 and 5 observations of the 12CO(…

2019 Monthly Notices of the Royal Astronomical Society
eHST 43
Dramatic spectral transition of X-ray pulsar GX 304-1 in low luminous state
DOI: 10.1093/mnrasl/sly236 Bibcode: 2019MNRAS.483L.144T

Doroshenko, Victor; Tsygankov, Sergey S.; Mushtukov, Alexander A. +5 more

We report on the discovery of a dramatic change in the energy spectrum of the X-ray pulsar GX 304-1 appearing at low luminosity. Particularly, we found that the cut-off power-law spectrum typical for accreting pulsars, including GX 304-1 at higher luminosities of LX ∼ 1036-1037 erg s-1, transformed at lo…

2019 Monthly Notices of the Royal Astronomical Society
INTEGRAL 43
Torus model properties of an ultra-hard X-ray selected sample of Seyfert galaxies
DOI: 10.1093/mnras/stz1003 Bibcode: 2019MNRAS.486.4917G

Hernán-Caballero, A.; Carrera, F. J.; Acosta-Pulido, J. A. +15 more

We characterize for the first time the torus properties of an ultra-hard X-ray (14-195 keV) volume-limited (DL < 40 Mpc) sample of 24 Seyfert (Sy) galaxies (BCS40 sample). The sample was selected from the Swift/BAT nine-month catalogue. We use high angular resolution nuclear infrared (IR) photometry and N-band spectroscopy…

2019 Monthly Notices of the Royal Astronomical Society
eHST 43
Masses and radii for the three super-Earths orbiting GJ 9827, and implications for the composition of small exoplanets
DOI: 10.1093/mnras/stz130 Bibcode: 2019MNRAS.484.3731R

Bouchy, F.; Vanderburg, A.; Poretti, E. +34 more

Super-Earths belong to a class of planet not found in the Solar system, but which appear common in the Galaxy. Given that some super-Earths are rocky, while others retain substantial atmospheres, their study can provide clues as to the formation of both rocky and gaseous planets, and - in particular - they can help to constrain the role of photoev…

2019 Monthly Notices of the Royal Astronomical Society
Gaia Hipparcos 42
Cosmological test using the Hubble diagram of high-z quasars
DOI: 10.1093/mnras/stz2120 Bibcode: 2019MNRAS.489..517M

Melia, Fulvio

It has been known for over three decades that the monochromatic X-ray and UV luminosities in quasars are correlated, though non-linearly. This offers the possibility of using high-z quasars as standard candles for cosmological testing. In this paper, we use a recently assembled, high-quality catalogue of 1598 quasars extending all the way to redsh…

2019 Monthly Notices of the Royal Astronomical Society
XMM-Newton 42
Machine-learning approaches to exoplanet transit detection and candidate validation in wide-field ground-based surveys
DOI: 10.1093/mnras/sty3146 Bibcode: 2019MNRAS.483.5534S

Bouchy, F.; Queloz, D.; Boumis, P. +23 more

Since the start of the Wide-angle Search for Planets (WASP) program, more than 160 transiting exoplanets have been discovered in the WASP data. In the past, possible transit-like events identified by the WASP pipeline have been vetted by human inspection to eliminate false alarms and obvious false positives. The goal of this paper is to assess the…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 42
Anisotropy of the Universe via the Pantheon supernovae sample revisited
DOI: 10.1093/mnras/stz1259 Bibcode: 2019MNRAS.486.5679Z

Zhao, Dong; Chang, Zhe; Zhou, Yong

We employ the hemisphere comparison (HC) method and the dipole fitting (DF) method to investigate the cosmic anisotropy in the recently released Pantheon sample of type Ia supernovae (SNe Ia) and five combinations among Pantheon. For the HC method, we find that the maximum anisotropy level in the full Pantheon sample is ALmax = 0.361 ± …

2019 Monthly Notices of the Royal Astronomical Society
eHST 42
The dust content of the Crab Nebula
DOI: 10.1093/mnras/stz1533 Bibcode: 2019MNRAS.488..164D

De Looze, I.; Gomez, H. L.; Barlow, M. J. +7 more

We have modelled the near-infrared to radio images of the Crab Nebula with a Bayesian SED model to simultaneously fit its synchrotron, interstellar (IS), and supernova dust emission. We infer an IS dust extinction map with an average AV = 1.08 ± 0.38 mag, consistent with a small contribution ({≲ }22{{ per cent}}) to the Crab's overall i…

2019 Monthly Notices of the Royal Astronomical Society
Herschel 42
More than just a wrinkle: a wave-like pattern in Ug versus Lz from Gaia data
DOI: 10.1093/mnras/stz2951 Bibcode: 2019MNRAS.490.5414F

Schönrich, Ralph; Friske, Jennifer K. S.

We present a newly found wave-like pattern in mean Galactocentric radial velocity {\overline{U}_ g} versus guiding centre radius Rg or angular momentum Lz of stars in the RV subsample of Gaia DR2. The short-wave pattern has a wavelength of order 1.2 kpc in Rg or 285 kpc km s^{-1} in Lz. The pattern shows…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 42
Star formation at the edge of the Local Group: a rising star formation history in the isolated galaxy WLM
DOI: 10.1093/mnras/stz2903 Bibcode: 2019MNRAS.490.5538A

Dolphin, Andrew E.; Skillman, Evan D.; Williams, Benjamin F. +11 more

We present the star formation history (SFH) of the isolated (D ∼ 970 kpc) Local Group dwarf galaxy Wolf-Lundmark-Melotte (WLM) measured from colour-magnitude diagrams (CMDs) constructed from deep Hubble Space Telescope imaging. Our observations include a central (0.5 r_h) and outer field (0.7 r_h) that reach below the oldest main-sequence turn-off…

2019 Monthly Notices of the Royal Astronomical Society
eHST 42