Search Publications

SPIDERMAN: an open-source code to model phase curves and secondary eclipses
DOI: 10.1093/mnras/sty558 Bibcode: 2018MNRAS.477.2613L

Kreidberg, Laura; Louden, Tom

We present SPIDERMAN (Secondary eclipse and Phase curve Integrator for 2D tempERature MAppiNg), a fast code for calculating exoplanet phase curves and secondary eclipses with arbitrary surface brightness distributions in two dimensions. Using a geometrical algorithm, the code solves exactly the area of sections of the disc of the planet that are o…

2018 Monthly Notices of the Royal Astronomical Society
eHST 40
Kinematics, turbulence, and star formation of z ∼ 1 strongly lensed galaxies seen with MUSE
DOI: 10.1093/mnras/sty555 Bibcode: 2018MNRAS.477...18P

Bauer, F. E.; Pelló, R.; Mahler, G. +18 more

We analyse a sample of eight highly magnified galaxies at redshift 0.6 < z < 1.5 observed with MUSE, exploring the resolved properties of these galaxies at sub-kiloparsec scales. Combining multiband HST photometry and MUSE spectra, we derive the stellar mass, global star formation rates (SFRs), extinction and metallicity from multiple nebula…

2018 Monthly Notices of the Royal Astronomical Society
eHST 40
Latest astronomical constraints on some non-linear parametric dark energy models
DOI: 10.1093/mnras/sty019 Bibcode: 2018MNRAS.475.2605Y

Yang, Weiqiang; Pan, Supriya; Paliathanasis, Andronikos

We consider non-linear redshift-dependent equation of state parameters as dark energy models in a spatially flat Friedmann-Lemaître-Robertson-Walker universe. To depict the expansion history of the universe in such cosmological scenarios, we take into account the large-scale behaviour of such parametric models and fit them using a set of latest ob…

2018 Monthly Notices of the Royal Astronomical Society
Planck 40
Debris disc constraints on planetesimal formation
DOI: 10.1093/mnras/stx2932 Bibcode: 2018MNRAS.474.2564K

Blum, Jürgen; Krivov, Alexander V.; Löhne, Torsten +2 more

Two basic routes for planetesimal formation have been proposed over the last decades. One is a classical `slow-growth' scenario. Another one is particle concentration models, in which small pebbles are concentrated locally and then collapse gravitationally to form planetesimals. Both types of models make certain predictions for the size spectrum a…

2018 Monthly Notices of the Royal Astronomical Society
Herschel 40
A free-form lensing model of A370 revealing stellar mass dominated BCGs, in Hubble Frontier Fields images
DOI: 10.1093/mnras/stx2609 Bibcode: 2018MNRAS.473.4279D

Schmidt, Kasper B.; Broadhurst, Tom; Zheng, Wei +9 more

We derive a free-form mass distribution for the unrelaxed cluster A370 (z = 0.375), using the first release of the Hubble Frontier Fields images (76 orbits) and GLASS spectroscopy. Starting from a reliable set of 10 multiply lensed systems, we produce a free-form lens model that identifies ≈80 multiple images. Good consistency is found between mod…

2018 Monthly Notices of the Royal Astronomical Society
eHST 40
JINGLE, a JCMT legacy survey of dust and gas for galaxy evolution studies - I. Survey overview and first results
DOI: 10.1093/mnras/sty2499 Bibcode: 2018MNRAS.481.3497S

Lamperti, Isabella; Saintonge, Amélie; Ho, Luis C. +88 more

JINGLE is a new JCMT legacy survey designed to systematically study the cold interstellar medium of galaxies in the local Universe. As part of the survey we perform 850 µm continuum measurements with SCUBA-2 for a representative sample of 193 Herschel-selected galaxies with M* > 109 M, as well as integrated CO(…

2018 Monthly Notices of the Royal Astronomical Society
Herschel 39
Magnetism, X-rays and accretion rates in WD 1145+017 and other polluted white dwarf systems
DOI: 10.1093/mnras/stx2664 Bibcode: 2018MNRAS.474..947F

Gänsicke, B. T.; Fossati, L.; Redfield, S. +9 more

This paper reports circular spectropolarimetry and X-ray observations of several polluted white dwarfs including WD 1145+017, with the aim to constrain the behaviour of disc material and instantaneous accretion rates in these evolved planetary systems. Two stars with previously observed Zeeman splitting, WD 0322-019 and WD 2105-820, are detected a…

2018 Monthly Notices of the Royal Astronomical Society
XMM-Newton 39
The stellar population and initial mass function of NGC 1399 with MUSE
DOI: 10.1093/mnras/sty1434 Bibcode: 2018MNRAS.479.2443V

Davies, Roger L.; Houghton, Ryan C. W.; Vaughan, Sam P. +1 more

We present spatially resolved measurements of the stellar initial mass function (IMF) in NGC 1399, the largest elliptical galaxy in the Fornax Cluster. Using data from the Multi Unit Spectroscopic Explorer (MUSE) and updated state-of-the-art stellar population synthesis models from Conroy et al., we use full spectral fitting to measure the low-mas…

2018 Monthly Notices of the Royal Astronomical Society
eHST 39
Discovery of synchronous X-ray and radio moding of PSR B0823+26
DOI: 10.1093/mnras/sty2075 Bibcode: 2018MNRAS.480.3655H

Tiburzi, C.; Grießmeier, J. -M.; Serylak, M. +10 more

Simultaneous observations of PSR B0823+26 with ESA's XMM-Newton, the Giant Metrewave Radio Telescope and international stations of the Low Frequency Array revealed synchronous X-ray/radio switching between a radio-bright (B) mode and a radio-quiet (Q) mode. During the B mode we detected PSR B0823+26 in 0.2 - 2 keV X-rays and discovered pulsed emis…

2018 Monthly Notices of the Royal Astronomical Society
XMM-Newton 39
A likely planet-induced gap in the disc around T Cha
DOI: 10.1093/mnrasl/slx184 Bibcode: 2018MNRAS.475L..62H

Pascucci, Ilaria; Henning, Thomas; Dong, Ruobing +7 more

We present high-resolution (0.11 × 0.06 arcsec2) 3 mm ALMA observations of the highly inclined transition disc around the star T Cha. Our continuum image reveals multiple dust structures: an inner disc, a spatially resolved dust gap, and an outer ring. When fitting sky-brightness models to the real component of the 3 mm visibilities, we…

2018 Monthly Notices of the Royal Astronomical Society
Gaia 39