Search Publications

L-GALAXIES 2020: The evolution of radial metallicity profiles and global metallicities in disc galaxies
DOI: 10.1093/mnras/stab741 Bibcode: 2021MNRAS.503.4474Y

White, Simon D. M.; Yates, Robert M.; Henriques, Bruno M. B. +5 more

We present a modified version of the L-GALAXIES2020 semi-analytic model of galaxy evolution, which includes significantly increased direct metal enrichment of the circumgalactic medium (CGM) by supernovae (SNe). These more metal-rich outflows do not require increased mass-loading factors, in contrast to some other galaxy evolution models. This mod…

2021 Monthly Notices of the Royal Astronomical Society
eHST 53
An inventory of atomic species in the atmosphere of WASP-121b using UVES high-resolution spectroscopy
DOI: 10.1093/mnras/stab1878 Bibcode: 2021MNRAS.506.3853M

Nikolov, Nikolay; de Mooij, Ernst J. W.; Gibson, Neale P. +8 more

Ultrahot Jupiters (UHJs) present excellent targets for atmospheric characterization. Their hot dayside temperatures (T ≳ 2200 K) strongly suppress the formation of condensates, leading to clear and highly inflated atmospheres extremely conducive to transmission spectroscopy. Recent studies using optical high-resolution spectra have discovered a pl…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 52
ZZ Piscis Austrinus (ZZ PsA): a bright red nova progenitor and the instability mass ratio of contact binary stars
DOI: 10.1093/mnras/staa3637 Bibcode: 2021MNRAS.501..229W

Filipović, Miroslav D.; Tothill, N. F. H.; Wadhwa, Surjit S. +4 more

ZZ Piscis Austrinus (ZZ PsA) is a neglected bright southern contact binary system with maximum V magnitude of 9.26. We present the first multiband photometric analysis and find the system to be in deep contact (>95 per cent) with an extremely low mass ratio of 0.078. The primary has a mass of 1.213 M in keeping with its reported spe…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 52
The PAU Survey: an improved photo-z sample in the COSMOS field
DOI: 10.1093/mnras/staa3659 Bibcode: 2021MNRAS.501.6103A

Alarcon, Alex; Carretero, Jorge; Castander, Francisco J. +21 more

We present - and make publicly available - accurate and precise photometric redshifts in the ACS footprint from the COSMOS field for objects with iAB ≤ 23. The redshifts are computed using a combination of narrow-band photometry from PAUS, a survey with 40 narrow bands spaced at $100\,\mathring{\rm A}$ intervals covering the range from …

2021 Monthly Notices of the Royal Astronomical Society
Gaia 52
A precise asteroseismic age and metallicity for HD 139614: a pre-main-sequence star with a protoplanetary disc in Upper Centaurus-Lupus
DOI: 10.1093/mnras/stab144 Bibcode: 2021MNRAS.502.1633M

Bedding, Timothy R.; White, Timothy R.; Murphy, Simon J. +2 more

HD 139614 is known to be a ∼14-Myr-old, possibly pre-main-sequence star in the Sco-Cen OB association in the Upper Centaurus-Lupus subgroup, with a slightly warped circumstellar disc containing ring structures hinting at one or more planets. The star's chemical abundance pattern is metal-deficient except for volatile elements, which places it in t…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 51
Mock light-cones and theory friendly catalogues for the CANDELS survey
DOI: 10.1093/mnras/stab231 Bibcode: 2021MNRAS.502.4858S

Ferguson, Henry C.; Somerville, Rachel S.; Yung, L. Y. Aaron +9 more

We present mock catalogues created to support the interpretation of the Cosmic Assembly Near-IR Deep Extragalactic Legacy Survey (CANDELS). We extract haloes along past light-cones from the Bolshoi Planck dissipationless N-body simulations and populate these haloes with galaxies using two different independently developed semi-analytic models of g…

2021 Monthly Notices of the Royal Astronomical Society
eHST 50
The number of globular clusters around the iconic UDG DF44 is as expected for dwarf galaxies
DOI: 10.1093/mnras/staa3016 Bibcode: 2021MNRAS.502.5921S

Beasley, Michael A.; Trujillo, Ignacio; Peletier, Reynier F. +2 more

There is a growing consensus that the vast majority of ultradiffuse galaxies (UDGs) are dwarf galaxies. However, there remain a few UDGs that seem to be special in terms of their globular cluster (GC) systems. In particular, according to some authors, certain UDGs exhibit large GC populations when compared to expectations from their stellar (or to…

2021 Monthly Notices of the Royal Astronomical Society
eHST 50
A constraint on light primordial black holes from the interstellar medium temperature
DOI: 10.1093/mnras/stab1222 Bibcode: 2021MNRAS.504.5475K

Kim, Hyungjin

Primordial black holes are a viable dark matter candidate. They decay via Hawking evaporation. Energetic particles from the Hawking radiation interact with interstellar gas, depositing their energy as heat and ionization. For a sufficiently high Hawking temperature, fast electrons produced by black holes deposit a substantial fraction of energy as…

2021 Monthly Notices of the Royal Astronomical Society
INTEGRAL 50
Structure and morphology of the MATLAS dwarf galaxies and their central nuclei
DOI: 10.1093/mnras/stab2092 Bibcode: 2021MNRAS.506.5494P

Müller, Oliver; Duc, Pierre-Alain; Lim, Sungsoon +10 more

We present a photometric study of the dwarf galaxy population in the low to moderate density environments of the MATLAS (Mass Assembly of early-Type gaLAxies with their fine Structures) deep imaging survey. The sample consists of 2210 dwarfs, including 508 nucleated. We define a nucleus as a compact source that is close to the galaxy photocentre (…

2021 Monthly Notices of the Royal Astronomical Society
Gaia eHST 50
The growth of intracluster light in XCS-HSC galaxy clusters from 0.1 < z < 0.5
DOI: 10.1093/mnras/stab065 Bibcode: 2021MNRAS.502.2419F

Baldry, Ivan K.; Kelvin, Lee S.; Stott, John P. +14 more

We estimate the intracluster light (ICL) component within a sample of 18 clusters detected in the XMM Cluster Survey (XCS) data using the deep (~26.8 mag) Hyper Suprime-Cam Subaru Strategic Programme data release 1 i-band data. We apply a rest-frame µB = 25 mag arcsec-2 isophotal threshold to our clusters, below which w…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 50