Search Publications

The discovery of rest-frame UV colour gradients and a diversity of dust morphologies in bright z ≃ 7 Lyman-break galaxies
DOI: 10.1093/mnras/stab3744 Bibcode: 2022MNRAS.510.5088B

Bowler, R. A. A.; Cullen, F.; McLure, R. J. +2 more

We present deep ALMA dust continuum observations for a sample of luminous (MUV < -22) star-forming galaxies at z ≃ 7. We detect five of the six sources in the far-infrared (FIR), providing key constraints on the obscured star formation rate (SFR) and the infrared-excess-β (IRX-β) relation without the need for stacking. Despite the ga…

2022 Monthly Notices of the Royal Astronomical Society
eHST 50
Implications for galaxy formation models from observations of globular clusters around ultra-diffuse galaxies
DOI: 10.1093/mnras/stac328 Bibcode: 2022MNRAS.511.4633S

Beasley, Michael A.; Trujillo, Ignacio; Peletier, Reynier F. +5 more

We present an analysis of Hubble Space Telescope observations of globular clusters (GCs) in six ultradiffuse galaxies (UDGs) in the Coma cluster, a sample that represents UDGs with large effective radii (Re), and use the results to evaluate competing formation models. We eliminate two significant sources of systematic uncertainty in the…

2022 Monthly Notices of the Royal Astronomical Society
eHST 49
MHD disc winds can reproduce fast disc dispersal and the correlation between accretion rate and disc mass in Lupus
DOI: 10.1093/mnrasl/slab124 Bibcode: 2022MNRAS.512L..74T

Lodato, G.; van Dishoeck, E. F.; Tabone, B. +3 more

The final architecture of planetary systems depends on the extraction of angular momentum and mass-loss processes of the discs in which they form. Theoretical studies proposed that magnetohydrodynamic winds launched from the discs (MHD disc winds) could govern accretion and disc dispersal. In this work, we revisit the observed disc demographics in…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 49
A deep survey of short GRB host galaxies over z 0-2: implications for offsets, redshifts, and environments
DOI: 10.1093/mnras/stac1982 Bibcode: 2022MNRAS.515.4890O

Troja, E.; Cenko, S. B.; Sakamoto, T. +10 more

A significant fraction (30 per cent) of well-localized short gamma-ray bursts (sGRBs) lack a coincident host galaxy. This leads to two main scenarios: (i) that the progenitor system merged outside of the visible light of its host, or (ii) that the sGRB resided within a faint and distant galaxy that was not detected by follow-up observations. Discr…

2022 Monthly Notices of the Royal Astronomical Society
eHST 48
A 5 per cent measurement of the Hubble-Lemaître constant from Type II supernovae
DOI: 10.1093/mnras/stac1661 Bibcode: 2022MNRAS.514.4620D

Zheng, W.; Galbany, L.; Filippenko, A. V. +4 more

The most stringent local measurement of the Hubble-Lemaître constant from Cepheid-calibrated Type Ia supernovae (SNe Ia) differs from the value inferred via the cosmic microwave background radiation (Planck+ΛCDM) by ~5σ. This so-called Hubble tension has been confirmed by other independent methods, and thus does not appear to be a possible consequ…

2022 Monthly Notices of the Royal Astronomical Society
eHST 48
The effect of returning radiation on relativistic reflection
DOI: 10.1093/mnras/stac1593 Bibcode: 2022MNRAS.514.3965D

Reynolds, C. S.; Dauser, T.; Wilms, J. +5 more

We study the effect of returning radiation on the shape of the X-ray reflection spectrum in the case of thin accretion discs. We show that the returning radiation mainly influences the observed reflection spectrum for a large black hole spin (a > 0.9) and a compact primary source of radiation close to the black hole at height h < 5rg

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 48
The kinematic properties of Milky Way stellar halo populations
DOI: 10.1093/mnras/stab3755 Bibcode: 2022MNRAS.510.5119L

Bovy, Jo; Lane, James M. M.; Mackereth, J. Ted

In the Gaia era, stellar kinematics are extensively used to study Galactic halo stellar populations, to search for halo structures, and to characterize the interface between the halo and hot disc populations. We use distribution function-based models of modern data sets with 6D phase space data to qualitatively describe a variety of kinematic spac…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 47
A pair of sub-Neptunes transiting the bright K-dwarf TOI-1064 characterized with CHEOPS
DOI: 10.1093/mnras/stab3799 Bibcode: 2022MNRAS.511.1043W

Lester, Kathryn V.; Charnoz, Sébastien; Triaud, Amaury H. M. J. +132 more

We report the discovery and characterization of a pair of sub-Neptunes transiting the bright K-dwarf TOI-1064 (TIC 79748331), initially detected in the Transiting Exoplanet Survey Satellite (TESS) photometry. To characterize the system, we performed and retrieved the CHaracterising ExOPlanets Satellite (CHEOPS), TESS, and ground-based photometry, …

2022 Monthly Notices of the Royal Astronomical Society
CHEOPS Gaia 47
Being KLEVER at cosmic noon: Ionized gas outflows are inconspicuous in low-mass star-forming galaxies but prominent in massive AGN hosts
DOI: 10.1093/mnras/stac1026 Bibcode: 2022MNRAS.513.2535C

Maiolino, Roberto; Cresci, Giovanni; Jones, Gareth C. +13 more

We investigate the presence of ionized gas outflows in a sample of 141 main-sequence star-forming galaxies at 1.2 < z < 2.6 from the KLEVER (KMOS Lensed Emission Lines and VElocity Review) survey. Our sample covers an exceptionally wide range of stellar masses, 8.1 < log (M/M) < 11.3, pushing outflow studies int…

2022 Monthly Notices of the Royal Astronomical Society
eHST 47
Results from The COPAINS Pilot Survey: four new BDs and a high companion detection rate for accelerating stars
DOI: 10.1093/mnras/stac1250 Bibcode: 2022MNRAS.513.5588B

Sozzetti, A.; Scholz, A.; Desidera, S. +7 more

The last decade of direct imaging (DI) searches for sub-stellar companions has uncovered a widely diverse sample that challenges the current formation models, while highlighting the intrinsically low occurrence rate of wide companions, especially at the lower end of the mass distribution. These results clearly show how blind surveys, crucial to co…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 46