Search Publications

The eccentricity distribution of wide binaries and their individual measurements
DOI: 10.1093/mnras/stac675 Bibcode: 2022MNRAS.512.3383H

Ting, Yuan-Sen; Zakamska, Nadia L.; Hwang, Hsiang-Chih

Eccentricity of wide binaries is difficult to measure due to their long orbital periods. With Gaia's high-precision astrometric measurements, eccentricity of a wide binary can be constrained by the angle between the separation vector and the relative velocity vector (the v-r angle). In this paper, by using the v-r angles of wide binaries in Gaia E…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 75
Analysis of Early Science observations with the CHaracterising ExOPlanets Satellite (CHEOPS) using PYCHEOPS
DOI: 10.1093/mnras/stab3371 Bibcode: 2022MNRAS.514...77M

Guterman, P.; Alonso, R.; Deleuil, M. +77 more

CHEOPS (CHaracterising ExOPlanet Satellite) is an ESA S-class mission that observes bright stars at high cadence from low-Earth orbit. The main aim of the mission is to characterize exoplanets that transit nearby stars using ultrahigh precision photometry. Here, we report the analysis of transits observed by CHEOPS during its Early Science observi…

2022 Monthly Notices of the Royal Astronomical Society
CHEOPS Gaia 72
The chemo-dynamical groups of Galactic globular clusters
DOI: 10.1093/mnras/stac1145 Bibcode: 2022MNRAS.513.4107C

Grand, Robert J. J.; Marinacci, Federico; Deason, Alis J. +3 more

We introduce a multicomponent chemo-dynamical method for splitting the Galactic population of globular clusters (GCs) into three distinct constituents: bulge, disc, and stellar halo. The latter is further decomposed into the individual large accretion events that built up the Galactic stellar halo: the Gaia-Enceladus-Sausage, Kraken and Sequoia st…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 72
Dual constraints with ALMA: new [O III] 88-µm and dust-continuum observations reveal the ISM conditions of luminous LBGs at z 7
DOI: 10.1093/mnras/stac1905 Bibcode: 2022MNRAS.515.1751W

Carniani, Stefano; Maiolino, Roberto; Jones, Gareth C. +10 more

We present new [${\rm O\, {\small III}}$] 88-$\mu \mathrm{{m}}$ observations of five bright z ~ 7 Lyman-break galaxies spectroscopically confirmed by ALMA through [${\rm C\, {\small II}}$] 158 $\mu \mathrm{{m}}$, unlike recent [${\rm O\, {\small III}}$] detections where Lyman α was used. This nearly doubles the sample of Epoch of Reionization gala…

2022 Monthly Notices of the Royal Astronomical Society
Gaia eHST 71
The star formation burstiness and ionizing efficiency of low-mass galaxies
DOI: 10.1093/mnras/stac360 Bibcode: 2022MNRAS.511.4464A

Contini, Thierry; van Dokkum, Pieter; Reddy, Naveen +5 more

We investigate the burstiness of star formation and the ionizing efficiency of a large sample of galaxies at 0.7 < z < 1.5 using HST grism spectroscopy and deep ultraviolet (UV) imaging in the GOODS-N and GOODS-S fields. The star formation history (SFH) in these strong emission-line low-mass galaxies indicates an elevated star formation rate…

2022 Monthly Notices of the Royal Astronomical Society
eHST 66
Dark Energy Survey Year 3 results: galaxy clustering and systematics treatment for lens galaxy samples
DOI: 10.1093/mnras/stac104 Bibcode: 2022MNRAS.511.2665R

Bacon, D.; Bechtol, K.; Smith, M. +103 more

In this work, we present the galaxy clustering measurements of the two DES lens galaxy samples: a magnitude-limited sample optimized for the measurement of cosmological parameters, MAGLIM, and a sample of luminous red galaxies selected with the REDMAGIC algorithm. MAGLIM/REDMAGIC sample contains over 10 million/2.5 million galaxies and is divided …

2022 Monthly Notices of the Royal Astronomical Society
Gaia 64
Measuring the Milky Way mass distribution in the presence of the LMC
DOI: 10.1093/mnras/stab3726 Bibcode: 2022MNRAS.511.2610C

Vasiliev, Eugene; Correa Magnus, Lilia

The ongoing interaction between the Milky Way (MW) and its largest satellite - the Large Magellanic Cloud (LMC) - creates a significant perturbation in the distribution and kinematics of distant halo stars, globular clusters and satellite galaxies, and leads to biases in MW mass estimates from these tracer populations. We present a method for comp…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 62
Continuum reverberation mapping and a new lag-luminosity relationship for AGN
DOI: 10.1093/mnras/stab3133 Bibcode: 2022MNRAS.509.2637N

Netzer, Hagai

High cadence, high quality observations of active galactic nuclei (AGN) clearly show continuum variations with lags, relative to the shortest observed variable UV continuum that increase with wavelength ('lag spectra'). These have been attributed to the irradiation and heating of the central accretion disc by the central X-ray emitting corona. An …

2022 Monthly Notices of the Royal Astronomical Society
eHST 62
Inferring the intergalactic medium neutral fraction at z 6-8 with low-luminosity Lyman break galaxies
DOI: 10.1093/mnras/stac1963 Bibcode: 2022MNRAS.517.3263B

Pentericci, Laura; Treu, Tommaso; Bradač, Maruša +6 more

We present a Bayesian inference on the neutral hydrogen fraction of the intergalactic medium (IGM), $\overline{x}_{\small HI}$, at z ~ 6-8 using the properties of Lyman break galaxies (LBGs) during the epoch of reionization. We use large samples of LBG candidates at 5.5 ≤ z ≤ 8.2 with spectroscopy from Keck/DEIMOS and Keck/MOSFIRE. For each galaxy…

2022 Monthly Notices of the Royal Astronomical Society
eHST 61
Dust, CO, and [C I]: cross-calibration of molecular gas mass tracers in metal-rich galaxies across cosmic time
DOI: 10.1093/mnras/stac2098 Bibcode: 2022MNRAS.517..962D

Ivison, R. J.; Dunne, L.; Gomez, H. L. +2 more

We present a self-consistent cross-calibration of the three main molecular gas mass tracers in galaxies, namely the 12CO(1-0), [C I](3P1-3P0) lines, and the submm dust continuum emission, using a sample of 407 galaxies, ranging from local discs to submillimetre-selected galaxies (SMGs) up to z…

2022 Monthly Notices of the Royal Astronomical Society
Herschel 60