Search Publications

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
A multimission catalogue of ultraluminous X-ray source candidates
DOI: 10.1093/mnras/stab3001 Bibcode: 2022MNRAS.509.1587W

Earnshaw, H. P.; Roberts, T. P.; Mateos, S. +4 more

We present a new, multimission catalogue of ultraluminous X-ray source (ULX) candidates, based on recent data releases from each of the XMM-Newton, Swift, and Chandra observatories (the 4XMM-DR10, 2SXPS, and CSC2 catalogues, respectively). This has been compiled by cross-correlating each of these X-ray archives with a large sample of galaxies prim…

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 59
Do quasar X-ray and UV flux measurements provide a useful test of cosmological models?
DOI: 10.1093/mnras/stab3678 Bibcode: 2022MNRAS.510.2753K

Khadka, Narayan; Ratra, Bharat

The recent compilation of quasar (QSO) X-ray and ultraviolet (UV) flux measurements include QSOs that appear to not be standardizable via the X-ray luminosity and UV luminosity (LX-LUV) relation and so should not be used to constrain cosmological model parameters. Here, we show that the largest of seven sub-samples in this co…

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 58
All-purpose, all-sky photometric redshifts for the Legacy Imaging Surveys Data Release 8
DOI: 10.1093/mnras/stac608 Bibcode: 2022MNRAS.512.3662D

Duncan, Kenneth J.

In this paper, we present photometric redshift (photo-z) estimates for the Dark Energy Spectroscopic Instrument (DESI) Legacy Imaging Surveys, currently the most sensitive optical survey covering the majority of the extragalactic sky. Our photo-z methodology is based on a machine-learning approach, using sparse Gaussian processes augmented with Ga…

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 56