Search Publications

The far-ultraviolet continuum slope as a Lyman Continuum escape estimator at high redshift
DOI: 10.1093/mnras/stac2874 Bibcode: 2022MNRAS.517.5104C

Chisholm, J.; Schaerer, D.; Marques-Chaves, R. +25 more

Most of the hydrogen in the intergalactic medium (IGM) was rapidly ionized at high redshifts. While observations have established that reionization occurred, observational constraints on the high-redshift ionizing emissivity remain elusive. Here, we present a new analysis of the Low-redshift Lyman Continuum Survey (LzLCS) and literature observatio…

2022 Monthly Notices of the Royal Astronomical Society
eHST 128
The synchrony of production and escape: half the bright Lyα emitters at z ≈ 2 have Lyman continuum escape fractions ≈50 per cent
DOI: 10.1093/mnras/stab3601 Bibcode: 2022MNRAS.510.4582N

Hayes, Matthew; Conroy, Charlie; Schaerer, Daniel +14 more

The ionizing photon escape fraction [Lyman continuum (LyC) fesc] of star-forming galaxies is the single greatest unknown in the reionization budget. Stochastic sightline effects prohibit the direct separation of LyC leakers from non-leakers at significant redshifts. Here we circumvent this uncertainty by inferring fesc using …

2022 Monthly Notices of the Royal Astronomical Society
eHST 119
The ALMA REBELS Survey: dust continuum detections at z > 6.5
DOI: 10.1093/mnras/stac1779 Bibcode: 2022MNRAS.515.3126I

Inami, Hanae; Nanayakkara, Themiya; Ferrara, Andrea +25 more

We report 18 dust continuum detections (≥3.3σ) at ~88 and 158 $\mu{\rm m}$ out of 49 ultraviolet (UV)-bright galaxies (MUV < -21.3 mag) at $z$ > 6.5, observed by the Cycle-7 Atacama Large Millimeter/submillimeter Array (ALMA) Large Program, Reionization-Era Bright Emission Line Survey (REBELS) and its pilot programs. This has more…

2022 Monthly Notices of the Royal Astronomical Society
Gaia eHST 106
A stringent upper limit on dark matter self-interaction cross-section from cluster strong lensing
DOI: 10.1093/mnras/stab3241 Bibcode: 2022MNRAS.510...54A

Andrade, Kevin E.; Fuson, Jackson; Gad-Nasr, Sophia +4 more

We analyse strongly lensed images in eight galaxy clusters to measure their dark matter density profiles in the radial region between 10 kpc and 150 kpc, and use this to constrain the self-interaction cross-section of dark matter (DM) particles. We infer the mass profiles of the central DM haloes, bright central galaxies, key member galaxies, and …

2022 Monthly Notices of the Royal Astronomical Society
eHST 84
Constraining the evolution of cataclysmic variables via the masses and accretion rates of their underlying white dwarfs
DOI: 10.1093/mnras/stab3449 Bibcode: 2022MNRAS.510.6110P

Reichart, D. E.; Knigge, C.; Gänsicke, B. T. +28 more

We report on the masses (MWD), effective temperatures ($\rm{T_\mathrm{eff}}$), and secular mean accretion rates ($\langle \dot{M} \rangle$) of 43 cataclysmic variable (CV) white dwarfs, 42 of which were obtained from the combined analysis of their Hubble Space Telescope ultraviolet data with the parallaxes provided by the Early Third Da…

2022 Monthly Notices of the Royal Astronomical Society
Gaia eHST 79
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
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
A black hole detected in the young massive LMC cluster NGC 1850
DOI: 10.1093/mnras/stab3159 Bibcode: 2022MNRAS.511.2914S

Dreizler, S.; Da Costa, G. S.; Cabrera-Ziri, I. +8 more

We report on the detection of a black hole (NGC 1850 BH1) in the ~100-Myr-old massive cluster NGC 1850 in the Large Magellanic Cloud. It is in a binary system with a main-sequence turn-off star (4.9 ± 0.4 M), which is starting to fill its Roche lobe and is becoming distorted. Using 17 epochs of Very Large Telescope/Multi-Unit Spectrosc…

2022 Monthly Notices of the Royal Astronomical Society
eHST 55