Search Publications

Resolving on 100 pc scales the UV-continuum in Lyman-α emitters between redshift 2 and 3 with gravitational lensing
DOI: 10.1093/mnras/sty2833 Bibcode: 2019MNRAS.482.4744R

Vegetti, S.; McKean, J. P.; Auger, M. W. +1 more

We present a study of 17 LAEs at redshift 2 < z < 3 gravitationally lensed by massive early-type galaxies (ETGs) at a mean redshift of approximately 0.5. Using a fully Bayesian grid-based technique, we model the gravitational lens mass distributions with elliptical power-law profiles and reconstruct the ultraviolet (UV)-continuum surface-bri…

2019 Monthly Notices of the Royal Astronomical Society
eHST 34
Hint of curvature in the orbital motion of the exoplanet 51 Eridani b using 3 yr of VLT/SPHERE monitoring
DOI: 10.1051/0004-6361/201935031 Bibcode: 2019A&A...624A.118M

Rouan, D.; Ménard, F.; Avenhaus, H. +49 more

Context. The 51 Eridani system harbors a complex architecture with its primary star forming a hierarchical system with the binary GJ 3305AB at a projected separation of 2000 au, a giant planet orbiting the primary star at 13 au, and a low-mass debris disk around the primary star with possible cold and warm components inferred from the spectral ene…

2019 Astronomy and Astrophysics
Gaia 34
The spectral energy distributions of active galactic nuclei
DOI: 10.1093/mnras/stz2324 Bibcode: 2019MNRAS.489.3351B

Salvato, M.; Ricci, C.; Brown, M. J. I. +5 more

We present spectral energy distributions (SEDs) of 41 active galactic nuclei, derived from multiwavelength photometry and archival spectroscopy. All of the SEDs span at least 0.09 to 30 µm, but in some instances wavelength coverage extends into the X-ray, far-infrared, and radio. For some active galactic nuclei (AGNs) we have fitted the meas…

2019 Monthly Notices of the Royal Astronomical Society
AKARI ISO IUE XMM-Newton eHST 34
Transient Inverse-FIP Plasma Composition Evolution within a Solar Flare
DOI: 10.3847/1538-4357/ab07c1 Bibcode: 2019ApJ...875...35B

Long, David M.; Matthews, Sarah A.; Brooks, David H. +9 more

Understanding elemental abundance variations in the solar corona provides an insight into how matter and energy flow from the chromosphere into the heliosphere. Observed variations depend on the first ionization potential (FIP) of the main elements of the Sun’s atmosphere. High-FIP elements (>10 eV) maintain photospheric abundances in the coron…

2019 The Astrophysical Journal
Hinode 34
The Milky Way Project second data release: bubbles and bow shocks
DOI: 10.1093/mnras/stz1738 Bibcode: 2019MNRAS.488.1141J

Kobulnicky, Henry A.; Kendrew, Sarah; Xu, Duo +9 more

Citizen science has helped astronomers comb through large data sets to identify patterns and objects that are not easily found through automated processes. The Milky Way Project (MWP), a citizen science initiative on the Zooniverse platform, presents internet users with infrared (IR) images from Spitzer Space Telescope Galactic plane surveys. MWP …

2019 Monthly Notices of the Royal Astronomical Society
Gaia Herschel 34
Primeval very low-mass stars and brown dwarfs - VI. Population properties of metal-poor degenerate brown dwarfs
DOI: 10.1093/mnras/stz777 Bibcode: 2019MNRAS.486.1260Z

Zapatero Osorio, M. R.; Pinfield, D. J.; Burgasser, A. J. +4 more

We presented 15 new T dwarfs that were selected from UKIRT Infrared Deep Sky Survey, Visible and Infrared Survey Telescope for Astronomy , and Wide-field Infrared Survey Explorer surveys, and confirmed with optical to near-infrared spectra obtained with the Very Large Telescope and the Gran Telescopio Canarias. One of these new T dwarfs is mildly …

2019 Monthly Notices of the Royal Astronomical Society
Gaia 34
The Second LBA Calibrator Survey of southern compact extragalactic radio sources - LCS2
DOI: 10.1093/mnras/stz242 Bibcode: 2019MNRAS.485...88P

Horiuchi, Shinji; Petrov, Leonid; de Witt, Alet +2 more

We present the second catalogue of accurate positions and correlated flux densities for 1100 compact extragalactic radio sources that were not observed before 2008 at high angular resolution. The catalogue spans the declination range [ -90°, -30°] and was constructed from 19 24-h VLBI observing sessions with the Australian Long Baseline Array at 8…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 34
On a New Method to Estimate the Distance, Reddening, and Metallicity of RR Lyrae Stars Using Optical/Near-infrared (B, V, I, J, H, K) Mean Magnitudes: ω Centauri as a First Test Case
DOI: 10.3847/1538-4357/aaf23f Bibcode: 2019ApJ...870..115B

Walker, A. R.; Mateo, M.; Valenti, E. +26 more

We developed a new approach to provide accurate estimates of the metal content, reddening, and true distance modulus of RR Lyrae stars (RRLs). The method is based on homogeneous optical (BVI) and near-infrared (JHK) mean magnitudes and on predicted period-luminosity-metallicity relations (IJHK) and absolute mean magnitude-metallicity relations (BV…

2019 The Astrophysical Journal
Gaia 34
Anchor Point of Electron Acceleration around Dipolarization Fronts in Space Plasmas
DOI: 10.3847/2041-8213/ab06cb Bibcode: 2019ApJ...873L...2L

Fu, H. S.; Liu, C. M.

An anchor point, which is an energy threshold above which electrons are accelerated and below which electrons are decelerated, has recently been reported within the dipolarizing flux bundles behind dipolarization fronts (DFs) both in observations and simulations. However, what determines this point and how it is formed remain unclear. In this stud…

2019 The Astrophysical Journal
Cluster 34
Galaxy Merger Fractions in Two Clusters at z\sim 2 Using the Hubble Space Telescope
DOI: 10.3847/1538-4357/ab06ef Bibcode: 2019ApJ...874...63W

Papovich, Casey; van Dokkum, Pieter; Momcheva, Ivelina +9 more

We measure the fraction of galaxy-galaxy mergers in two clusters at z ∼ 2 using imaging and grism observations from the Hubble Space Telescope. The two galaxy cluster candidates were originally identified as overdensities of objects using deep mid-infrared imaging and observations from the Spitzer Space Telescope, and were subsequently followed up…

2019 The Astrophysical Journal
eHST 34