Search Publications

Giant galaxy growing from recycled gas: ALMA maps the circumgalactic molecular medium of the Spiderweb in [C I]
DOI: 10.1093/mnrasl/sly034 Bibcode: 2018MNRAS.477L..60E

Villar-Martín, M.; Dannerbauer, H.; Guillard, P. +9 more

The circumgalactic medium (CGM) of the massive Spiderweb Galaxy, a conglomerate of merging proto-cluster galaxies at z = 2.2, forms an enriched interface where feedback and recycling act on accreted gas. This is shown by observations of [C I], CO(1-0), and CO(4-3) performed with the Atacama Large Millimeter Array and Australia Telescope Compact Ar…

2018 Monthly Notices of the Royal Astronomical Society
eHST 67
Chasing passive galaxies in the early Universe: a critical analysis in CANDELS GOODS-South
DOI: 10.1093/mnras/stx2385 Bibcode: 2018MNRAS.473.2098M

Elbaz, D.; Ciesla, L.; Wang, T. +12 more

We search for passive galaxies at z > 3 in the GOODS-South field, using different techniques based on photometric data, and paying attention to develop methods that are sensitive to objects that have become passive shortly before the epoch of observation. We use CANDELS HST catalogues, ultra-deep Ks data and new IRAC photometry, performing spec…

2018 Monthly Notices of the Royal Astronomical Society
eHST 67
The R-Process Alliance: A Comprehensive Abundance Analysis of HD 222925, a Metal-poor Star with an Extreme R-process Enhancement of [Eu/H] = -0.14
DOI: 10.3847/1538-4357/aadd92 Bibcode: 2018ApJ...865..129R

Beers, Timothy C.; Placco, Vinicius M.; Hansen, Terese T. +4 more

We present a detailed abundance analysis of the bright (V = 9.02), metal-poor ([Fe/H] = -1.47 ± 0.08) field red horizontal-branch star HD 222925, which was observed as part of an ongoing survey by the R-Process Alliance. We calculate stellar parameters and derive abundances for 46 elements based on 901 lines examined in a high-resolution optical s…

2018 The Astrophysical Journal
Gaia 67
New ultra-cool and brown dwarf candidates in Gaia DR2
DOI: 10.1051/0004-6361/201834082 Bibcode: 2018A&A...619L...8R

Reylé, C.

Context. The second Gaia data release (Gaia DR2) contains high-precision positions, parallaxes, and proper motions for 1.3 billion sources. The resulting Hertzsprung-Russel diagram reveals fine structures throughout the mass range.
Aims: This paper aims to investigate the content of Gaia DR2 at the low-mass end and to characterize ultra-cool …

2018 Astronomy and Astrophysics
Gaia 66
The LEECH Exoplanet Imaging Survey: Limits on Planet Occurrence Rates under Conservative Assumptions
DOI: 10.3847/1538-3881/aaec00 Bibcode: 2018AJ....156..286S

Fortney, Jonathan J.; De Rosa, Robert J.; Weigelt, Gerd +33 more

We present the results of the largest L‧ (3.8 µm) direct imaging survey for exoplanets to date, the Large Binocular Telescope Interferometer Exozodi Exoplanet Common Hunt (LEECH). We observed 98 stars with spectral types from B to M. Cool planets emit a larger share of their flux in L‧ compared to shorter wavelengths, affording LEECH an adva…

2018 The Astronomical Journal
Gaia 66
Chemical interactions between Saturn's atmosphere and its rings
DOI: 10.1126/science.aat2382 Bibcode: 2018Sci...362.2382W

Kurth, W. S.; Mitchell, D. G.; Wahlund, J. -E. +25 more

The Pioneer and Voyager spacecraft made close-up measurements of Saturn's ionosphere and upper atmosphere in the 1970s and 1980s that suggested a chemical interaction between the rings and atmosphere. Exploring this interaction provides information on ring composition and the influence on Saturn's atmosphere from infalling material. The Cassini Io…

2018 Science
Cassini 66
Characteristics of Late-phase >100 MeV Gamma-Ray Emission in Solar Eruptive Events
DOI: 10.3847/1538-4357/aaebf7 Bibcode: 2018ApJ...869..182S

White, S. M.; Dennis, B. R.; Murphy, R. J. +5 more

We characterize and catalog 30 solar eruptive events observed by the Fermi Large Area Telescope (LAT) having late-phase >100 MeV γ-ray emission (LPGRE), identified 30 yr ago in what were called long-duration gamma-ray flares. We show that LPGRE is temporally and spectrally distinct from impulsive phase emission in these events. The spectra are …

2018 The Astrophysical Journal
INTEGRAL 66
BANYAN. XII. New Members of Nearby Young Associations from GAIA-Tycho Data
DOI: 10.3847/1538-4357/aac2b8 Bibcode: 2018ApJ...860...43G

Faherty, Jacqueline K.; Gagné, Jonathan; Doyon, René +2 more

We present a search for stellar members of young associations within 150 pc of the Sun, based on TGAS and an updated version of the BANYAN Σ software to determine Bayesian membership probabilities that includes Gaia-2MASS color-magnitude diagrams. We identify 32 new F0-M3-type bona fide members of the 10-200 Myr old Sco-Cen, Carina, Tucana-Horolog…

2018 The Astrophysical Journal
Gaia XMM-Newton 66
The Redshift Evolution of Rest-UV Spectroscopic Properties in Lyman-break Galaxies at z ∼ 2-4
DOI: 10.3847/1538-4357/aabfcf Bibcode: 2018ApJ...860...75D

Pettini, Max; Erb, Dawn K.; Shapley, Alice E. +8 more

We present the first comprehensive evolutionary analysis of the rest-frame UV spectroscopic properties of star-forming galaxies at z ∼ 2-4. We match samples at different redshifts in UV luminosity and stellar mass, and perform systematic measurements of spectral features and stellar population modeling. By creating composite spectra grouped accord…

2018 The Astrophysical Journal
eHST 66
The Distance of the Dark Matter Deficient Galaxy NGC 1052-DF2
DOI: 10.3847/2041-8213/aada4d Bibcode: 2018ApJ...864L..18V

van Dokkum, Pieter; Romanowsky, Aaron J.; Conroy, Charlie +2 more

We recently inferred that the galaxy NGC 1052-DF2 has little or no dark matter and a rich system of unusual globular clusters. We assumed that the galaxy is a satellite of the luminous elliptical galaxy NGC 1052 at ≈20 Mpc, on the basis of its surface brightness fluctuations (SBFs) distance of 19.0 ± 1.7 Mpc, its radial velocity of ≈1800 km s

2018 The Astrophysical Journal
eHST 66