Search Publications

Dust in the Reionization Era: ALMA Observations of a z = 8.38 Gravitationally Lensed Galaxy
DOI: 10.3847/2041-8213/aa62aa Bibcode: 2017ApJ...837L..21L

Pérez-Fournon, I.; Laporte, N.; Bauer, F. E. +6 more

We report on the detailed analysis of a gravitationally lensed Y-band dropout, A2744_YD4, selected from deep Hubble Space Telescope imaging in the Frontier Field cluster Abell 2744. Band 7 observations with the Atacama Large Millimeter/submillimeter Array (ALMA) indicate the proximate detection of a significant 1 mm continuum flux suggesting the p…

2017 The Astrophysical Journal
Gaia eHST 292
Global constraints on absolute neutrino masses and their ordering
DOI: 10.1103/PhysRevD.95.096014 Bibcode: 2017PhRvD..95i6014C

Di Valentino, Eleonora; Melchiorri, Alessandro; Capozzi, Francesco +3 more

Within the standard three-neutrino framework, the absolute neutrino masses and their ordering (either normal, NO, or inverted, IO) are currently unknown. However, the combination of current data coming from oscillation experiments, neutrinoless double beta (0 ν β β ) decay searches, and cosmological surveys, can provide interesting constraints for…

2017 Physical Review D
Planck 285
Standing on the Shoulders of Dwarfs: the Kepler Asteroseismic LEGACY Sample. II.Radii, Masses, and Ages
DOI: 10.3847/1538-4357/835/2/173 Bibcode: 2017ApJ...835..173S

Chaplin, William J.; Davies, Guy R.; Latham, David W. +21 more

We use asteroseismic data from the Kepler satellite to determine fundamental stellar properties of the 66 main-sequence targets observed for at least one full year by the mission. We distributed tens of individual oscillation frequencies extracted from the time series of each star among seven modeling teams who applied different methods to determi…

2017 The Astrophysical Journal
Gaia 261
The z ∼ 6 Luminosity Function Fainter than -15 mag from the Hubble Frontier Fields: The Impact of Magnification Uncertainties
DOI: 10.3847/1538-4357/aa70a4 Bibcode: 2017ApJ...843..129B

Oesch, P. A.; Bouwens, R. J.; Illingworth, G. D. +2 more

We use the largest sample of z∼ 6 galaxies to date from the first four Hubble Frontier Fields clusters to set constraints on the shape of the z∼ 6 luminosity functions (LFs) to fainter than {M}{UV,{AB}}=-14 mag. We quantify, for the first time, the impact of magnification uncertainties on LF results and thus provide more realistic const…

2017 The Astrophysical Journal
eHST 251
Structural and Star-forming Relations since z ∼ 3: Connecting Compact Star-forming and Quiescent Galaxies
DOI: 10.3847/1538-4357/aa6b05 Bibcode: 2017ApJ...840...47B

Barro, Guillermo; Pérez-González, Pablo G.; Kocevski, Dale D. +13 more

We study the evolution of the scaling relations that compare the effective density ({{{Σ }}}{{e}},r< {r}{{e}}) and core density ({{{Σ }}}1,r< 1 kpc) to the stellar masses of star-forming galaxies (SFGs) and quiescent galaxies. These relations have been fully in place since z∼ 3 and have exhibited almost const…

2017 The Astrophysical Journal
eHST 249
Three-dimensional mapping of the local interstellar medium with composite data
DOI: 10.1051/0004-6361/201730831 Bibcode: 2017A&A...606A..65C

Monreal-Ibero, A.; Elyajouri, M.; Lallement, R. +2 more

Context. Three-dimensional maps of the Galactic interstellar medium are general astrophysical tools. Reddening maps may be based on the inversion of color excess measurements for individual target stars or on statistical methods using stellar surveys. Three-dimensional maps based on diffuse interstellar bands (DIBs) have also been produced. All me…

2017 Astronomy and Astrophysics
Gaia Hipparcos 249
Precision Stellar Characterization of FGKM Stars using an Empirical Spectral Library
DOI: 10.3847/1538-4357/836/1/77 Bibcode: 2017ApJ...836...77Y

Petigura, Erik A.; von Braun, Kaspar; Yee, Samuel W.

Classification of stars, by comparing their optical spectra to a few dozen spectral standards, has been a workhorse of observational astronomy for more than a century. Here, we extend this technique by compiling a library of optical spectra of 404 touchstone stars observed with Keck/HIRES by the California Planet Search. The spectra have high reso…

2017 The Astrophysical Journal
Gaia 248
The COS-Halos Survey: Metallicities in the Low-redshift Circumgalactic Medium
DOI: 10.3847/1538-4357/aa6007 Bibcode: 2017ApJ...837..169P

Tripp, Todd M.; Worseck, Gábor; Prochaska, J. Xavier +8 more

We analyze new far-ultraviolet spectra of 13 quasars from the z∼ 0.2 COS-Halos survey that cover the H I Lyman limit of 14 circumgalactic medium (CGM) systems. These data yield precise estimates or more constraining limits than previous COS-Halos measurements on the H I column densities {N}{{H}{{I}}}. We then apply a Monte-Carlo Markov …

2017 The Astrophysical Journal
eHST 245
CMB bounds on disk-accreting massive primordial black holes
DOI: 10.1103/PhysRevD.96.083524 Bibcode: 2017PhRvD..96h3524P

Calore, Francesca; Kohri, Kazunori; Poulin, Vivian +2 more

Stellar-mass primordial black holes (PBH) have been recently reconsidered as a dark matter (DM) candidate after the aLIGO discovery of several binary black hole (BH) mergers with masses of tens of M . Matter accretion on such massive objects leads to the emission of high-energy photons, capable of altering the ionization and thermal hi…

2017 Physical Review D
Planck 244
Electromagnetic evidence that SSS17a is the result of a binary neutron star merger
DOI: 10.1126/science.aaq0073 Bibcode: 2017Sci...358.1583K

Rest, A.; Foley, R. J.; Boutsia, K. +18 more

Eleven hours after the detection of gravitational wave source GW170817 by the Laser Interferometer Gravitational-Wave Observatory and Virgo Interferometers, an associated optical transient, SSS17a, was identified in the galaxy NGC 4993. Although the gravitational wave data indicate that GW170817 is consistent with the merger of two compact objects…

2017 Science
eHST 243