Search Publications

Clusters of Primordial Black Holes
DOI: 10.1140/epjc/s10052-019-6741-4 Bibcode: 2019EPJC...79..246B

Belotsky, Konstantin M.; Dokuchaev, Vyacheslav I.; Eroshenko, Yury N. +7 more

The Primordial Black Holes (PBHs) are a well-established probe for new physics in the very early Universe. We discuss here the possibility of PBH agglomeration into clusters that may have several prominent observable features. The clusters can form due to closed domain walls appearance in the natural and hybrid inflation models whose subsequent ev…

2019 European Physical Journal C
INTEGRAL 187
Dark Energy Survey year 1 results: Constraints on extended cosmological models from galaxy clustering and weak lensing
DOI: 10.1103/PhysRevD.99.123505 Bibcode: 2019PhRvD..99l3505A

Bechtol, K.; Smith, M.; Nichol, R. C. +112 more

We present constraints on extensions of the minimal cosmological models dominated by dark matter and dark energy, Λ CDM and w CDM , by using a combined analysis of galaxy clustering and weak gravitational lensing from the first-year data of the Dark Energy Survey (DES Y1) in combination with external data. We consider four extensions of the minima…

2019 Physical Review D
eHST 187
Dynamical heating across the Milky Way disc using APOGEE and Gaia
DOI: 10.1093/mnras/stz1521 Bibcode: 2019MNRAS.489..176M

Bovy, Jo; Chaplin, William J.; Cunha, Katia +14 more

The kinematics of the Milky Way disc as a function of age are well measured at the solar radius, but have not been studied over a wider range of Galactocentric radii. Here, we measure the kinematics of mono-age, mono-[Fe/H] populations in the low and high [α/Fe] discs between 4 ≲ R ≲ 13 kpc and |z| ≲ 2 kpc using 65 719 stars in common between APOG…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 185
The Ophiuchus DIsc Survey Employing ALMA (ODISEA) - I: project description and continuum images at 28 au resolution
DOI: 10.1093/mnras/sty2653 Bibcode: 2019MNRAS.482..698C

Ansdell, Megan; Gonzalez-Ruilova, Camilo; Cieza, Lucas A. +20 more

We introduce the Ophiuchus DIsc Survey Employing ALMA (ODISEA), a project aiming to study the entire population of Spitzer-selected protoplanetary discs in the Ophiuchus Molecular Cloud (∼300 objects) from both millimetre continuum and CO isotopologues data. Here we present 1.3 mm/230 GHz continuum images of 147 targets at 0.2 arcsec (28 au) resol…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 185
Pulsating white dwarfs: new insights
DOI: 10.1007/s00159-019-0118-4 Bibcode: 2019A&ARv..27....7C

Kepler, S. O.; Córsico, Alejandro H.; Althaus, Leandro G. +1 more

Stars are extremely important astronomical objects that constitute the pillars on which the Universe is built, and as such, their study has gained increasing interest over the years. White dwarf stars are not the exception. Indeed, these stars constitute the final evolutionary stage for more than 95% of all stars. The Galactic population of white …

2019 Astronomy and Astrophysics Review
Gaia 185
A sub-Neptune exoplanet with a low-metallicity methane-depleted atmosphere and Mie-scattering clouds
DOI: 10.1038/s41550-019-0800-5 Bibcode: 2019NatAs...3..813B

Deming, Drake; Désert, Jean-Michel; Knutson, Heather A. +15 more

With no analogues in the Solar System, the discovery of thousands of exoplanets with masses and radii intermediate between Earth and Neptune was one of the big surprises of exoplanet science. These super-Earths and sub-Neptunes probably represent the most common outcome of planet formation1,2. Mass and radius measurements indicate a div…

2019 Nature Astronomy
eHST 185
Absence of a thick atmosphere on the terrestrial exoplanet LHS 3844b
DOI: 10.1038/s41586-019-1497-4 Bibcode: 2019Natur.573...87K

Deming, Drake; Vanderburg, Andrew; Stevenson, Kevin B. +16 more

Most known terrestrial planets orbit small stars with radii less than 60 per cent of that of the Sun1,2. Theoretical models predict that these planets are more vulnerable to atmospheric loss than their counterparts orbiting Sun-like stars3-6. To determine whether a thick atmosphere has survived on a small planet, one approach…

2019 Nature
Gaia 184
A wide star-black-hole binary system from radial-velocity measurements
DOI: 10.1038/s41586-019-1766-2 Bibcode: 2019Natur.575..618L

Soria, Roberto; Zhao, Gang; Wang, Wei +52 more

All stellar-mass black holes have hitherto been identified by X-rays emitted from gas that is accreting onto the black hole from a companion star. These systems are all binaries with a black-hole mass that is less than 30 times that of the Sun1-4. Theory predicts, however, that X-ray-emitting systems form a minority of the total populat…

2019 Nature
Gaia 184
Constraining the Neutral Fraction of Hydrogen in the IGM at Redshift 7.5
DOI: 10.3847/1538-4357/ab1de7 Bibcode: 2019ApJ...878...12H

Hoag, A.; Bradač, M.; Treu, T. +8 more

We present a large spectroscopic campaign with Keck/Multi-Object Spectrometer for InfraRed Exploration (MOSFIRE) targeting Lyα emission (Lyα) from intrinsically faint Lyman-break galaxies (LBGs) behind 12 efficient galaxy cluster lenses. Gravitational lensing allows us to probe the more abundant faint galaxy population to sensitive Lyα equivalent-…

2019 The Astrophysical Journal
eHST 184
RELICS: Reionization Lensing Cluster Survey
DOI: 10.3847/1538-4357/ab412b Bibcode: 2019ApJ...884...85C

Ouchi, Masami; Mahler, Guillaume; Frye, Brenda L. +54 more

Large surveys of galaxy clusters with the Hubble Space Telescope (HST) and Spitzer, including the Cluster Lensing And Supernova survey with Hubble and the Frontier Fields, have demonstrated the power of strong gravitational lensing to efficiently deliver large samples of high-redshift galaxies. We extend this strategy through a wider, shallower su…

2019 The Astrophysical Journal
eHST 183