Search Publications

GRB 190114C in the nuclear region of an interacting galaxy. A detailed host analysis using ALMA, the HST, and the VLT
DOI: 10.1051/0004-6361/201936668 Bibcode: 2020A&A...633A..68D

Covino, S.; Sánchez-Ramírez, R.; Salvaterra, R. +28 more

Context. For the first time, very high energy emission up to the TeV range has been reported for a gamma-ray burst (GRB). It is still unclear whether the environmental properties of GRB 190114C might have contributed to the production of these very high energy photons, or if it is solely related to the released GRB emission.
Aims: The relativ…

2020 Astronomy and Astrophysics
eHST 20
A full characterization of the supermassive black hole in IRAS-=09149-6206
DOI: 10.1093/mnras/staa2961 Bibcode: 2020MNRAS.499.1480W

Harrison, F. A.; Stern, D.; Fabian, A. C. +11 more

We present new broad-band X-ray observations of the type-I Seyfert galaxy IRAS 09149-6206, taken in 2018 with XMM-Newton, NuSTAR, and Swift. The source is highly complex, showing a classic 'warm' X-ray absorber, additional absorption from highly ionized iron, strong relativistic reflection from the innermost accretion disc and further reprocessing…

2020 Monthly Notices of the Royal Astronomical Society
XMM-Newton 20
A Fast, Two-dimensional Gaussian Process Method Based on Celerite: Applications to Transiting Exoplanet Discovery and Characterization
DOI: 10.3847/1538-3881/abbc16 Bibcode: 2020AJ....160..240G

Foreman-Mackey, Daniel; Gordon, Tyler A.; Agol, Eric

Gaussian processes (GPs) are commonly used as a model of stochastic variability in astrophysical time series. In particular, GPs are frequently employed to account for correlated stellar variability in planetary transit light curves. The efficient application of GPs to light curves containing thousands to tens of thousands of data points has been …

2020 The Astronomical Journal
SOHO 20
GG Tauri A: gas properties and dynamics from the cavity to the outer disk
DOI: 10.1051/0004-6361/201936173 Bibcode: 2020A&A...635A..12P

Beck, T.; Chapillon, E.; Hersant, F. +13 more

Context. GG Tauri A is the prototype of a young triple T Tauri star that is surrounded by a massive and extended Keplerian outer disk. The central cavity is not devoid of gas and dust and at least GG Tauri Aa exhibits its own disk of gas and dust emitting at millimeter wavelengths. Its observed properties make this source an ideal laboratory for i…

2020 Astronomy and Astrophysics
Gaia 20
The effects of dwarf galaxies on the orbital evolution of galactic globular clusters
DOI: 10.1093/mnras/staa2773 Bibcode: 2020MNRAS.499..804G

Bovy, Jo; Webb, Jeremy J.; Garrow, Turner

We investigate the effect that dwarf galaxies have on the orbits, tidal histories, and assumed formation environment of Milky Way globular clusters. We determine the orbits of the Milky Way's 150 globular clusters in a gravitational potential both with and without dwarf galaxies. We find that the presence of a small number of satellite galaxies ca…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 20
The stellar variability noise floor for transiting exoplanet photometry with PLATO
DOI: 10.1093/mnras/staa618 Bibcode: 2020MNRAS.493.5489M

Hawley, Suzanne L.; Agol, Eric; Morris, Brett M. +2 more

One of the main science motivations for the ESA PLAnetary Transit and Oscillations (PLATO) mission is to measure exoplanet transit radii with 3 per cent precision. In addition to flares and starspots, stellar oscillations and granulation will enforce fundamental noise floors for transiting exoplanet radius measurements. We simulate light curves of…

2020 Monthly Notices of the Royal Astronomical Society
SOHO 20
Euclid preparation. VIII. The Complete Calibration of the Colour-Redshift Relation survey: VLT/KMOS observations and data release
DOI: 10.1051/0004-6361/202038334 Bibcode: 2020A&A...642A.192E

Cimatti, A.; Ilbert, O.; Burigana, C. +145 more

The Complete Calibration of the Colour-Redshift Relation survey (C3R2) is a spectroscopic effort involving ESO and Keck facilities designed specifically to empirically calibrate the galaxy colour-redshift relation - P(z|C) to the Euclid depth (iAB = 24.5) and is intimately linked to the success of upcoming Stage IV dark energy missions …

2020 Astronomy and Astrophysics
eHST 20
A year-long plateau in the late-time near-infrared light curves of type Ia supernovae
DOI: 10.1038/s41550-019-0901-1 Bibcode: 2020NatAs...4..188G

Ryan, R.; Maguire, K.; Graur, O. +6 more

The light curves of type Ia supernovae are routinely used to constrain cosmology models. Driven by radioactive decay of 56Ni, the light curves steadily decline over time, but after 150 d post-explosion the near-infrared portion is poorly characterized. We report a year-long plateau in the near-infrared light curve at 150-500 d, followed…

2020 Nature Astronomy
eHST 20
An Analysis of the Shapes of Interstellar Extinction Curves. VIII. The Optical Extinction Structure
DOI: 10.3847/1538-4357/ab6f01 Bibcode: 2020ApJ...891...67M

Gordon, Karl D.; Fitzpatrick, E. L.; Massa, Derck

New Hubble Space Telescope/STIS optical spectra were obtained for a sample of early-type stars with existing International Ultraviolet Explorer UV spectra. These data were used to construct optical extinction curves whose general properties are discussed elsewhere. In this paper, we identify extinction features in the curves that are wider than di…

2020 The Astrophysical Journal
eHST 20
On the Chemical and Kinematic Consistency between N-rich Metal-poor Field Stars and Enriched Populations in Globular Clusters
DOI: 10.3847/1538-4357/ab7233 Bibcode: 2020ApJ...891...28T

Shi, Jianrong; Fernández-Trincado, J. G.; Gao, Qi +5 more

Interesting chemically peculiar field stars may reflect their stellar evolution history and their possible origin in a different environment from where they are found now; this is one of the most important research fields in Galactic archeology. To explore this further, we have used the CN-CH bands around 4000 Å to identify N-rich metal-poor field…

2020 The Astrophysical Journal
Gaia 20