Search Publications

The Morphology-Density Relationship in 1 < z < 2 Clusters
DOI: 10.3847/1538-4357/aba42f Bibcode: 2020ApJ...899...85S

Rodriguez-Gomez, Vicente; Snyder, Gregory F.; Brodwin, Mark +8 more

The morphology-density relationship states that dense cosmic environments such as galaxy clusters have an overabundance of quiescent elliptical galaxies, but it is unclear at which redshift this relationship is first established. We study the morphology of four clusters with 1.2 < z < 1.8 using Hubble Space Telescope imaging and the morpholo…

2020 The Astrophysical Journal
eHST 32
An Isolated White Dwarf with 317 s Rotation and Magnetic Emission
DOI: 10.3847/1538-4357/ab8239 Bibcode: 2020ApJ...894...19R

Hermes, J. J.; Clemens, J. C.; Vanderbosch, Z. +5 more

We report the discovery of short-period photometric variability and modulated Zeeman-split hydrogen emission in SDSSJ125230.93-023417.72 (EPIC 228939929), a variable white dwarf star observed at long cadence in K2 Campaign 10. The behavior is associated with a magnetic (B = 5.0 MG) spot on the stellar surface, making the 317.278 s period a direct …

2020 The Astrophysical Journal
Gaia 32
An Extended Theoretical Scenario for Classical Cepheids. I. Modeling Galactic Cepheids in the Gaia Photometric System
DOI: 10.3847/1538-4365/ab7204 Bibcode: 2020ApJS..247...30D

Cignoni, Michele; Marconi, Marcella; Molinaro, Roberto +3 more

We present a new extended and detailed set of models for classical Cepheid pulsators at solar chemical composition (Z = 0.02, Y = 0.28) based on a well-tested nonlinear hydrodynamical approach. In order to model the possible dependence on crucial assumptions such as the mass-luminosity relation of central helium burning intermediate-mass stars or …

2020 The Astrophysical Journal Supplement Series
Gaia 32
Assessment of supervised machine learning for atmospheric retrieval of exoplanets
DOI: 10.1093/mnras/staa1150 Bibcode: 2020MNRAS.496..269N

Madhusudhan, Nikku; Nixon, Matthew C.

Atmospheric retrieval of exoplanets from spectroscopic observations requires an extensive exploration of a highly degenerate and high-dimensional parameter space to accurately constrain atmospheric parameters. Retrieval methods commonly conduct Bayesian parameter estimation and statistical inference using sampling algorithms such as Markov chain M…

2020 Monthly Notices of the Royal Astronomical Society
eHST 32
KELT-25 b and KELT-26 b: A Hot Jupiter and a Substellar Companion Transiting Young A Stars Observed by TESS
DOI: 10.3847/1538-3881/ab9f2d Bibcode: 2020AJ....160..111R

Cargile, Phillip A.; Bieryla, Allyson; Latham, David W. +89 more

We present the discoveries of KELT-25 b (TIC 65412605, TOI-626.01) and KELT-26 b (TIC 160708862, TOI-1337.01), two transiting companions orbiting relatively bright, early A stars. The transit signals were initially detected by the KELT survey and subsequently confirmed by Transiting Exoplanet Survey Satellite (TESS) photometry. KELT-25 b is on a 4…

2020 The Astronomical Journal
Gaia 32
Asteroid masses obtained with INPOP planetary ephemerides
DOI: 10.1093/mnras/stz3407 Bibcode: 2020MNRAS.492..589F

Fienga, A.; Avdellidou, C.; Hanuš, J.

In this paper, we present masses of 103 asteroids deduced from their perturbations on the orbits of the inner planets, in particular Mars and the Earth. These determinations and the INPOP19a planetary ephemerides are improved by the recent Mars orbiter navigation data and the updated orbit of Jupiter based on the Juno mission data. More realistic …

2020 Monthly Notices of the Royal Astronomical Society
AKARI 32
The soft excess of the NLS1 galaxy Mrk 359 studied with an XMM-Newton-NuSTAR monitoring campaign
DOI: 10.1051/0004-6361/202038112 Bibcode: 2020A&A...640A..99M

Bianchi, S.; Cappi, M.; Petrucci, P. -O. +7 more

Context. Joint XMM-Newton and NuSTAR multiple exposures allow us to disentangle the different emission components of active galactic nuclei (AGNs) and to study the evolution of their different spectral features. In this work, we present the timing and spectral properties of five simultaneous XMM-NewtonandNuSTAR observations of the Narrow Line Seyf…

2020 Astronomy and Astrophysics
XMM-Newton 32
Blazars at the Cosmic Dawn
DOI: 10.3847/1538-4357/ab9c1a Bibcode: 2020ApJ...897..177P

Ajello, M.; Giroletti, M.; Madejski, Greg +5 more

The uncharted territory of the high-redshift (z ≳ 3) universe holds the key to understanding the evolution of quasars. In an attempt to identify the most extreme members of the quasar population, that is, blazars, we have carried out a multiwavelength study of a large sample of radio-loud quasars beyond z = 3. Our sample consists of nine γ-ray-det…

2020 The Astrophysical Journal
XMM-Newton 32
The Chandra Deep Wide-field Survey: A New Chandra Legacy Survey in the Boötes Field. I. X-Ray Point Source Catalog, Number Counts, and Multiwavelength Counterparts
DOI: 10.3847/1538-4365/abb607 Bibcode: 2020ApJS..251....2M

Miller, Eric D.; Myers, Adam D.; Aird, James +30 more

We present a new, ambitious survey performed with the Chandra X-ray Observatory of the 9.3 deg2 Boötes field of the NOAO Deep Wide-Field Survey. The wide field probes a statistically representative volume of the universe at high redshift. The Chandra Deep Wide-field Survey exploits the excellent sensitivity and angular resolution of Cha…

2020 The Astrophysical Journal Supplement Series
Gaia 32
The dark matter component of the Gaia radially anisotropic substructure
DOI: 10.1088/1475-7516/2020/07/036 Bibcode: 2020JCAP...07..036B

Grand, Robert J. J.; Gómez, Facundo A.; Fattahi, Azadeh +5 more

We study the properties of the dark matter component of the radially anisotropic stellar population recently identified in the Gaia data, using magneto-hydrodynamical simulations of Milky Way-like halos from the Auriga project. We identify 10 simulated galaxies that approximately match the rotation curve and stellar mass of the Milky Way. Four of …

2020 Journal of Cosmology and Astroparticle Physics
Gaia 32