Search Publications

Selection of Massive Evolved Galaxies at 3 ≤ z ≤ 4.5 in the CANDELS Fields
DOI: 10.3847/1538-4357/ab96c5 Bibcode: 2020ApJ...897...44S

Papovich, Casey; Finkelstein, Steven L.; Dickinson, Mark +14 more

Using the CANDELS photometric catalogs for the Hubble Space Telescope/ACS and WFC3, we identified massive evolved galaxies at 3 < z < 4.5 employing three different selection methods. We find the comoving number density of these objects to be ∼2 × 10-5 and 8 × 10-6 Mpc-3 after correction for completeness for t…

2020 The Astrophysical Journal
eHST 29
The TESS-Keck Survey. III. A Stellar Obliquity Measurement of TOI-1726 c
DOI: 10.3847/1538-3881/abb3bd Bibcode: 2020AJ....160..193D

Kristiansen, Martti H.; Batalha, Natalie M.; Latham, David W. +43 more

We report the measurement of a spectroscopic transit of TOI-1726c, one of two planets transiting a G-type star with V = 6.9 in the Ursa Major Moving Group (∼400 Myr). With a precise age constraint from cluster membership, TOI-1726 provides a great opportunity to test various obliquity excitation scenarios that operate on different timescales. By m…

2020 The Astronomical Journal
Gaia 29
Hard X-Ray Excess from the Magnificent Seven Neutron Stars
DOI: 10.3847/1538-4357/abb4ea Bibcode: 2020ApJ...904...42D

Safdi, Benjamin R.; Foster, Joshua W.; Dessert, Christopher

We report significant hard X-ray excesses in the energy range 2-8 keV for two nearby isolated neutron stars: RX J1856.6-3754 and RX J0420.0-5022. These neutron stars have previously been observed in soft X-rays to have nearly thermal spectra at temperatures ∼100 eV, which are thought to arise from the warm neutron star surfaces. We find nontrivial…

2020 The Astrophysical Journal
XMM-Newton 29
X-Ray Binary Luminosity Function Scaling Relations in Elliptical Galaxies: Evidence for Globular Cluster Seeding of Low-mass X-Ray Binaries in Galactic Fields
DOI: 10.3847/1538-4365/ab9175 Bibcode: 2020ApJS..248...31L

Brandt, William N.; Tzanavaris, Panayiotis; Basu-Zych, Antara +10 more

We investigate X-ray binary (XRB) luminosity function (XLF) scaling relations for Chandra-detected populations of low-mass XRBs (LMXBs) within the footprints of 24 early-type galaxies. Our sample includes Chandra and Hubble Space Telescope observed galaxies at $D\lesssim 25$ Mpc that have estimates of the globular cluster (GC) specific frequency (…

2020 The Astrophysical Journal Supplement Series
Herschel eHST 29
Whistler Waves and Electron Properties in the Inner Heliosphere: Helios Observations
DOI: 10.3847/1538-4357/ab94a1 Bibcode: 2020ApJ...897..118J

Alexandrova, Olga; de Wit, Thierry Dudok; Maksimovic, Milan +4 more

We present the analysis of narrowband whistler wave signatures observed in the inner heliosphere (0.3-1 au). These signatures are bumps in the spectral density in the 10-200 Hz frequency range of the AC magnetic field as measured by the search coil magnetometer on board the Helios 1 spacecraft. We show that the majority of whistler signatures are …

2020 The Astrophysical Journal
Cluster 29
Phase reddening on asteroid Bennu from visible and near-infrared spectroscopy
DOI: 10.1051/0004-6361/202039552 Bibcode: 2020A&A...644A.142F

Barucci, M. A.; Fornasier, S.; Li, J. -Y. +10 more

Context. The NASA mission OSIRIS-REx (Origins, Spectral Interpretation, Resource Identification, and Security-Regolith Explorer) has been observing near-Earth asteroid (101955) Bennu in close proximity since December 2018. In October 2020, the spacecraft collected a sample of surface material from Bennu to return to Earth.
Aims: In this work,…

2020 Astronomy and Astrophysics
Rosetta 29
High-resolution, 3D radiative transfer modelling. III. The DustPedia barred galaxies
DOI: 10.1051/0004-6361/201936176 Bibcode: 2020A&A...637A..25N

Clark, Christopher J. R.; Mosenkov, Aleksandr V.; De Looze, Ilse +17 more

Context. Dust in late-type galaxies in the local Universe is responsible for absorbing approximately one third of the energy emitted by stars. It is often assumed that dust heating is mainly attributable to the absorption of ultraviolet and optical photons emitted by the youngest (≤100 Myr) stars. Consequently, thermal re-emission by dust at far-i…

2020 Astronomy and Astrophysics
Herschel 29
Hot Subdwarf Stars Identified in Gaia DR2 with Spectra of LAMOST DR6 and DR7. I. Single-lined Spectra
DOI: 10.3847/1538-4357/ab660a Bibcode: 2020ApJ...889..117L

Zhao, Gang; Németh, Péter; Zhao, Jingkun +1 more

182 single-lined hot subdwarf stars are identified by using spectra from the sixth and seventh data releases (DR6 and DR7) of the Large Sky Area Multi-Object Fibre Spectroscopic Telescope survey. We classified all the hot subdwarf stars using a canonical classification scheme, and got 89 sdB, 37 sdOB, 26 sdO, 24 He-sdOB, 3 He-sdO, and 3 He-sdB sta…

2020 The Astrophysical Journal
Gaia 29
A multiplicity study of transiting exoplanet host stars. II. Revised properties of transiting planetary systems with companions
DOI: 10.1051/0004-6361/201937334 Bibcode: 2020A&A...635A..74S

Ginski, C.; Southworth, J.; Mancini, L. +2 more

Context. Binarity is a widespread phenomenon around solar-type stars, including the host stars of transiting extrasolar planets.
Aims: We performed a detailed study of six transiting planetary systems with relatively bright stars close enough to affect observations of these systems. These contaminants were characterised in a companion work. <…

2020 Astronomy and Astrophysics
Gaia 29
First detection of ozone in the mid-infrared at Mars: implications for methane detection
DOI: 10.1051/0004-6361/202038125 Bibcode: 2020A&A...639A.141O

Montmessin, F.; Fedorova, A.; Korablev, O. +9 more


Aims: The ExoMars Trace Gas Orbiter was sent to Mars in March 2016 to search for trace gases diagnostic of active geological or biogenic processes.
Methods: We report the first observation of the spectral features of Martian ozone (O3) in the mid-infrared range using the Atmospheric Chemistry Suite Mid-InfaRed (MIR) channel, a…

2020 Astronomy and Astrophysics
ExoMars-16 29