Search Publications

Cataclysmic Variables in the First Year of the Zwicky Transient Facility
DOI: 10.3847/1538-3881/ab7cce Bibcode: 2020AJ....159..198S

Riddle, Reed; Szkody, Paula; Bellm, Eric C. +25 more

Using selection criteria based on amplitude, time, and color, we have identified 329 objects as known or candidate cataclysmic variables (CVs) during the first year of testing and operation of the Zwicky Transient Facility. Of these, 90 are previously confirmed CVs, 218 are strong candidates based on the shape and color of their light curves obtai…

2020 The Astronomical Journal
Gaia 29
The MASSIVE Survey. XV. A Stellar Dynamical Mass Measurement of the Supermassive Black Hole in Massive Elliptical Galaxy NGC 1453
DOI: 10.3847/1538-4357/ab6f71 Bibcode: 2020ApJ...891....4L

Ma, Chung-Pei; Greene, Jenny E.; Blakeslee, John P. +4 more

We present a new stellar dynamical mass measurement (M_{BH}) of the supermassive black hole (SMBH) in NGC 1453, a fast-rotating massive elliptical galaxy in the MASSIVE survey. We measure stellar kinematics in 135 spatial bins in the central 1.5 kpc × 2 kpc region of the galaxy using high signal-to-noise ratio (S/N ∼ 130) spectra from the Gemini-N…

2020 The Astrophysical Journal
eHST 29
Returning Samples from Enceladus for Life Detection
DOI: 10.3389/fspas.2020.00026 Bibcode: 2020FrASS...7...26N

MacKenzie, Shannon M.; Davila, Alfonso F.; Neveu, Marc +7 more

Evidence suggests that Saturn's icy moon Enceladus has a subsurface ocean that sources plumes of water vapor and ice vented to space from its south pole. In situ analyses of this material by the Cassini spacecraft have shown that the ocean contains key ingredients for life (elements H, C, N, O and possibly S; simple and complex organic compounds; …

2020 Frontiers in Astronomy and Space Sciences
Cassini 29
Transmission Spectroscopy of WASP-79b from 0.6 to 5.0 µm
DOI: 10.3847/1538-3881/ab5442 Bibcode: 2020AJ....159....5S

Jayaraman, Rahul; Nikolov, Nikolay; Sing, David K. +18 more

As part of the Panchromatic Exoplanet Treasury program, we have conducted a spectroscopic study of WASP-79b, an inflated hot Jupiter orbiting an F-type star in Eridanus with a period of 3.66 days. Building on the original WASP and TRAPPIST photometry of Smalley et al., we examine Hubble Space Telescope (HST)/Wide Field Camera 3 (WFC3) (1.125-1.650…

2020 The Astronomical Journal
Gaia XMM-Newton eHST 29
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