Search Publications

Presupernova Neutrinos: Directional Sensitivity and Prospects for Progenitor Identification
DOI: 10.3847/1538-4357/ab99a6 Bibcode: 2020ApJ...899..153M

Timmes, F. X.; Mukhopadhyay, Mainak; Lunardini, Cecilia +1 more

We explore the potential of current and future liquid scintillator neutrino detectors of ${ \mathcal O }(10)$ kt mass to localize a presupernova neutrino signal in the sky. In the hours preceding the core collapse of a nearby star (at distance $D\lesssim 1$ kpc), tens to hundreds of inverse beta decay events will be recorded, and their reconstruct…

2020 The Astrophysical Journal
Gaia 41
Spectroscopically Confirmed Lyα Emitters from Redshift 5 to 7 behind 10 Galaxy Cluster Lenses
DOI: 10.3847/1538-4357/ab959f Bibcode: 2020ApJ...896..156F

Hoag, A.; Bradač, M.; Treu, T. +10 more

We present 36 spectroscopically confirmed intrinsically UV-faint Lyα-emitting galaxies from follow-up observations with Keck/DEep Imaging Multi-Object Spectrograph of gravitationally lensed high-redshift candidates. Candidates were selected to be between 5 ≲ z ≲ 7 from photometric data using Hubble Space Telescope and Spitzer imaging surveys. We p…

2020 The Astrophysical Journal
eHST 41
Hot Plasma Flows and Oscillations in the Loop-top Region During the 2017 September 10 X8.2 Solar Flare
DOI: 10.3847/1538-4357/abc4e0 Bibcode: 2020ApJ...905..165R

Reeves, Katharine K.; Polito, Vanessa; Chen, Bin +4 more

In this study, we investigate motions in the hot plasma above the flare loops during the 2017 September 10 X8.2 flare event. We examine the region to the south of the main flare arcade, where there is data from the Interface Region Imaging Spectrograph (IRIS) and the Extreme ultraviolet Imaging Spectrometer (EIS) on Hinode. We find that there are …

2020 The Astrophysical Journal
Hinode IRIS 41
Model-independent Constraints on Cosmic Curvature: Implication from Updated Hubble Diagram of High-redshift Standard Candles
DOI: 10.3847/1538-4357/abb0e4 Bibcode: 2020ApJ...901..129L

Li, Xiaolei; Liu, Yuting; Cao, Shuo +4 more

The cosmic curvature (Ωk) is a fundamental parameter for cosmology. In this paper, we propose an improved model-independent method to constrain the cosmic curvature, which is geometrically related to the Hubble parameter H(z) and luminosity distance DL(z). Using the currently largest H(z) sample from the well-known cosmic chr…

2020 The Astrophysical Journal
eHST 41
Exploring the Galactic Warp through Asymmetries in the Kinematics of the Galactic Disk
DOI: 10.3847/1538-4357/abc3c2 Bibcode: 2020ApJ...905...49C

Majewski, Steven R.; Cheng, Xinlun; Anguiano, Borja +10 more

Previous analyses of large databases of Milky Way stars have revealed the stellar disk of our Galaxy to be warped and that this imparts a strong signature on the kinematics of stars beyond the solar neighborhood. However, due to the limitation of accurate distance estimates, many attempts to explore the extent of these Galactic features have gener…

2020 The Astrophysical Journal
Gaia 41
A Catalog of M-dwarf Flares with ASAS-SN
DOI: 10.3847/1538-4357/ab793a Bibcode: 2020ApJ...892..144R

Holoien, Thomas W. -S.; Auchettl, Katie; Kochanek, Christopher S. +5 more

We analyzed the light curves of 1376 early-to-late, nearby M dwarfs to search for white-light flares using photometry from the All-Sky Automated Survey for Supernovae. We identified 480 M dwarfs with at least one potential flare employing a simple statistical algorithm that searches for sudden increases in V-band flux. After more detailed evaluati…

2020 The Astrophysical Journal
Gaia 41
Dissecting the Phase Space Snail Shell
DOI: 10.3847/1538-4357/ab6b21 Bibcode: 2020ApJ...890...85L

Shen, Juntai; Li, Zhao-Yu

The ongoing vertical phase-mixing, manifesting itself as a snail shell in the $Z-{V}_{Z}$ phase space, has been discovered with Gaia DR2 data. To better understand the origin and properties of the phase-mixing process, we study the vertical phase-mixing signatures in arches (including the classical "moving groups") of the ${V}_{R}-{V}_{\phi }$ pha…

2020 The Astrophysical Journal
Gaia 40
Pressure Profiles and Mass Estimates Using High-resolution Sunyaev-Zel'dovich Effect Observations of Zwicky 3146 with MUSTANG-2
DOI: 10.3847/1538-4357/ab6d70 Bibcode: 2020ApJ...891...90R

Battaglia, Nicholas; Mroczkowski, Tony; Devlin, Mark +12 more

The galaxy cluster Zwicky 3146 is a sloshing cool core cluster at z = 0.291 that in X-ray imaging does not appear to exhibit significant pressure substructure in the intracluster medium (ICM). The published M500 values range between 3.88-0.58+0.62 to (22.50 ± 7.58) × 1014 M, where ICM-based e…

2020 The Astrophysical Journal
XMM-Newton 40
Consistently Simulating a Wide Range of Atmospheric Scenarios for K2-18b with a Flexible Radiative Transfer Module
DOI: 10.3847/1538-4357/ab9084 Bibcode: 2020ApJ...898...44S

Rauer, H.; Kappel, D.; Herbst, K. +6 more

The atmospheres of small, potentially rocky exoplanets are expected to cover a diverse range in composition and mass. Studying such objects therefore requires flexible and wide-ranging modeling capabilities. We present in this work the essential development steps that lead to our flexible radiative transfer module, REDFOX, and validate REDFOX for …

2020 The Astrophysical Journal
eHST 40
Stellar Characterization of M Dwarfs from the APOGEE Survey: A Calibrator Sample for M-dwarf Metallicities
DOI: 10.3847/1538-4357/ab6d07 Bibcode: 2020ApJ...890..133S

Wanderley, Fábio; Cunha, Katia; Smith, Verne V. +18 more

We present spectroscopic determinations of the effective temperatures, surface gravities, and metallicities for 21 M dwarfs observed at high resolution (R ∼ 22,500) in the H band as part of the Sloan Digital Sky Survey (SDSS)-IV Apache Point Observatory Galactic Evolution Experiment (APOGEE) survey. The atmospheric parameters and metallicities are…

2020 The Astrophysical Journal
Gaia 40