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期刊名:Astrophysical journal

缩写:ASTROPHYS J

ISSN:0004-637X

e-ISSN:1538-4357

IF/分区:5.7/Q1

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Clinical Trial Case Reports Meta-Analysis RCT Review Systematic Review
Classical Article Case Reports Clinical Study Clinical Trial Clinical Trial Protocol Comment Comparative Study Editorial Guideline Letter Meta-Analysis Multicenter Study Observational Study Randomized Controlled Trial Review Systematic Review
Isak G B Wold,Amy J Barger,Lennox L Cowie Isak G B Wold
We construct a flux-limited sample of 135 candidate z ~ 1 Lyα emitters (LAEs) from Galaxy Evolution Explorer (GALEX) grism data using a new data cube search method. These LAEs have luminosities comparable to those at high redshifts and lie...
Courtney D Dressing,Kevin Hardegree-Ullman,Joshua E Schlieder et al. Courtney D Dressing et al.
We present revised stellar properties for 172 K2 target stars that were identified as possible hosts of transiting planets during Campaigns 1-17. Using medium-resolution near-infrared spectra acquired with the NASA Infrared Telescope Facili...
Trevor Knuth,Lindsay Glesener Trevor Knuth
Solar flares are known to release a large amount of energy into accelerating electrons. Studying small timescale (⩽2s) fluctuations in nonthermal X-ray flux offers the opportunity to probe the nature of those acceleration mechanisms. By co...
Juliana T Vievering,Lindsay Glesener,Brian W Grefenstette et al. Juliana T Vievering et al.
We study the structure and dynamics of extreme flaring events on young stellar objects (YSOs) observed in hard X-rays by the Nuclear Spectroscopic Telescope Array (NuSTAR). During 2015 and 2016, NuSTAR made three observations of the star-fo...
Juliana T Vievering,Lindsay Glesener,P S Athiray et al. Juliana T Vievering et al.
We study the nature of energy release and transfer for two sub-A class solar microflares observed during the second Focusing Optics X-ray Solar Imager (FOXSI-2) sounding rocket flight on 2014 December 11. FOXSI is the first solar-dedicated ...
Jessie Duncan,Lindsay Glesener,Brian W Grefenstette et al. Jessie Duncan et al.
Solar flares are explosive releases of magnetic energy. Hard X-ray (HXR) flare emission originates from both hot (millions of Kelvin) plasma and nonthermal accelerated particles, giving insight into flare energy release. The Nuclear Spectro...
K J Knizhnik,M G Linton,C R DeVore K J Knizhnik
It has been observationally well established that the magnetic configurations most favorable for producing energetic flaring events reside in δ-spots, a class of sunspots defined as having opposite-polarity umbrae sharing a common penumbra...
M Ajello,L Baldini,G Barbiellini et al. M Ajello et al.
We use joint observations by the Neil Gehrels Swift X-ray Telescope (XRT) and the Fermi Large Area Telescope (LAT) of gamma-ray burst (GRB) afterglows to investigate the nature of the long-lived high-energy emission observed by Fermi LAT. J...
Jacob Heerikhuisen,Konstantin V Gamayunov,Eric J Zirnstein et al. Jacob Heerikhuisen et al.
In this paper, we present results from our three-dimensional (3D) simulations of the interaction between the solar wind and local interstellar medium with an emphasis on the phase-space properties of energetic neutral atoms (ENAs) along a s...
Amy C Gall,Adam R Foster,Roshani Silwal et al. Amy C Gall et al.
Motivated by possible atomic origins of the unidentified emission line detected at 3.55-3.57 keV in a stacked spectrum of galaxy clusters, an electron beam ion trap (EBIT) was used to investigate the resonant dielectronic recombination (DR)...