Search Publications

A Catalog of RV Variable Star Candidates from LAMOST
DOI: 10.3847/1538-4365/ab9904 Bibcode: 2020ApJS..249...22T

Liu, Gaochao; Wu, Yaqian; Xiang, Maosheng +14 more

Radial velocity (RV) variable stars are important in astrophysics. The Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) spectroscopic survey has provided ∼6.5 million stellar spectra in its Data Release 4 (DR4). During the survey ∼4.7 million unique sources were targeted and ∼1 million stars observed repeatedly. The probabilities…

2020 The Astrophysical Journal Supplement Series
Gaia 21
Turbulence and Energetic Particles in Radiative Shock Waves in the Cygnus Loop. I. Shock Properties
DOI: 10.3847/1538-4357/ab886d Bibcode: 2020ApJ...894..108R

Blair, William P.; Slavin, Jonathan D.; Raymond, John C. +3 more

We have obtained a contiguous set of long-slit spectra of a shock wave in the Cygnus Loop to investigate its structure, which is far from the morphology predicted by 1D models. Proper motions from Hubble Space Telescope images combined with the known distance to the Cygnus Loop provide an accurate shock speed. Earlier analyses of shock spectra est…

2020 The Astrophysical Journal
eHST 21
Recurring Homologous Solar Eruptions in NOAA AR 11429
DOI: 10.3847/1538-4357/abacbc Bibcode: 2020ApJ...901...40D

Zhang, Jie; Vemareddy, Panditi; Karna, Nishu +1 more

We present the study of three homologous solar eruptions from NOAA active region (AR) 11429 over four days. This large and complex AR is divided into two relatively simple subregions: northeast (NE) and southwest (SW). Recurrent eruptions occurred from the SW subregion over different evolutionary phases, which provided a unique opportunity to isol…

2020 The Astrophysical Journal
Hinode SOHO 21
Spectroscopic Constraints on the Buildup of Intracluster Light in the Coma Cluster
DOI: 10.3847/1538-4357/ab845c Bibcode: 2020ApJ...894...32G

van Dokkum, Pieter; Bizyaev, Dmitry; Pan, Kaike +14 more

The stellar content of the intracluster light (ICL) provides unique insight into the hierarchical assembly process of galaxy clusters. We present optical spectra of three ICL regions (µg ≈ 25.3-26.2 mag arcsec-2) in the Coma cluster, located between 100 and 180 kpc from their nearest brightest cluster galaxies (BCGs): N…

2020 The Astrophysical Journal
eHST 21
The spatial evolution of young massive clusters. II. Looking for imprints of star formation in NGC 2264 with Gaia DR2
DOI: 10.1051/0004-6361/201936935 Bibcode: 2020A&A...636A..80B

Hacar, Álvaro; Buckner, Anne S. M.; Khorrami, Zeinab +12 more

Context. Better understanding of star formation in clusters with high-mass stars requires rigorous dynamical and spatial analyses of star-forming regions.
Aims: We seek to demonstrate that "INDICATE" is a powerful spatial analysis tool which when combined with kinematic data from Gaia DR2 can be used to probe star formation history in a robus…

2020 Astronomy and Astrophysics
Gaia Herschel 21
Very wide companion fraction from Gaia DR2: A weak or no enhancement for hot Jupiter hosts, and a strong enhancement for contact binaries
DOI: 10.1093/mnras/staa2124 Bibcode: 2020MNRAS.497.2250H

Zakamska, Nadia L.; Schlaufman, Kevin C.; Hwang, Hsiang-Chih +1 more

There is an ongoing debate on whether hot Jupiter hosts are more likely to be found in wide binaries with separations of ≳100 AU. In this paper, we search for comoving, very wide companions with separations of 103-104 AU for hot Jupiter hosts and main-sequence contact binaries in Gaia DR2, and compare the very wide companion …

2020 Monthly Notices of the Royal Astronomical Society
Gaia 21
Monte Carlo control loops for cosmic shear cosmology with DES Year 1 data
DOI: 10.1103/PhysRevD.101.082003 Bibcode: 2020PhRvD.101h2003K

Smith, M.; Annis, J.; Bertin, E. +53 more

Weak lensing by large-scale structure is a powerful probe of cosmology and of the dark universe. This cosmic shear technique relies on the accurate measurement of the shapes and redshifts of background galaxies and requires precise control of systematic errors. Monte Carlo control loops (MCCL) is a forward modeling method designed to tackle this p…

2020 Physical Review D
Gaia 21
Chemical Properties of the Local Galactic Disk and Halo. I. Fundamental Properties of 1544 Nearby, High Proper-motion M Dwarfs and Subdwarfs
DOI: 10.3847/1538-3881/ab563c Bibcode: 2020AJ....159...30H

Lépine, Sébastien; Rich, R. Michael; Shara, Michael M. +2 more

Due to their ubiquity and very long main-sequence lifetimes, M dwarfs provide an excellent tool to study the formation and chemical enrichment history of our Galaxy. However, owing to their intrinsic faintness, the acquisition of high-resolution, high signal-to-noise spectra of low-mass stars has been limited to small numbers of very nearby stars,…

2020 The Astronomical Journal
Gaia 21
Magnetospheric Studies: A Requirement for Addressing Interdisciplinary Mysteries in the Ice Giant Systems
DOI: 10.1007/s11214-020-00696-5 Bibcode: 2020SSRv..216...78K

Roussos, E.; Rymer, A.; Allen, R. C. +18 more

Uranus and Neptune are the least-explored planets in our Solar System. This paper summarizes mysteries about these incredibly intriguing planets and their environments spurred by our limited observations from Voyager 2 and Earth-based systems. Several of these observations are either inconsistent with our current understanding built from exploring…

2020 Space Science Reviews
Cluster 21
Super-resolution of SDO/HMI Magnetograms Using Novel Deep Learning Methods
DOI: 10.3847/2041-8213/ab9d79 Bibcode: 2020ApJ...897L..32R

Moon, Yong-Jae; Lim, Daye; Rahman, Sumiaya +3 more

Image super-resolution is a technique of enhancing the resolution of an image where a high-resolution (HR) image is reconstructed from a low-resolution (LR) image. In this Letter, we apply two novel deep learning models (residual attention model and progressive GAN model) for enhancing Solar Dynamics Observatory (SDO)/Helioseismic and Magnetic Ima…

2020 The Astrophysical Journal
Hinode 21