Search Publications

Coronal bright points
DOI: 10.1007/s41116-019-0018-8 Bibcode: 2019LRSP...16....2M

Madjarska, Maria S.

Coronal bright points (CBPs) are a fundamental class of solar activity. They represent a set of low-corona small-scale loops with enhanced emission in the extreme-ultraviolet and X-ray spectrum that connect magnetic flux concentrations of opposite polarities. CBPs are one of the main building blocks of the solar atmosphere outside active regions u…

2019 Living Reviews in Solar Physics
Hinode IRIS SOHO 65
ExoEarth yield landscape for future direct imaging space telescopes
DOI: 10.1117/1.JATIS.5.2.024009 Bibcode: 2019JATIS...5b4009S

Stark, Christopher C.; Mazoyer, Johan; Pueyo, Laurent +19 more

The expected yield of potentially Earth-like planets is a useful metric for designing future exoplanet-imaging missions. Recent yield studies of direct-imaging missions have focused primarily on yield methods and trade studies using "toy" models of missions. Here, we increase the fidelity of these calculations substantially, adopting more realisti…

2019 Journal of Astronomical Telescopes, Instruments, and Systems
Gaia 64
The mean Hα EW and Lyman-continuum photon production efficiency for faint z ≈ 4-5 galaxies
DOI: 10.1051/0004-6361/201935227 Bibcode: 2019A&A...627A.164L

Bacon, Roland; Boogaard, Leindert A.; Mahler, Guillaume +9 more

We present the first measurements of the Lyman-continuum photon production efficiency ξion, 0 at z ∼ 4-5 for galaxies fainter than 0.2 L* (-19 mag). ξion, 0 quantifies the production rate of ionizing photons with respect to the UV luminosity density assuming a fiducial escape fraction of zero. Extending previous me…

2019 Astronomy and Astrophysics
eHST 64
AKARI/IRC near-infrared asteroid spectroscopic survey: AcuA-spec
DOI: 10.1093/pasj/psy125 Bibcode: 2019PASJ...71....1U

Hasegawa, Sunao; Onaka, Takashi; Usui, Fumihiko +1 more

Knowledge of water in the solar system is important for the understanding of a wide range of evolutionary processes and the thermal history of the solar system. To explore the existence of water in the solar system, it is indispensable to investigate hydrated minerals and/or water ice on asteroids. These water-related materials show absorption fea…

2019 Publications of the Astronomical Society of Japan
AKARI 64
Merging Cluster Collaboration: A Panchromatic Atlas of Radio Relic Mergers
DOI: 10.3847/1538-4357/ab2f90 Bibcode: 2019ApJ...882...69G

Bradač, M.; Venturi, T.; Jee, M. J. +13 more

Golovich et al. present an optical imaging and spectroscopic survey of 29 radio relic merging galaxy clusters. In this paper, we study this survey to identify substructure and quantify the dynamics of the mergers. Using a combined photometric and spectroscopic approach, we identify the minimum number of substructures in each system to describe the…

2019 The Astrophysical Journal
XMM-Newton eHST 64
The Polycyclic Aromatic Hydrocarbon Mass Fraction on a 10 pc Scale in the Magellanic Clouds
DOI: 10.3847/1538-4357/ab16cf Bibcode: 2019ApJ...876...62C

Gordon, Karl D.; Bot, Caroline; Leroy, Adam K. +8 more

We present maps of the dust properties in the Small and Large Magellanic Clouds (SMC, LMC) from fitting Spitzer and Herschel observations with the Draine & Li dust model. We derive the abundance of the small carbonaceous grain (or polycyclic aromatic hydrocarbon; PAH) component. The global PAH fraction ({q}{{PAH}}, the fraction of t…

2019 The Astrophysical Journal
Herschel 64
Cosmological constraints on an exponential interaction in the dark sector
DOI: 10.1093/mnras/sty2780 Bibcode: 2019MNRAS.482.1007Y

Yang, Weiqiang; Pan, Supriya; Paliathanasis, Andronikos

Cosmological models where dark matter (DM) and dark energy (DE) interact with each other are the general scenarios in compared to the non-interacting models. The interaction is usually motivated from the phenomenological ground and thus there is no such rule to prefer a particular interaction between DM and DE. Being motivated, in this work, allow…

2019 Monthly Notices of the Royal Astronomical Society
eHST 64
ALMA 26 arcmin2 Survey of GOODS-S at 1 mm (ASAGAO): Near-infrared-dark Faint ALMA Sources
DOI: 10.3847/1538-4357/ab0d22 Bibcode: 2019ApJ...878...73Y

Ouchi, Masami; Fujimoto, Seiji; Tamura, Yoichi +21 more

We report detections of two 1.2 mm continuum sources (S 1.2 mm ∼ 0.6 mJy) without any counterparts in the deep H- and/or K-band image (i.e., K-band magnitude ≳26 mag). These near-infrared-dark faint millimeter sources are uncovered by ASAGAO, a deep and wide-field (≃26 arcmin2) Atacama Large Millimeter/submillimeter Array (AL…

2019 The Astrophysical Journal
Gaia eHST 64
Geological Evidence of Planet-Wide Groundwater System on Mars
DOI: 10.1029/2018JE005802 Bibcode: 2019JGRE..124..374S

Ori, Gian Gabriele; Salese, Francesco; Pondrelli, Monica +2 more

The scale of groundwater upwelling on Mars, as well as its relation to sedimentary systems, remains an ongoing debate. Several deep craters (basins) in the northern equatorial regions show compelling signs that large amounts of water once existed on Mars at a planet-wide scale. The presence of water-formed features, including fluvial Gilbert and s…

2019 Journal of Geophysical Research (Planets)
MEx 64
The ALMA Discovery of the Rotating Disk and Fast Outflow of Cold Molecular Gas in NGC 1275
DOI: 10.3847/1538-4357/ab3e6e Bibcode: 2019ApJ...883..193N

Fukazawa, Y.; Nagai, H.; Onishi, K. +13 more

We present observations using the Atacama Large Millimeter/submillimeter Array of the CO(2-1), HCN(3-2), and HCO+(3-2) lines in the nearby radio galaxy/brightest cluster galaxy (BCG) NGC 1275 with a spatial resolution of ∼20 pc. In previous observations, the CO(2-1) emission was detected as radial filaments lying in the east-west direct…

2019 The Astrophysical Journal
eHST 64