Search Publications

SHARDS Frontier Fields: Physical Properties of a Low-mass Lyα Emitter at z = 5.75
DOI: 10.3847/1538-4357/aa917f Bibcode: 2017ApJ...849...82H

Pérez-González, Pablo G.; Richard, Johan; Conselice, Christopher J. +20 more

We analyze the properties of a multiply imaged Lyα (Lyα) emitter at z = 5.75 identified through SHARDS Frontier Fields intermediate-band imaging of the Hubble Frontier Fields (HFF) cluster Abell 370. The source, A370-L57, has low intrinsic luminosity (M UV ∼ -16.5), steep UV spectral index (β = -2.4 ± 0.1), and extreme rest-frame equiva…

2017 The Astrophysical Journal
eHST 13
Growth rate measurement of ULF waves in the ion foreshock
DOI: 10.1002/2017GL072692 Bibcode: 2017GeoRL..44.2120D

Hietala, H.; Angelopoulos, V.; Dorfman, S. +1 more

We report the first satellite measurement of the ultralow frequency (ULF) wave growth rate in the upstream region of the Earth's bow shock. We employ the two identical ARTEMIS spacecraft orbiting the Moon to characterize crescent-shaped reflected ion beams and relatively monochromatic ULF waves. The event presented here features spacecraft separat…

2017 Geophysical Research Letters
Cluster 12
Characterizing dw1335-29, a recently discovered dwarf satellite of M83
DOI: 10.1093/mnras/stw3025 Bibcode: 2017MNRAS.465.5026C

Bell, Eric F.; Monachesi, Antonela; Bailin, Jeremy +4 more

The number, distribution and properties of dwarf satellites are crucial probes of the physics of galaxy formation at low masses and the response of satellite galaxies to the tidal and gas dynamical effects of their more massive parent. To make progress, it is necessary to augment and solidify the census of dwarf satellites of galaxies outside the …

2017 Monthly Notices of the Royal Astronomical Society
eHST 12
Gaia eclipsing binary and multiple systems. Supervised classification and self-organizing maps
DOI: 10.1051/0004-6361/201629710 Bibcode: 2017A&A...603A.117S

Rimoldini, L.; Holl, B.; Mowlavi, N. +6 more

Context. Large surveys producing tera- and petabyte-scale databases require machine-learning and knowledge discovery methods to deal with the overwhelming quantity of data and the difficulties of extracting concise, meaningful information with reliable assessment of its uncertainty. This study investigates the potential of a few machine-learning m…

2017 Astronomy and Astrophysics
Gaia Hipparcos 12
Calibrating the Planck Cluster Mass Scale with Cluster Velocity Dispersions
DOI: 10.3847/1538-4357/aa7063 Bibcode: 2017ApJ...844..101A

Chary, Ranga-Ram; Stern, Daniel; Shim, Hyunjin +7 more

We measure the Planck cluster mass bias using dynamical mass measurements based on velocity dispersions of a subsample of 17 Planck-detected clusters. The velocity dispersions were calculated using redshifts determined from spectra that were obtained at the Gemini observatory with the GMOS multi-object spectrograph. We correct our estimates for ef…

2017 The Astrophysical Journal
Planck 12
Pushing the limits: detecting H2 emission from faint bipolar planetary nebulae in the IPHAS sample
DOI: 10.1093/mnras/stx1519 Bibcode: 2017MNRAS.470.3707R

Guerrero, M. A.; Santamaría, E.; Ramos-Larios, G. +1 more

We have obtained deep narrowband images in the near-infrared H2 λ2.122 µm emission line for a sample of 15 faint Isaac Newton Telescope Photometric H α Survey (IPHAS) bipolar planetary nebulae (PNe) to search for molecular material. H2 emission is found in most of them (14 out of 15), mostly associated with rings at the…

2017 Monthly Notices of the Royal Astronomical Society
eHST 12
The Deflection of the Cartwheel CME: ForeCAT Results
DOI: 10.3847/1538-4357/aa6a16 Bibcode: 2017ApJ...839...37C

Landi, Enrico; Kay, Christina; Capannolo, Luisa +1 more

We analyze the Cartwheel coronal mass ejection's (CME; 2008 April 9) trajectory in the low corona with the ForeCAT model. This complex event presented a significant rotation in the low corona and a reversal in its original latitude direction. We successfully reproduce the observed CME’s trajectory (latitude and longitude deflection) and speed. Thr…

2017 The Astrophysical Journal
SOHO 12
The Roles of Reconnected Flux and Overlying Fields in CME Speeds
DOI: 10.1007/s11207-016-1036-5 Bibcode: 2017SoPh..292...17D

Welsch, Brian T.; Deng, Minda

Researchers have reported i) correlations of coronal mass ejection (CME) speeds and the total photospheric magnetic flux swept out by flare ribbons in flare-associated eruptive events, and, separately, ii) correlations of CME speeds and more rapid decay, with height, of magnetic fields in potential-field coronal models above eruption sites. Here, …

2017 Solar Physics
SOHO 12
IRTF/TEXES observations of the H II regions H1 and H2 in the Galactic Centre
DOI: 10.1093/mnras/stx1266 Bibcode: 2017MNRAS.470..561D

Wang, Q. Daniel; Dong, Hui; Schödel, Rainer +6 more

We present new [Ne II] (12.8 µm) IRTF/TEXES observations of the Galactic Center H II regions H1 and H2, which are at a projected distance of ∼11 pc from the centre of the Galaxy. The new observations allow us to map the radial velocity distributions of ionized gas. The high spectroscopic resolution (∼4 km s-1) helps us to disentan…

2017 Monthly Notices of the Royal Astronomical Society
eHST 12
Whistler Mode Waves Below Lower Hybrid Resonance Frequency: Generation and Spectral Features
DOI: 10.1002/2017JA024416 Bibcode: 2017JGRA..12210072S

Balikhin, M. A.; Shklyar, D. R.

Equatorial noise in the frequency range below the lower hybrid resonance frequency, whose structure is shaped by high proton cyclotron harmonics, has been observed by the Cluster spacecraft. We develop a model of this wave phenomenon which assumes (as, in general, has been suggested long ago) that the observed spectrum is excited due to loss cone …

2017 Journal of Geophysical Research (Space Physics)
Cluster 12