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Evaluating the Morphology of the Local Interstellar Medium: Using New Data to Distinguish between Multiple Discrete Clouds and a Continuous Medium
DOI: 10.1088/0004-637X/812/2/125 Bibcode: 2015ApJ...812..125R

Redfield, Seth; Linsky, Jeffrey L.

Ultraviolet and optical spectra of interstellar gas along the lines of sight to nearby stars have been interpreted by Redfield & Linsky and previous studies as a set of discrete warm, partially ionized clouds each with a different flow vector, temperature, and metal depletion. Recently, Gry & Jenkins proposed a fundamentally different mode…

2015 The Astrophysical Journal
eHST 26
First Infrared-Based Implications for the Dust Attenuation and Star Formation of Typical Lyα Emitters
DOI: 10.1088/2041-8205/800/2/L29 Bibcode: 2015ApJ...800L..29K

Ouchi, Masami; Shimasaku, Kazuhiro; Nakajima, Kimihiko +1 more

By stacking publicly available deep Spitzer/MIPS 24 µm and Herschel/PACS images for 213 z≃ 2.18 Lyα Emitters (LAEs) in GOODS-South, we obtain a strong upper limit to the IR luminosity of typical LAEs and discuss their attenuation curve for the first time. The 3σ upper limit LTIR = 1.1× {{10}10} {{L}⊙ …

2015 The Astrophysical Journal
Herschel eHST 26
The Absolute Age of the Globular Cluster M15 Using Near-infrared Adaptive Optics Images from PISCES/LBT.
DOI: 10.1088/0004-637X/812/1/25 Bibcode: 2015ApJ...812...25M

Boutsia, K.; Massari, D.; Arcidiacono, C. +26 more

We present deep near-infrared J, {K}{{s}} photometry of the old, metal-poor Galactic globular cluster M15 obtained with images collected with the LUCI1 and PISCES cameras available at the Large Binocular Telescope (LBT). We show how the use of First Light Adaptive Optics (FLAO) system coupled with the PISCES camera allows us to improve …

2015 The Astrophysical Journal
eHST 26
AKARI Observation of the Sub-degree Scale Fluctuation of the Near-infrared Background
DOI: 10.1088/0004-637X/807/2/140 Bibcode: 2015ApJ...807..140S

Lee, Hyung Mok; Lee, Myung Gyoon; Jeong, W. -S. +3 more

We report spatial fluctuation analysis of the sky brightness in the near-infrared from observations toward the north ecliptic pole (NEP) by the AKARI at 2.4 and 3.2 µm. As a follow-up study of our previous work on the Monitor field of AKARI, we used NEP deep survey data, which covered a circular area of about 0.4 square degrees, in order to …

2015 The Astrophysical Journal
AKARI 26
Interstellar Flow Longitude from the Symmetry of the Pickup Ion Cut-off at 1 AU
DOI: 10.1088/0004-637X/815/1/20 Bibcode: 2015ApJ...815...20M

Möbius, E.; Lee, M. A.; Drews, C.

We provide a proof of concept that the pickup ion (PUI) cutoff speed variation with ecliptic longitude can provide the interstellar neutral (ISN) flow longitude {λ }{ISN∞ } outside the heliosphere with a precision of the order of 0.°1. We compare 2007-2014 STEREO A PLASTIC observations in the solar wind frame with a simple analytical cu…

2015 The Astrophysical Journal
SOHO 25
Autoclassification of the Variable 3XMM Sources Using the Random Forest Machine Learning Algorithm
DOI: 10.1088/0004-637X/813/1/28 Bibcode: 2015ApJ...813...28F

Farrell, Sean A.; Murphy, Tara; Lo, Kitty K.

In the current era of large surveys and massive data sets, autoclassification of astrophysical sources using intelligent algorithms is becoming increasingly important. In this paper we present the catalog of variable sources in the Third XMM-Newton Serendipitous Source catalog (3XMM) autoclassified using the Random Forest machine learning algorith…

2015 The Astrophysical Journal
XMM-Newton 25
Weather on Other Worlds. III. A Survey for T Dwarfs with High-amplitude Optical Variability
DOI: 10.1088/0004-637X/801/2/104 Bibcode: 2015ApJ...801..104H

Metchev, Stanimir; Heinze, Aren N.; Kellogg, Kendra

We have monitored 12 T dwarfs with the Kitt Peak 2.1 m telescope using an F814W filter (0.7-0.95 µm) to place in context the remarkable 10%-20% variability exhibited by the nearby T dwarf Luhman 16B in this wavelength regime. The motivation was the poorly known red optical behavior of T dwarfs, which have been monitored almost exclusively at…

2015 The Astrophysical Journal
eHST 25
New Constraints on Cosmic Polarization Rotation from the ACTPol Cosmic Microwave Background B-mode Polarization Observation and the BICEP2 Constraint Update
DOI: 10.1088/0004-637X/805/2/107 Bibcode: 2015ApJ...805..107M

di Serego Alighieri, Sperello; Xu, Lixin; Mei, Hsien-Hao +2 more

Recently, ACTPol measured the cosmic microwave background (CMB) B-mode and E-mode polarizations and obtained TE, EE, BB, TB, and EB power spectra in the multipole range 225-8725. In our previous paper (Paper I), we jointly analyzed the results of three experiments on the CMB B-mode polarization—SPTpol, POLARBEAR, and BICEP2—to include in the model…

2015 The Astrophysical Journal
Planck 25
A Full Study on the Sun-Earth Connection of an Earth-directed CME Magnetic Flux Rope
DOI: 10.1088/0004-637X/814/1/59 Bibcode: 2015ApJ...814...59V

Vemareddy, Panditi; Mishra, Wageesh

We present an investigation of an eruption event of a coronal mass ejection (CME) magnetic flux rope (MFR) from the source active region (AR) NOAA 11719 on 2013 April 11 utilizing observations from the Solar Dynamic Observatory, the Solar Terrestrial Relations Observatory, the Solar and Heliospheric Observatory, and the WIND spacecraft. The source…

2015 The Astrophysical Journal
SOHO 25
Suzaku X-Ray Observations of the Fermi Bubbles: Northernmost Cap and Southeast Claw Discovered With MAXI-SSC
DOI: 10.1088/0004-637X/802/2/91 Bibcode: 2015ApJ...802...91T

Hiraga, J. S.; Cheung, C. C.; Kataoka, J. +8 more

We report on Suzaku observations of large-scale X-ray structures possibly related to the Fermi Bubbles obtained in 2013 with a total duration of ≃80 ks. The observed regions were (1) the northern cap (N-cap; l ∼ 0°, 45°\lt b\lt 55°) seen in the mid-band (1.7-4.0 keV) map recently provided by Monitor of All-sky X-ray Image Solid-state Slit Camera (…

2015 The Astrophysical Journal
Suzaku 25