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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
The far-ultraviolet main auroral emission at Jupiter - Part 1: Dawn-dusk brightness asymmetries
DOI: 10.5194/angeo-33-1203-2015 Bibcode: 2015AnGeo..33.1203B

Khurana, K. K.; Badman, S. V.; Bonfond, B. +6 more

The main auroral emission at Jupiter generally appears as a quasi-closed curtain centered around the magnetic pole. This auroral feature, which accounts for approximately half of the total power emitted by the aurorae in the ultraviolet range, is related to corotation enforcement currents in the middle magnetosphere. Early models for these current…

2015 Annales Geophysicae
eHST 26
An HST/WFC3 view of stellar populations on the horizontal branch of NGC 2419
DOI: 10.1093/mnras/stu2167 Bibcode: 2015MNRAS.446.1469D

Di Criscienzo, M.; Milone, A. P.; D'Antona, F. +4 more

We use images acquired with the Hubble Space Telescope Wide Field Camera 3 and new models to probe the horizontal branch (HB) population of the Galactic globular cluster (GC) NGC 2419. A detailed analysis of the composite HB highlights three populations: (1) the blue luminous HB, hosting standard helium stars (Y = 0.25) with a very small spread of…

2015 Monthly Notices of the Royal Astronomical Society
eHST 26
Genus topology and cross-correlation of BICEP2 and Planck 353 GHz B-modes: further evidence favouring gravity wave detection
DOI: 10.1093/mnras/stu2547 Bibcode: 2015MNRAS.447.2034C

Colley, Wesley N.; Gott, J. Richard

We have analysed the genus topology of the BICEP2 B-modes and found them to be Gaussian random phase as expected if they have a cosmological origin. These BICEP2 B-modes can be produced by gravity waves in the early Universe, but question has arisen as to whether these B-modes (for 50 < l < 120) may instead be produced by foreground-polarize…

2015 Monthly Notices of the Royal Astronomical Society
Planck 26
Towards a fully consistent Milky Way disc model - III. Constraining the initial mass function
DOI: 10.1093/mnras/stu2734 Bibcode: 2015MNRAS.447.3880R

Rybizki, J.; Just, A.

We use our vertical Milky Way disc model together with Galaxia to create mock observations of stellar samples in the solar neighbourhood. We compare these to the corresponding volume complete observational samples of dereddened and binary accounted data from Hipparcos and the Catalogue of Nearby Stars. Sampling the likelihood in the parameter spac…

2015 Monthly Notices of the Royal Astronomical Society
Hipparcos 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
The Cepheid distance to the maser-host galaxy NGC 4258: studying systematics with the Large Binocular Telescope
DOI: 10.1093/mnras/stv881 Bibcode: 2015MNRAS.450.3597F

Kochanek, C. S.; Stanek, K. Z.; Fausnaugh, M. M. +3 more

We identify and phase a sample of 81 Cepheids in the maser-host galaxy NGC 4258 using the Large Binocular Telescope, and obtain calibrated mean magnitudes in up to four filters for a subset of 43 Cepheids using archival Hubble Space Telescope data. We employ three models to study the systematic effects of extinction, the assumed extinction law, an…

2015 Monthly Notices of the Royal Astronomical Society
eHST 25
From forced collapse to H ii region expansion in Mon R2: Envelope density structure and age determination with Herschel⋆
DOI: 10.1051/0004-6361/201526239 Bibcode: 2015A&A...584A...4D

Bernard, J. -P.; Hill, T.; White, G. J. +32 more

Context. The surroundings of H ii regions can have a profound influence on their development, morphology, and evolution. This paper explores the effect of the environment on H ii regions in the MonR2 molecular cloud.
Aims: We aim to investigate the density structure of envelopes surrounding H ii regions and to determine their collapse and ion…

2015 Astronomy and Astrophysics
Herschel 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