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NuSTAR Reveals an Intrinsically X-Ray Weak Broad Absorption Line Quasar in the Ultraluminous Infrared Galaxy Markarian 231
DOI: 10.1088/0004-637X/785/1/19 Bibcode: 2014ApJ...785...19T

Rigby, J. R.; Veilleux, S.; Harrison, F. A. +24 more

We present high-energy (3-30 keV) NuSTAR observations of the nearest quasar, the ultraluminous infrared galaxy (ULIRG) Markarian 231 (Mrk 231), supplemented with new and simultaneous low-energy (0.5-8 keV) data from Chandra. The source was detected, though at much fainter levels than previously reported, likely due to contamination in the large ap…

2014 The Astrophysical Journal
XMM-Newton 87
Globular Cluster Systems in Brightest Cluster Galaxies: A Near-universal Luminosity Function?
DOI: 10.1088/0004-637X/797/2/128 Bibcode: 2014ApJ...797..128H

Bailin, Jeremy; Whitmore, Bradley C.; Côté, Patrick +10 more

We present the first results from our Hubble Space Telescope brightest cluster galaxy (BCG) survey of seven central supergiant cluster galaxies and their globular cluster (GC) systems. We measure a total of 48,000 GCs in all seven galaxies, representing the largest single GC database. We find that a log-normal shape accurately matches the observed…

2014 The Astrophysical Journal
eHST 86
Observations of Environmental Quenching in Groups in the 11 GYR since z = 2.5: Different Quenching for Central and Satellite Galaxies
DOI: 10.1088/0004-637X/789/2/164 Bibcode: 2014ApJ...789..164T

van Dokkum, Pieter G.; Franx, Marijn; Illingworth, Garth D. +16 more

We present direct observational evidence for star formation quenching in galaxy groups in the redshift range 0 < z < 2.5. We utilize a large sample of nearly 6000 groups, selected by fixed cumulative number density from three photometric catalogs, to follow the evolving quiescent fractions of central and satellite galaxies over roughly 11 Gy…

2014 The Astrophysical Journal
eHST 86
Measurement of Galaxy Clustering at z ~ 7.2 and the Evolution of Galaxy Bias from 3.8 < z < 8 in the XDF, GOODS-S, and GOODS-N
DOI: 10.1088/0004-637X/793/1/17 Bibcode: 2014ApJ...793...17B

Trenti, M.; Oesch, P. A.; Carollo, C. M. +8 more

Lyman-break galaxy (LBG) samples observed during reionization (z >~ 6) with the Hubble Space Telescope's Wide Field Camera 3 are reaching sizes sufficient to characterize their clustering properties. Using a combined catalog from the Hubble eXtreme Deep Field and CANDELS surveys, containing N = 743 LBG candidates at z >= 6.5 at a mean redshi…

2014 The Astrophysical Journal
eHST 86
Evolution of Thermally Pulsing Asymptotic Giant Branch Stars. IV. Constraining Mass loss and Lifetimes of Low Mass, Low Metallicity AGB Stars
DOI: 10.1088/0004-637X/790/1/22 Bibcode: 2014ApJ...790...22R

Williams, Benjamin F.; Dolphin, Andrew; Girardi, Léo +7 more

The evolution and lifetimes of thermally pulsating asymptotic giant branch (TP-AGB) stars suffer from significant uncertainties. In this work, we analyze the numbers and luminosity functions of TP-AGB stars in six quiescent, low metallicity ([Fe/H] <~ -0.86) galaxies taken from the ACS Nearby Galaxy Survey Treasury sample, using Hubble Space Te…

2014 The Astrophysical Journal
eHST 86
Carbon-rich Dust Past the Asymptotic Giant Branch: Aliphatics, Aromatics, and Fullerenes in the Magellanic Clouds
DOI: 10.1088/0004-637X/791/1/28 Bibcode: 2014ApJ...791...28S

Sahai, R.; Zijlstra, A. A.; Peeters, E. +10 more

Infrared spectra of carbon-rich objects that have evolved off the asymptotic giant branch reveal a range of dust properties, including fullerenes, polycyclic aromatic hydrocarbons (PAHs), aliphatic hydrocarbons, and several unidentified features, including the 21 µm emission feature. To test for the presence of fullerenes, we used the positi…

2014 The Astrophysical Journal
ISO 85
The INTEGRAL High-energy Cut-off Distribution of Type 1 Active Galactic Nuclei
DOI: 10.1088/2041-8205/782/2/L25 Bibcode: 2014ApJ...782L..25M

Bird, A. J.; Ubertini, P.; Malizia, A. +4 more

In this Letter we present the primary continuum parameters, the photon index Γ, and the high-energy cut-off E c of 41 type-1 Seyfert galaxies extracted from the International Gamma-Ray Astrophysics Laboratory (INTEGRAL) complete sample of active galactic nuclei (AGNs). We performed broadband (0.3-100 keV) spectral analysis by simultaneo…

2014 The Astrophysical Journal
INTEGRAL XMM-Newton 85
Disintegrating Asteroid P/2013 R3
DOI: 10.1088/2041-8205/784/1/L8 Bibcode: 2014ApJ...784L...8J

Mutchler, Max; Jewitt, David; Agarwal, Jessica +3 more

Splitting of the nuclei of comets into multiple components has been frequently observed but, to date, no main-belt asteroid has been observed to break up. Using the Hubble Space Telescope, we find that main-belt asteroid P/2013 R3 consists of 10 or more distinct components, the largest up to 200 m in radius (assumed geometric albedo of 0.05) each …

2014 The Astrophysical Journal
eHST 85
The Light Curve of SN 1987A Revisited: Constraining Production Masses of Radioactive Nuclides
DOI: 10.1088/0004-637X/792/1/10 Bibcode: 2014ApJ...792...10S

Seitenzahl, Ivo R.; Timmes, F. X.; Magkotsios, Georgios

We revisit the evidence for the contribution of the long-lived radioactive nuclides 44Ti, 55Fe, 56Co, 57Co, and 60Co to the UVOIR light curve of SN 1987A. We show that the V-band luminosity constitutes a roughly constant fraction of the bolometric luminosity between 900 and 1900 days, and we o…

2014 The Astrophysical Journal
INTEGRAL 84
NuSTAR and XMM-NEWTON Observations of NGC 1365: Extreme Absorption Variability and a Constant Inner Accretion Disk
DOI: 10.1088/0004-637X/788/1/76 Bibcode: 2014ApJ...788...76W

Harrison, F. A.; Stern, D.; Zhang, W. W. +24 more

We present a spectral analysis of four coordinated NuSTAR+XMM-Newton observations of the Seyfert galaxy NGC 1365. These exhibit an extreme level of spectral variability, which is primarily due to variable line-of-sight absorption, revealing relatively unobscured states in this source for the first time. Despite the diverse range of absorption stat…

2014 The Astrophysical Journal
XMM-Newton 84