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The Redshift Evolution of the Mean Temperature, Pressure, and Entropy Profiles in 80 SPT-Selected Galaxy Clusters
DOI: 10.1088/0004-637X/794/1/67 Bibcode: 2014ApJ...794...67M

Gladders, M. D.; Rest, A.; Foley, R. J. +63 more

We present the results of an X-ray analysis of 80 galaxy clusters selected in the 2500 deg2 South Pole Telescope survey and observed with the Chandra X-ray Observatory. We divide the full sample into subsamples of ~20 clusters based on redshift and central density, performing a joint X-ray spectral fit to all clusters in a subsample sim…

2014 The Astrophysical Journal
Planck 116
Three Wide Planetary-mass Companions to FW Tau, ROXs 12, and ROXs 42B
DOI: 10.1088/0004-637X/781/1/20 Bibcode: 2014ApJ...781...20K

Hinkley, Sasha; Dupuy, Trent J.; Ireland, Michael J. +4 more

We report the discovery of three planetary-mass companions (M = 6-20 M Jup) in wide orbits (ρ ~ 150-300 AU) around the young stars FW Tau (Taurus-Auriga), ROXs 12 (Ophiuchus), and ROXs 42B (Ophiuchus). All three wide planetary-mass companions (PMCs) were reported as candidate companions in previous binary survey programs, but then were …

2014 The Astrophysical Journal
eHST 116
Herschel Observations of Extraordinary Sources: Analysis of the HIFI 1.2 THz Wide Spectral Survey toward Orion KL. I. Methods
DOI: 10.1088/0004-637X/787/2/112 Bibcode: 2014ApJ...787..112C

Cernicharo, José; McGuire, Brett A.; Bergin, Edwin A. +19 more

We present a comprehensive analysis of a broadband spectral line survey of the Orion Kleinmann-Low nebula (Orion KL), one of the most chemically rich regions in the Galaxy, using the HIFI instrument on board the Herschel Space Observatory. This survey spans a frequency range from 480 to 1907 GHz at a resolution of 1.1 MHz. These observations thus …

2014 The Astrophysical Journal
Herschel 115
The Lyα Reference Sample. I. Survey Outline and First Results for Markarian 259
DOI: 10.1088/0004-637X/797/1/11 Bibcode: 2014ApJ...797...11O

Verhamme, Anne; Cannon, John M.; Hayes, Matthew +20 more

The Lyα Reference Sample (LARS) is a substantial program with the Hubble Space Telescope (HST) that provides a sample of local universe laboratory galaxies in which to study the detailed astrophysics of the visibility and strength of the Lyαline of neutral hydrogen. Lyα is the dominant spectral line in use for characterizing high-redshift (z) gala…

2014 The Astrophysical Journal
eHST 115
High-resolution Observations of the Shock Wave Behavior for Sunspot Oscillations with the Interface Region Imaging Spectrograph
DOI: 10.1088/0004-637X/786/2/137 Bibcode: 2014ApJ...786..137T

Weber, M.; Golub, L.; Tian, H. +20 more

We present the first results of sunspot oscillations from observations by the Interface Region Imaging Spectrograph. The strongly nonlinear oscillation is identified in both the slit-jaw images and the spectra of several emission lines formed in the transition region and chromosphere. We first apply a single Gaussian fit to the profiles of the Mg …

2014 The Astrophysical Journal
IRIS 113
CLASH: A Census of Magnified Star-forming Galaxies at z ~ 6-8
DOI: 10.1088/0004-637X/792/1/76 Bibcode: 2014ApJ...792...76B

Shu, X.; Infante, L.; Zheng, W. +34 more

We utilize 16 band Hubble Space Telescope (HST) observations of 18 lensing clusters obtained as part of the Cluster Lensing And Supernova survey with Hubble (CLASH) Multi-Cycle Treasury program to search for z ~ 6-8 galaxies. We report the discovery of 204, 45, and 13 Lyman-break galaxy candidates at z ~ 6, z ~ 7, and z ~ 8, respectively, identifi…

2014 The Astrophysical Journal
eHST 111
Global and Nonglobal Parameters of Horizontal-branch Morphology of Globular Clusters
DOI: 10.1088/0004-637X/785/1/21 Bibcode: 2014ApJ...785...21M

Milone, A. P.; Marino, A. F.; Sarajedini, A. +10 more

The horizontal-branch (HB) morphology of globular clusters (GCs) is mainly determined by metallicity. However, the fact that GCs with almost the same metallicity exhibit different HB morphologies demonstrates that at least one more parameter is needed to explain the HB morphology. It has been suggested that one of these should be a global paramete…

2014 The Astrophysical Journal
eHST 110
Broadband X-Ray Spectra of the Ultraluminous X-Ray Source Holmberg IX X-1 Observed with NuSTAR, XMM-Newton, and Suzaku
DOI: 10.1088/0004-637X/793/1/21 Bibcode: 2014ApJ...793...21W

Harrison, F. A.; Ptak, A.; Stern, D. +16 more

We present results from the coordinated broadband X-ray observations of the extreme ultraluminous X-ray source Holmberg IX X-1 performed by NuSTAR, XMM-Newton, and Suzaku in late 2012. These observations provide the first high-quality spectra of Holmberg IX X-1 above 10 keV to date, extending the X-ray coverage of this remarkable source up to ~30 …

2014 The Astrophysical Journal
Suzaku XMM-Newton 110
NuSTAR and XMM-Newton Observations of Luminous, Heavily Obscured, WISE-selected Quasars at z ~ 2
DOI: 10.1088/0004-637X/794/2/102 Bibcode: 2014ApJ...794..102S

Harrison, F. A.; Stern, D.; Zhang, W. W. +32 more

We report on a NuSTAR and XMM-Newton program that has observed a sample of three extremely luminous, heavily obscured WISE-selected active galactic nuclei (AGNs) at z ~ 2 across a broad X-ray band (0.1 - 79 keV). The parent sample, selected to be faint or undetected in the WISE 3.4 µm (W1) and 4.6 µm (W2) bands but bright at 12 µ…

2014 The Astrophysical Journal
XMM-Newton 110
The Peculiar Extinction Law of SN 2014J Measured with the Hubble Space Telescope
DOI: 10.1088/2041-8205/788/2/L21 Bibcode: 2014ApJ...788L..21A

Kulkarni, S. R.; Nugent, P. E.; Amanullah, R. +10 more

The wavelength dependence of the extinction of Type Ia SN 2014J in the nearby galaxy M82 has been measured using UV to near-IR photometry obtained with the Hubble Space Telescope, the Nordic Optical Telescope, and the Mount Abu Infrared Telescope. This is the first time that the reddening of an SN Ia is characterized over the full wavelength range…

2014 The Astrophysical Journal
eHST 109