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The XMM-Newton serendipitous survey. VII. The third XMM-Newton serendipitous source catalogue
DOI: 10.1051/0004-6361/201526416 Bibcode: 2016A&A...590A...1R

Esquej, P.; Motch, C.; Ballet, J. +37 more

Context. Thanks to the large collecting area (3 ×~1500 cm2 at 1.5 keV) and wide field of view (30' across in full field mode) of the X-ray cameras on board the European Space Agency X-ray observatory XMM-Newton, each individual pointing can result in the detection of up to several hundred X-ray sources, most of which are newly discovere…

2016 Astronomy and Astrophysics
XMM-Newton 338
Dark energy at early times, the Hubble parameter, and the string axiverse
DOI: 10.1103/PhysRevD.94.103523 Bibcode: 2016PhRvD..94j3523K

Kamionkowski, Marc; Karwal, Tanvi

Precise measurements of the cosmic microwave background (CMB) power spectrum are in excellent agreement with the predictions of the standard Λ CDM cosmological model. However, there is some tension between the value of the Hubble parameter H0 inferred from the CMB and that inferred from observations of the Universe at lower redshifts, a…

2016 Physical Review D
Planck 338
Discovery of Coherent Pulsations from the Ultraluminous X-Ray Source NGC 7793 P13
DOI: 10.3847/2041-8205/831/2/L14 Bibcode: 2016ApJ...831L..14F

Harrison, F. A.; Ptak, A.; Stern, D. +12 more

We report the detection of coherent pulsations from the ultraluminous X-ray source (ULX) NGC 7793 P13. The ≈0.42 s nearly sinusoidal pulsations were initially discovered in broadband X-ray observations using XMM-Newton and NuSTAR taken in 2016. We subsequently also found pulsations in archival XMM-Newton data taken in 2013 and 2014. The significan…

2016 The Astrophysical Journal
XMM-Newton 337
Large gradual solar energetic particle events
DOI: 10.1007/s41116-016-0002-5 Bibcode: 2016LRSP...13....3D

Giacalone, Joe; Desai, Mihir

Solar energetic particles, or SEPs, from suprathermal (few keV) up to relativistic (few GeV) energies are accelerated near the Sun in at least two ways: (1) by magnetic reconnection-driven processes during solar flares resulting in impulsive SEPs, and (2) at fast cor…

2016 Living Reviews in Solar Physics
SOHO 336
Reconciling Planck with the local value of H0 in extended parameter space
DOI: 10.1016/j.physletb.2016.08.043 Bibcode: 2016PhLB..761..242D

Di Valentino, Eleonora; Melchiorri, Alessandro; Silk, Joseph

The recent determination of the local value of the Hubble constant by Riess et al., 2016 (hereafter R16) is now 3.3 sigma higher than the value derived from the most recent CMB anisotropy data provided by the Planck satellite in a ΛCDM model. Here we perform a combined analysis of the Planck and R16 results in an extended parameter space, varying …

2016 Physics Letters B
Planck 335
The MUSCLES Treasury Survey. I. Motivation and Overview
DOI: 10.3847/0004-637X/820/2/89 Bibcode: 2016ApJ...820...89F

Loyd, R. O. Parke; Kowalski, Adam F.; Hawley, Suzanne L. +19 more

Ground- and space-based planet searches employing radial velocity techniques and transit photometry have detected thousands of planet-hosting stars in the Milky Way. With so many planets discovered, the next step toward identifying potentially habitable planets is atmospheric characterization. While the Sun-Earth system provides a good framework f…

2016 The Astrophysical Journal
IUE XMM-Newton eHST 335
Optimal binning of X-ray spectra and response matrix design
DOI: 10.1051/0004-6361/201527395 Bibcode: 2016A&A...587A.151K

Kaastra, J. S.; Bleeker, J. A. M.


Aims: A theoretical framework is developed to estimate the optimal binning of X-ray spectra.
Methods: We derived expressions for the optimal bin size for model spectra as well as for observed data using different levels of sophistication.
Results: It is shown that by taking into account both the number of photons in a given spectral…

2016 Astronomy and Astrophysics
XMM-Newton 325
The Evolution of the Galaxy Stellar Mass Function at z = 4-8: A Steepening Low-mass-end Slope with Increasing Redshift
DOI: 10.3847/0004-637X/825/1/5 Bibcode: 2016ApJ...825....5S

Papovich, Casey; Finkelstein, Steven L.; Dickinson, Mark +16 more

We present galaxy stellar mass functions (GSMFs) at z = 4-8 from a rest-frame ultraviolet (UV) selected sample of ∼4500 galaxies, found via photometric redshifts over an area of ∼280 arcmin2 in the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (CANDELS)/Great Observatories Origins Deep Survey (GOODS) fields and the Hubb…

2016 The Astrophysical Journal
eHST 323
Spectral Properties of Cool Stars: Extended Abundance Analysis of 1,617 Planet-search Stars
DOI: 10.3847/0067-0049/225/2/32 Bibcode: 2016ApJS..225...32B

Valenti, Jeff A.; Fischer, Debra A.; Brewer, John M. +1 more

We present a catalog of uniformly determined stellar properties and abundances for 1,617 F, G, and K stars using an automated spectral synthesis modeling procedure. All stars were observed using the HIRES spectrograph at Keck Observatory. Our procedure used a single line list to fit model spectra to observations of all stars to determine effective…

2016 The Astrophysical Journal Supplement Series
Hipparcos 320
The RedMaPPer Galaxy Cluster Catalog From DES Science Verification Data
DOI: 10.3847/0067-0049/224/1/1 Bibcode: 2016ApJS..224....1R

Benoit-Lévy, A.; Nichol, R. C.; D'Andrea, C. B. +87 more

We describe updates to the redMaPPer algorithm, a photometric red-sequence cluster finder specifically designed for large photometric surveys. The updated algorithm is applied to 150 {{deg}}2 of Science Verification (SV) data from the Dark Energy Survey (DES), and to the Sloan Digital Sky Survey (SDSS) DR8 photometric data set. The DES …

2016 The Astrophysical Journal Supplement Series
XMM-Newton 320