Search Publications

The 2-79 keV X-Ray Spectrum of the Circinus Galaxy with NuSTAR, XMM-Newton, and Chandra: A Fully Compton-thick Active Galactic Nucleus
DOI: 10.1088/0004-637X/791/2/81 Bibcode: 2014ApJ...791...81A

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

The Circinus galaxy is one of the closest obscured active galactic nuclei (AGNs), making it an ideal target for detailed study. Combining archival Chandra and XMM-Newton data with new NuSTAR observations, we model the 2-79 keV spectrum to constrain the primary AGN continuum and to derive physical parameters for the obscuring material. Chandra's hi…

2014 The Astrophysical Journal
XMM-Newton 123
Planck intermediate results. XVI. Profile likelihoods for cosmological parameters
DOI: 10.1051/0004-6361/201323003 Bibcode: 2014A&A...566A..54P

Kneissl, R.; Miville-Deschênes, M. -A.; Bernard, J. -P. +182 more

We explore the 2013 Planck likelihood function with a high-precision multi-dimensional minimizer (Minuit). This allows a refinement of the ΛCDM best-fit solution with respect to previously-released results, and the construction of frequentist confidence intervals using profile likelihoods. The agreement with the cosmological results from the Bayes…

2014 Astronomy and Astrophysics
Planck 123
The Progenitors of the Compact Early-type Galaxies at High Redshift
DOI: 10.1088/0004-637X/780/1/1 Bibcode: 2014ApJ...780....1W

Barro, Guillermo; Bell, Eric F.; Ferguson, Henry C. +19 more

We use GOODS and CANDELS images to identify progenitors of massive (M > 1010 M ) compact early-type galaxies (ETGs) at z ~ 1.6. Because merging and accretion increase the size of the stellar component of galaxies, if the progenitors are among known star-forming galaxies, these must be compact themselves. We select candida…

2014 The Astrophysical Journal
eHST 122
The Identification of Filaments on Far-infrared and Submillimiter Images: Morphology, Physical Conditions and Relation with Star Formation of Filamentary Structure
DOI: 10.1088/0004-637X/791/1/27 Bibcode: 2014ApJ...791...27S

Paladini, R.; Moore, T. J. T.; Rygl, K. L. J. +12 more

Observations of molecular clouds reveal a complex structure, with gas and dust often arranged in filamentary, rather than spherical geometries. The association of pre- and proto-stellar cores with the filaments suggests a direct link with the process of star formation. Any study of the properties of such filaments requires representative samples f…

2014 The Astrophysical Journal
Herschel 122
Gas structure inside dust cavities of transition disks: Ophiuchus IRS 48 observed by ALMA
DOI: 10.1051/0004-6361/201322857 Bibcode: 2014A&A...562A..26B

van Dishoeck, Ewine F.; van der Marel, Nienke; Bruderer, Simon +1 more

Context. Transition disks are recognized by the absence of emission of small dust grains inside a radius of up to several 10s of AUs. Owing to the lack of angular resolution and sensitivity, the gas content of these dust holes has not yet been determined, but is of importance for constraining the mechanism leading to the dust holes. It is thought …

2014 Astronomy and Astrophysics
AKARI 122
The Rise of SN 2014J in the Nearby Galaxy M82
DOI: 10.1088/2041-8205/784/1/L12 Bibcode: 2014ApJ...784L..12G

Cenko, S. B.; Sollerman, J.; Bloom, J. S. +31 more

We report on the discovery of SN 2014J in the nearby galaxy M82. Given its proximity, it offers the best opportunity to date to study a thermonuclear supernova (SN) over a wide range of the electromagnetic spectrum. Optical, near-IR, and mid-IR observations on the rising light curve, orchestrated by the intermediate Palomar Transient Factory, show…

2014 The Astrophysical Journal
eHST 122
Neutrino cosmology and Planck
DOI: 10.1088/1367-2630/16/6/065002 Bibcode: 2014NJPh...16f5002L

Lesgourgues, Julien; Pastor, Sergio

Relic neutrinos play an important role in the evolution of the Universe, modifying some of the cosmological observables. We summarize the main aspects of cosmological neutrinos and describe how the precision of present cosmological data can be used to learn about neutrino properties. In particular, we discuss how cosmology provides information on …

2014 New Journal of Physics
Planck 121
The Solar Neighborhood. XXXIII. Parallax Results from the CTIOPI 0.9 m Program: Trigonometric Parallaxes of Nearby Low-mass Active and Young Systems
DOI: 10.1088/0004-6256/147/4/85 Bibcode: 2014AJ....147...85R

Gies, Douglas R.; Nelan, Edmund P.; Blunt, Sarah C. +14 more

We present basic observational data and association membership analysis for 45 young and active low-mass stellar systems from the ongoing Research Consortium On Nearby Stars photometry and astrometry program at the Cerro Tololo Inter-American Observatory. Most of these systems have saturated X-ray emission (log (LX /L bol) &g…

2014 The Astronomical Journal
eHST 121
Planck intermediate results. XIII. Constraints on peculiar velocities
DOI: 10.1051/0004-6361/201321299 Bibcode: 2014A&A...561A..97P

Dahle, H.; Miville-Deschênes, M. -A.; Bernard, J. -P. +182 more

Using Planck data combined with the Meta Catalogue of X-ray detected Clusters of galaxies (MCXC), we address the study of peculiar motions by searching for evidence of the kinetic Sunyaev-Zeldovich effect (kSZ). By implementing various filters designed to extract the kSZ generated at the positions of the clusters, we obtain consistent constraints …

2014 Astronomy and Astrophysics
Planck 121
Dense Cores in Galaxies Out to z = 2.5 in SDSS, UltraVISTA, and the Five 3D-HST/CANDELS Fields
DOI: 10.1088/0004-637X/791/1/45 Bibcode: 2014ApJ...791...45V

van Dokkum, Pieter G.; Muzzin, Adam; Labbé, Ivo +15 more

The dense interiors of massive galaxies are among the most intriguing environments in the universe. In this paper,we ask when these dense cores were formed and determine how galaxies gradually assembled around them. We select galaxies that have a stellar mass >3 × 1010 M inside r = 1 kpc out to z = 2.5, using the 3D-HST …

2014 The Astrophysical Journal
eHST 121