Search Publications

Observational Constraints on Planet Nine: Cassini Range Observations
DOI: 10.3847/0004-6256/152/4/94 Bibcode: 2016AJ....152...94H

Holman, Matthew J.; Payne, Matthew J.

We examine the tidal perturbations induced by a possible additional, distant planet in the solar system on the distance between the Earth and the Cassini spacecraft. We find that measured range residuals alone can significantly constrain the sky position, distance, and mass of the perturbing planet to sections of the sky essentially orthogonal to …

2016 The Astronomical Journal
Cassini 43
NuSTAR and XMM-Newton Observations of the Hard X-Ray Spectrum of Centaurus A
DOI: 10.3847/0004-637X/819/2/150 Bibcode: 2016ApJ...819..150F

Harrison, F. A.; Stern, D.; Farrah, D. +28 more

We present simultaneous XMM-Newton and Nuclear Spectroscopic Telescope Array (NuSTAR) observations spanning 3-78 keV of the nearest radio galaxy, Centaurus A (Cen A). The accretion geometry around the central engine in Cen A is still debated, and we investigate possible configurations using detailed X-ray spectral modeling. NuSTAR imaged the centr…

2016 The Astrophysical Journal
XMM-Newton 43
Planck intermediate results. XLIII. Spectral energy distribution of dust in clusters of galaxies
DOI: 10.1051/0004-6361/201628522 Bibcode: 2016A&A...596A.104P

Kneissl, R.; Miville-Deschênes, M. -A.; Planck Collaboration +179 more

Although infrared (IR) overall dust emission from clusters of galaxies has been statistically detected using data from the Infrared Astronomical Satellite (IRAS), it has not been possible to sample the spectral energy distribution (SED) of this emission over its peak, and thus to break the degeneracy between dust temperature and mass. By complemen…

2016 Astronomy and Astrophysics
Planck 43
Constraints on the running of the running of the scalar tilt from CMB anisotropies and spectral distortions
DOI: 10.1103/PhysRevD.94.023523 Bibcode: 2016PhRvD..94b3523C

Di Valentino, Eleonora; Melchiorri, Alessandro; Cabass, Giovanni +2 more

We use the recent observations of cosmic microwave background (CMB) temperature and polarization anisotropies provided by the Planck satellite experiment to place constraints on the running αs=d ns/d log k and the running of the running βs=d αs/d log k of the spectral index ns of primordial sc…

2016 Physical Review D
Planck 43
A Search for an Optical Counterpart to the Gravitational-wave Event GW151226
DOI: 10.3847/2041-8205/827/2/L40 Bibcode: 2016ApJ...827L..40S

Della Valle, M.; Sollerman, J.; Gal-Yam, A. +37 more

We present a search for an electromagnetic counterpart of the gravitational-wave source GW151226. Using the Pan-STARRS1 telescope we mapped out 290 square degrees in the optical I P1 filter, starting 11.5 hr after the LIGO information release and lasting for an additional 28 days. The first observations started 49.5 hr after the time of…

2016 The Astrophysical Journal
eHST 43
The SOPHIE search for northern extrasolar planets. IX. Populating the brown dwarf desert
DOI: 10.1051/0004-6361/201527581 Bibcode: 2016A&A...588A.144W

Bouchy, F.; Deleuil, M.; Moutou, C. +20 more

Radial velocity planet search surveys of nearby solar-type stars have shown a strong scarcity of brown dwarf companions within ~5 AU. There is presently no comprehensive explanation for this lack of brown dwarf companions; therefore, increasing the sample of such objects is crucial to understand their formation and evolution. Based on precise radi…

2016 Astronomy and Astrophysics
Hipparcos 43
The Hubble Space Telescope UV Legacy Survey of Galactic globular clusters - X. The radial distribution of stellar populations in NGC 2808
DOI: 10.1093/mnras/stw2003 Bibcode: 2016MNRAS.463..449S

Milone, A. P.; Bedin, L. R.; Piotto, G. +4 more

Due to their extreme helium abundance, the multiple stellar populations of the globular cluster NGC 2808 have been widely investigated from a photometric, spectroscopic, and kinematic perspective. The most striking feature of the colour-magnitude diagram of NGC 2808 is the triple main sequence (MS), with the red MS corresponding to a stellar popul…

2016 Monthly Notices of the Royal Astronomical Society
eHST 43
Lighting the Dark Molecular Gas: H2 as a Direct Tracer
DOI: 10.3847/0004-637X/830/1/18 Bibcode: 2016ApJ...830...18T

Togi, Aditya; Smith, J. D. T.

Robust knowledge of molecular gas mass is critical for understanding star formation in galaxies. The {{{H}}}2 molecule does not emit efficiently in the cold interstellar medium, hence the molecular gas content of galaxies is typically inferred using indirect tracers. At low metallicity and in other extreme environments, these tracers ca…

2016 The Astrophysical Journal
Herschel 43
Extreme star formation events in quasar hosts over 0.5 < z < 4
DOI: 10.1093/mnras/stw1840 Bibcode: 2016MNRAS.462.4067P

Wang, L.; Feltre, A.; Hatziminaoglou, E. +7 more

We explore the relationship between active galactic nuclei (AGN) and star formation in a sample of 513 optically luminous type 1 quasars up to redshifts of ∼4 hosting extremely high star formation rates (SFRs). The quasars are selected to be individually detected by the Herschel SPIRE instrument at >3σ at 250 µm, leading to typical SFRs o…

2016 Monthly Notices of the Royal Astronomical Society
Herschel 43
Towards the statistical detection of the warm-hot intergalactic medium in intercluster filaments of the cosmic web
DOI: 10.1093/mnras/stv2376 Bibcode: 2016MNRAS.455.2662T

Prochaska, J. Xavier; Tejos, Nicolas; Morris, Simon L. +6 more

Modern analyses of structure formation predict a universe tangled in a `cosmic web' of dark matter and diffuse baryons. These theories further predict that at low z, a significant fraction of the baryons will be shock-heated to T ∼ 105-107 K yielding a warm-hot intergalactic medium (WHIM), but whose actual existence has elude…

2016 Monthly Notices of the Royal Astronomical Society
eHST 43