Search Publications

Emerging trends and a comet taxonomy based on the volatile chemistry measured in thirty comets with high-resolution infrared spectroscopy between 1997 and 2013
DOI: 10.1016/j.icarus.2016.05.039 Bibcode: 2016Icar..278..301D

Weaver, Harold A.; Vervack, Ronald J.; Kawakita, Hideyo +1 more

A systematic analysis of the mixing ratios with respect to H2O for eight species (CH3OH, HCN, NH3, H2CO, C2H2, C2H6, CH4, and CO) measured with high-resolution infrared spectroscopy in thirty comets between 1997 and 2013 is presented. Some trends are…

2016 Icarus
eHST 129
ISM Excitation and Metallicity of Star-forming Galaxies at z ≃ 3.3 from Near-IR Spectroscopy
DOI: 10.3847/0004-637X/822/1/42 Bibcode: 2016ApJ...822...42O

Daddi, E.; Capak, P.; Carollo, C. M. +8 more

We study the relationship between stellar mass, star formation rate (SFR), ionization state, and gas-phase metallicity for a sample of 41 normal star-forming galaxies at 3 ≲ z ≲ 3.7. The gas-phase oxygen abundance, ionization parameter, and electron density of ionized gas are derived from rest-frame optical strong emission lines measured on near-i…

2016 The Astrophysical Journal
eHST 129
Morphologies of ~190,000 Galaxies at z = 0-10 Revealed with HST Legacy Data. II. Evolution of Clumpy Galaxies
DOI: 10.3847/0004-637X/821/2/72 Bibcode: 2016ApJ...821...72S

Ouchi, Masami; Harikane, Yuichi; Shibuya, Takatoshi +1 more

We investigate the evolution of clumpy galaxies with Hubble Space Telescope (HST) samples of ∼17,000 photo-z and Lyman break galaxies at z ≃ 0-8. We detect clumpy galaxies with off-center clumps in a self-consistent algorithm that is well tested with previous study results, and we measure the number fraction of clumpy galaxies at the rest-frame UV…

2016 The Astrophysical Journal
eHST 129
Coalescence of magnetic flux ropes in the ion diffusion region of magnetic reconnection
DOI: 10.1038/nphys3578 Bibcode: 2016NatPh..12..263W

Wang, Shui; Huang, Can; Guo, Fan +7 more

Merging magnetic flux ropes, which are believed to play an important role in magnetic reconnection, have now been clearly identified. Observations show that coalescence is indeed closely related to reconnection dynamics and also to turbulence.

2016 Nature Physics
Cluster 129
Measurements of Extragalactic Background Light from the Far UV to the Far IR from Deep Ground- and Space-based Galaxy Counts
DOI: 10.3847/0004-637X/827/2/108 Bibcode: 2016ApJ...827..108D

Cohen, Seth; Driver, Simon P.; Robotham, Aaron S. G. +7 more

We combine wide and deep galaxy number-count data from the Galaxy And Mass Assembly, COSMOS/G10, Hubble Space Telescope (HST) Early Release Science, HST UVUDF, and various near-, mid-, and far-IR data sets from ESO, Spitzer, and Herschel. The combined data range from the far UV (0.15 µm) to far-IR (500 µm), and in all cases the contrib…

2016 The Astrophysical Journal
Herschel eHST 128
How Isotropic is the Universe?
DOI: 10.1103/PhysRevLett.117.131302 Bibcode: 2016PhRvL.117m1302S

Peiris, Hiranya V.; Feeney, Stephen M.; Pontzen, Andrew +2 more

A fundamental assumption in the standard model of cosmology is that the Universe is isotropic on large scales. Breaking this assumption leads to a set of solutions to Einstein's field equations, known as Bianchi cosmologies, only a subset of which have ever been tested against data. For the first time, we consider all degrees of freedom in these s…

2016 Physical Review Letters
Planck 128
High-molecular-weight organic matter in the particles of comet 67P/Churyumov-Gerasimenko
DOI: 10.1038/nature19320 Bibcode: 2016Natur.538...72F

Krüger, Harald; Haerendel, Gerhard; Langevin, Yves +39 more

The presence of solid carbonaceous matter in cometary dust was established by the detection of elements such as carbon, hydrogen, oxygen and nitrogen in particles from comet 1P/Halley. Such matter is generally thought to have originated in the interstellar medium, but it might have formed in the solar nebula—the cloud of gas and dust that was left…

2016 Nature
Rosetta 126
Line strengths of rovibrational and rotational transitions in the X2 Π ground state of OH
DOI: 10.1016/j.jqsrt.2015.07.021 Bibcode: 2016JQSRT.168..142B

Li, Gang; Afşar, Melike; Sneden, Christopher +4 more

A new line list including positions and absolute transition strengths (in the form of Einstein A values and oscillator strengths) has been produced for the OH ground X2 Π state rovibrational (Meinel system) and pure rotational transitions. All possible transitions are included with v and v ″ up to 13, and J up to between 9.5…

2016 Journal of Quantitative Spectroscopy and Radiative Transfer
VenusExpress 126
The Swift Gamma-Ray Burst Host Galaxy Legacy Survey. I. Sample Selection and Redshift Distribution
DOI: 10.3847/0004-637X/817/1/7 Bibcode: 2016ApJ...817....7P

Cenko, S. B.; Greiner, J.; Berger, E. +20 more

We introduce the Swift Gamma-Ray Burst Host Galaxy Legacy Survey (“SHOALS”), a multi-observatory high-redshift galaxy survey targeting the largest unbiased sample of long-duration gamma-ray burst (GRB) hosts yet assembled (119 in total). We describe the motivations of the survey and the development of our selection criteria, including an assessmen…

2016 The Astrophysical Journal
eHST 126
Planck intermediate results. XLII. Large-scale Galactic magnetic fields
DOI: 10.1051/0004-6361/201528033 Bibcode: 2016A&A...596A.103P

Miville-Deschênes, M. -A.; Boulanger, F.; Bernard, J. -P. +175 more

Recent models for the large-scale Galactic magnetic fields in the literature have been largely constrained by synchrotron emission and Faraday rotation measures. We use three different but representative models to compare their predicted polarized synchrotron and dust emission with that measured by the Planck satellite. We first update these model…

2016 Astronomy and Astrophysics
Planck 125