Search Publications

Hubble Space Telescope Grism Spectroscopy of Extreme Starbursts across Cosmic Time: The Role of Dwarf Galaxies in the Star Formation History of the Universe
DOI: 10.1088/0004-637X/789/2/96 Bibcode: 2014ApJ...789...96A

Martin, Crystal L.; Teplitz, Harry I.; Bunker, Andrew J. +15 more

Near infrared slitless spectroscopy with the Wide Field Camera 3, on board the Hubble Space Telescope, offers a unique opportunity to study low-mass galaxy populations at high redshift (z ~ 1-2). While most high-z surveys are biased toward massive galaxies, we are able to select sources via their emission lines that have very faint continua. We in…

2014 The Astrophysical Journal
eHST 56
ALMA Observations of a Candidate Molecular Outflow in an Obscured Quasar
DOI: 10.1088/0004-637X/790/2/160 Bibcode: 2014ApJ...790..160S

Greene, Jenny E.; Zakamska, Nadia L.; Nesvadba, Nicole P. H. +1 more

We present Atacama Large Millimeter/Submillimeter Array CO (1-0) and CO (3-2) observations of SDSS J135646.10+102609.0, an obscured quasar and ultra-luminous infrared galaxy with two merging nuclei and a known 20 kpc scale ionized outflow. The total molecular gas mass is M_{mol}\approx 9^{+19}_{-6}\times 10^8 M , mostly distributed in …

2014 The Astrophysical Journal
Herschel eHST 56
Spatially Resolving the Very High Energy Emission from MGRO J2019+37 with VERITAS
DOI: 10.1088/0004-637X/788/1/78 Bibcode: 2014ApJ...788...78A

Fortin, P.; Reyes, L. C.; Aune, T. +80 more

We present very high energy (VHE) imaging of MGRO J2019+37 obtained with the VERITAS observatory. The bright extended (~2°) unidentified Milagro source is located toward the rich star formation region Cygnus-X. MGRO J2019+37 is resolved into two VERITAS sources. The faint, point-like source VER J2016+371 overlaps CTB 87, a filled-center remnant (S…

2014 The Astrophysical Journal
XMM-Newton 55
A Rigorous Free-form Lens Model of A2744 to Meet the Hubble Frontier Fields Challenge
DOI: 10.1088/0004-637X/797/2/98 Bibcode: 2014ApJ...797...98L

Broadhurst, Tom; Zheng, Wei; Coe, Dan +4 more

Hubble Frontier Fields (HFF) imaging of the most powerful lensing clusters provides access to the most magnified distant galaxies. The challenge is to construct lens models capable of describing these complex massive, merging clusters so that individual lensed systems can be reliably identified and their intrinsic properties accurately derived. We…

2014 The Astrophysical Journal
eHST 55
The Onset of Spiral Structure in the Universe
DOI: 10.1088/0004-637X/781/1/11 Bibcode: 2014ApJ...781...11E

Elmegreen, Bruce G.; Elmegreen, Debra Meloy

The onset of spiral structure in galaxies appears to occur between redshifts 1.4 and 1.8 when disks have developed a cool stellar component, rotation dominates over turbulent motions in the gas, and massive clumps become less frequent. During the transition from clumpy to spiral disks, two unusual types of spirals are found in the Hubble Ultra Dee…

2014 The Astrophysical Journal
eHST 55
The Solar Wind Neon Abundance Observed with ACE/SWICS and Ulysses/SWICS
DOI: 10.1088/0004-637X/789/1/60 Bibcode: 2014ApJ...789...60S

Landi, Enrico; Zurbuchen, Thomas H.; von Steiger, Rudolf +5 more

Using in situ ion spectrometry data from ACE/SWICS, we determine the solar wind Ne/O elemental abundance ratio and examine its dependence on wind speed and evolution with the solar cycle. We find that Ne/O is inversely correlated with wind speed, is nearly constant in the fast wind, and correlates strongly with solar activity in the slow wind. In …

2014 The Astrophysical Journal
Ulysses 55
The Star-forming Galaxy Contribution to the Cosmic MeV and GeV Gamma-Ray Background
DOI: 10.1088/0004-637X/786/1/40 Bibcode: 2014ApJ...786...40L

Beacom, John F.; Horiuchi, Shunsaku; Lacki, Brian C.

Star-forming galaxies could be major contributors to the cosmic GeV γ-ray background, and they are expected to be MeV-dim because of the "pion bump" falling off below ~100 MeV. However, there are very few observations of galaxies in the MeV range and other emission processes could be present. We investigate the MeV background from star-forming gal…

2014 The Astrophysical Journal
INTEGRAL 55
An Unorthodox X-Class Long-duration Confined Flare
DOI: 10.1088/0004-637X/790/1/8 Bibcode: 2014ApJ...790....8L

Wang, Haimin; Wang, Yuming; Liu, Rui +3 more

We report the observation of an X-class long-duration flare which is clearly confined. It appears as a compact-loop flare in the traditional EUV passbands (171 and 195 Å), but in the passbands sensitive to flare plasmas (94 and 131 Å), it exhibits a cusp-shaped structure above an arcade of loops like other long-duration events. Inspecting images i…

2014 The Astrophysical Journal
SOHO 55
The SCUBA-2 Cosmology Legacy Survey: Ultraluminous Star-forming Galaxies in a z = 1.6 Cluster
DOI: 10.1088/0004-637X/782/1/19 Bibcode: 2014ApJ...782...19S

Thomson, A. P.; Ivison, R. J.; Scott, D. +23 more

We analyze new SCUBA-2 submillimeter and archival SPIRE far-infrared imaging of a z = 1.62 cluster, Cl 0218.3-0510, which lies in the UKIRT Infrared Deep Sky Survey/Ultra-Deep Survey field of the SCUBA-2 Cosmology Legacy Survey. Combining these tracers of obscured star-formation activity with the extensive photometric and spectroscopic information…

2014 The Astrophysical Journal
Herschel 55
The Puzzling Chemical Composition of GJ 436b's Atmosphere: Influence of Tidal Heating on the Chemistry
DOI: 10.1088/0004-637X/781/2/68 Bibcode: 2014ApJ...781...68A

Agúndez, Marcelino; Venot, Olivia; Iro, Nicolas +1 more

The dissipation of the tidal energy deposited on eccentric planets may induce a heating of the planet that affects its atmospheric thermal structure. Here we study the influence of tidal heating on the atmospheric composition of the eccentric (e = 0.16) "hot Neptune" GJ 436b, for which inconclusive chemical abundances are retrieved from multiwavel…

2014 The Astrophysical Journal
eHST 55