Search Publications

Scaling Relations Between Warm Galactic Outflows and Their Host Galaxies
DOI: 10.1088/0004-637X/811/2/149 Bibcode: 2015ApJ...811..149C

Chisholm, John; Leitherer, Claus; Chen, Yanmei +3 more

We report on a sample of 48 nearby, star-forming galaxies observed with the Cosmic Origin Spectrograph on the Hubble Space Telescope. We measure the kinematics of warm gas in galactic outflows using a combination of four Si ii absorption lines. We use multi-wavelength ancillary data to estimate stellar masses (M*), star formation rates …

2015 The Astrophysical Journal
eHST 145
X-Ray Constraints on the Local Supermassive Black Hole Occupation Fraction
DOI: 10.1088/0004-637X/799/1/98 Bibcode: 2015ApJ...799...98M

Treu, Tommaso; Greene, Jenny E.; Gallo, Elena +4 more

Distinct seed formation mechanisms are imprinted upon the fraction of dwarf galaxies currently containing a central supermassive black hole. Seeding by Population III remnants is expected to produce a higher occupation fraction than is generated with direct gas collapse precursors. Chandra observations of nearby early-type galaxies can directly de…

2015 The Astrophysical Journal
eHST 144
Particle acceleration by a solar flare termination shock
DOI: 10.1126/science.aac8467 Bibcode: 2015Sci...350.1238C

Krucker, Säm; Chen, Bin; Gary, Dale E. +3 more

Solar flares—the most powerful explosions in the solar system—are also efficient particle accelerators, capable of energizing a large number of charged particles to relativistic speeds. A termination shock is often invoked in the standard model of solar flares as a possible driver for particle acceleration, yet its existence and role have remained…

2015 Science
Hinode SOHO 144
Dust aerosol, clouds, and the atmospheric optical depth record over 5 Mars years of the Mars Exploration Rover mission
DOI: 10.1016/j.icarus.2014.03.029 Bibcode: 2015Icar..251...96L

Lemmon, Mark T.; Smith, Michael D.; Bell, James F., III +3 more

Dust aerosol plays a fundamental role in the behavior and evolution of the martian atmosphere. The first five Mars years of Mars Exploration Rover data provide an unprecedented record of the dust load at two sites. This record is useful for characterization of the atmosphere at the sites and as ground truth for orbital observations. Atmospheric ex…

2015 Icarus
eHST 143
AEGIS-X: Deep Chandra Imaging of the Central Groth Strip
DOI: 10.1088/0067-0049/220/1/10 Bibcode: 2015ApJS..220...10N

Barmby, P.; Ivison, R. J.; Cooper, M. C. +22 more

We present the results of deep Chandra imaging of the central region of the Extended Groth Strip, the AEGIS-X Deep (AEGIS-XD) survey. When combined with previous Chandra observations of a wider area of the strip, AEGIS-X Wide (AEGIS-XW), these provide data to a nominal exposure depth of 800 ks in the three central ACIS-I fields, a region of approx…

2015 The Astrophysical Journal Supplement Series
eHST 143
Hubble Space Telescope Proper Motion (HSTPROMO) Catalogs of Galactic Globular Cluster. II. Kinematic Profiles and Maps
DOI: 10.1088/0004-637X/803/1/29 Bibcode: 2015ApJ...803...29W

Anderson, Jay; van der Marel, Roeland P.; Watkins, Laura L. +1 more

We present kinematical analyses of 22 Galactic globular clusters using the Hubble Space Telescope proper motion catalogs recently presented in Bellini et al. For most clusters, this is the first proper-motion study ever performed, and, for many, this is the most detailed kinematic study of any kind. We use cleaned samples of bright stars to determ…

2015 The Astrophysical Journal
eHST 143
Are Compton-thick AGNs the Missing Link between Mergers and Black Hole Growth?
DOI: 10.1088/0004-637X/814/2/104 Bibcode: 2015ApJ...814..104K

Bell, Eric F.; Kartaltepe, Jeyhan S.; Kocevski, Dale D. +12 more

We examine the host morphologies of heavily obscured active galactic nuclei (AGNs) at z∼ 1 to test whether obscured super-massive black hole growth at this epoch is preferentially linked to galaxy mergers. Our sample consists of 154 obscured AGNs with {N}{{H}}\gt {10}23.5 {{cm}}-2 and z\lt 1.5. Using visual classif…

2015 The Astrophysical Journal
eHST 143
Density and Charge of Pristine Fluffy Particles from Comet 67P/Churyumov-Gerasimenko
DOI: 10.1088/2041-8205/802/1/L12 Bibcode: 2015ApJ...802L..12F

Lamy, P. L.; Szego, K.; Fulle, M. +38 more

The Grain Impact Analyzer and Dust Accumulator (GIADA) instrument on board ESA’s Rosetta mission is constraining the origin of the dust particles detected within the coma of comet 67 P/Churyumov-Gerasimenko (67P). The collected particles belong to two families: (i) compact particles (ranging in size from 0.03 to 1 mm), witnessing the presence of m…

2015 The Astrophysical Journal
Rosetta 143
Radio Loud AGNs are Mergers
DOI: 10.1088/0004-637X/806/2/147 Bibcode: 2015ApJ...806..147C

Lotz, Jennifer M.; Chiaberge, Marco; Norman, Colin +1 more

We measure the merger fraction of Type 2 radio-loud and radio-quiet active galactic nuclei (AGNs) at z\gt 1 using new samples. The objects have Hubble Space Telescope (HST) images taken with Wide Field Camera 3 (WFC3) in the IR channel. These samples are compared to the 3CR sample of radio galaxies at z\gt 1 and to a sample of non-active galaxies.…

2015 The Astrophysical Journal
eHST 143
Accretion-powered Pulsations in an Apparently Quiescent Neutron Star Binary
DOI: 10.1088/0004-637X/807/1/62 Bibcode: 2015ApJ...807...62A

Deller, Adam T.; Lyne, Andrew G.; Bogdanov, Slavko +10 more

Accreting millisecond X-ray pulsars (AMXPs) are an important subset of low-mass X-ray binaries (LMXBs) in which coherent X-ray pulsations can be observed during occasional, bright outbursts (X-ray luminosity {L}{{X}}∼ {10}36 {erg} {{{s}}}-1). These pulsations show that matter is being channeled onto the neutron sta…

2015 The Astrophysical Journal
XMM-Newton 142