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Bulgeless Galaxies at Intermediate Redshift: Sample Selection, Color Properties, and the Existence of Powerful Active Galactic Nuclei
DOI: 10.1088/0004-637X/782/1/22 Bibcode: 2014ApJ...782...22B

Bell, Eric F.; Brinchmann, Jarle; Bizzocchi, Luca +11 more

We present a catalog of bulgeless galaxies, which includes 19,225 objects selected in four of the deepest, largest multi-wavelength data sets available—COSMOS, AEGIS, GEMS, and GOODS—at intermediate redshift (0.4 <= z <= 1.0). The morphological classification was provided by the Advanced Camera for Surveys General Catalog (ACS-GC), which use…

2014 The Astrophysical Journal
eHST 14
First far-ultraviolet disk-integrated phase curve analysis of Mimas, Tethys and Dione from the Cassini-UVIS data sets
DOI: 10.1016/j.icarus.2014.07.026 Bibcode: 2014Icar..242..158R

Hendrix, Amanda R.; Royer, Emilie M.

We perform an analysis of the photometric properties of the icy saturnian satellites at 180 nm, based on the first far-UV disk-integrated phase curves of Mimas, Tethys and Dione. Their interactions with the environment (the E-ring and the magnetosphere) are investigated, leading to a better understanding of the effects of exogenic processes on the…

2014 Icarus
Cassini 14
The XMM-Newton view of the radio-loud narrow-line Seyfert 1 galaxy PMN J0948+0022
DOI: 10.1093/mnras/stu239 Bibcode: 2014MNRAS.440..106B

Bhatt, Himali; Bhattacharyya, Subir; Bhatt, Nilay +1 more

We analysed the archival XMM-Newton data of the radio-loud narrow-line Seyfert 1 galaxy PMN J0948+0022 in the energy range 0.3-10.0 keV. The X-ray data reveal that the spectrum in the 0.3-10.0 keV energy band is not a simple power law as previously described in the literature. Instead it consists of a power law with soft excess below 2.5 keV. The …

2014 Monthly Notices of the Royal Astronomical Society
XMM-Newton 14
On the Dust Environment of Comet C/2012 S1 (ISON) from 12 AU Pre-perihelion to the End of its Activity around Perihelion
DOI: 10.1088/0004-637X/791/2/118 Bibcode: 2014ApJ...791..118M

López-Moreno, J. J.; Moreno, F.; García, F. +48 more

A Monte Carlo dust tail model has been applied to extract the dust environment parameters of the comet C/2012 S1 (ISON) from both Earth-based and SOHO LASCO C3 observations, performed from about six astronomical units (AU) inbound, to just after perihelion passage, when only a small portion of the original comet nucleus has survived in the form of…

2014 The Astrophysical Journal
SOHO 14
UV surface brightness of galaxies from the local universe to z ~ 5
DOI: 10.1142/S0218271814500588 Bibcode: 2014IJMPD..2350058L

Scarpa, Riccardo; Falomo, Renato; Lerner, Eric J.

The Tolman test for surface brightness (SB) dimming was originally proposed as a test for the expansion of the universe. The test, which is independent of the details of the assumed cosmology, is based on comparisons of the SB of identical objects at different cosmological distances. Claims have been made that the Tolman test provides compelling e…

2014 International Journal of Modern Physics D
eHST 14
Pre-perihelion activity of comet 67P/Churyumov-Gerasimenko
DOI: 10.1051/0004-6361/201424186 Bibcode: 2014A&A...567L...2G

Schulz, R.; Tozzi, G. P.; Rożek, A. +3 more

Context. Comets are believed to hold a relatively pristine record of the physical and chemical processes that occurred during the formation and evolution of the solar system. Thorough investigations of these small bodies, such as the one that will be performed by the ESA/Rosetta cornerstone mission, are thus supposed to bring strong and unique con…

2014 Astronomy and Astrophysics
Rosetta 14
Fluctuation Spectroscopy: A New Probe of Old Stellar Populations
DOI: 10.1088/0004-637X/797/1/56 Bibcode: 2014ApJ...797...56V

van Dokkum, Pieter G.; Conroy, Charlie

We introduce a new method to determine the relative contributions of different types of stars to the integrated light of nearby early-type galaxies. As is well known, the surface brightness of these galaxies shows pixel-to-pixel fluctuations due to Poisson variations in the number of giant stars. Differential spectroscopy of pixels as a function o…

2014 The Astrophysical Journal
eHST 14
Nighttime sensitivity of ionospheric VLF measurements to X-ray bursts from a remote cosmic source
DOI: 10.1002/2013JA019670 Bibcode: 2014JGRA..119.4758R

Giménez de Castro, C. Guillermo; Raulin, Jean-Pierre; Correia, Emilia +2 more

On 22 January 2009, a series of X-ray bursts were emitted by the soft gamma ray repeater SGR J1550-5418. Some of these bursts produced enhanced ionization in the nighttime lower ionosphere. These ionospheric disturbances were studied using X-ray measurements from the Anti-Coincidence Shield of the Spectrometer for Integral onboard the Internationa…

2014 Journal of Geophysical Research (Space Physics)
INTEGRAL 14
Discovery of an Ultra-faint Dwarf Galaxy in the Intracluster Field of the Virgo Center: A Fossil of the First Galaxies?
DOI: 10.1088/2041-8205/795/1/L6 Bibcode: 2014ApJ...795L...6J

Lee, Myung Gyoon; Jang, In Sung

Ultra-faint dwarf galaxies (UFDs) are newcomers among galaxies, and are the faintest galaxies in the observed universe. To date, they have only been found around the Milky Way Galaxy and M31 in the Local Group. We present the discovery of a UFD in the intracluster field in the core of the Virgo cluster (Virgo UFD1), which is far from any massive g…

2014 The Astrophysical Journal
eHST 14
Dayglow and auroral emissions of Uranus in H2 FUV bands
DOI: 10.1016/j.icarus.2014.05.035 Bibcode: 2014Icar..239..160B

Lamy, L.; Roueff, E.; Cessateur, G. +7 more

Following the recent detection of an auroral signal on Uranus (Lamy et al. [2012]. Geophys. Res. Lett. 39, 7105) during HST/STIS observation performed in November 2011, we analyzed the associated HST/STIS FUV spectral images obtained in 2011 and 2012. Our purpose was to extract any possible H2 emission produced in the upper atmosphere o…

2014 Icarus
eHST 14