Search Publications

Disk emission and atmospheric absorption lines in black hole candidate 4U 1630-472
DOI: 10.1051/0004-6361/201321567 Bibcode: 2014A&A...562A..81R

Różańska, A.; Madej, J.; Bagińska, P. +2 more

Context. We analyzed Suzaku data of the black hole candidate 4U 1630-472 when it was in the high/soft state. The source, known for X-ray outbursts and for absorption dips, has an X-ray continuum spectrum that is interpreted correctly as emission from an accretion disk. Additionally, two absorption lines from He and H-like iron have been clearly de…

2014 Astronomy and Astrophysics
Suzaku 7
Early-type Galaxies at Intermediate Redshift Observed with Hubble Space Telescope WFC3: Perspectives on Recent Star Formation
DOI: 10.1088/0004-637X/796/2/101 Bibcode: 2014ApJ...796..101R

Hathi, Nimish P.; Rutkowski, Michael J.; Windhorst, Rogier A. +7 more

We present an analysis of the stellar populations of 102 visually selected early-type galaxies (ETGs) with spectroscopic redshifts (0.35 lsim z lsim 1.5) from observations in the Early Release Science program with the Wide Field Camera 3 (WFC3) on the Hubble Space Telescope (HST). We fit one- and two-component synthetic stellar models to the ETGs …

2014 The Astrophysical Journal
eHST 7
BICEP2 constrains composite inflation
DOI: 10.1142/S0218271814500709 Bibcode: 2014IJMPD..2350070C

Channuie, Phongpichit

In light of BICEP2, we re-examine single field inflationary models in which the inflation is a composite state stemming from various four-dimensional strongly coupled theories. We study in the Einstein frame a set of cosmological parameters, the primordial spectral index ns and tensor-to-scalar ratio r, predicted by such models. We conf…

2014 International Journal of Modern Physics D
Planck 7
Full Particle Electromagnetic Simulations of Entropy Generation across a Collisionless Shock
DOI: 10.1088/2041-8205/793/1/L11 Bibcode: 2014ApJ...793L..11Y

Wang, Rui; Yang, Zhongwei; Liu, Ying D. +5 more

Experimental data from Cluster have shown that entropy density can be generated across Earth's bow shock. These new observations are a starting point for a more sophisticated analysis that includes computer modeling of a collisionless shock using observed shock parameters as input. In this Letter, we present the first comparison between observatio…

2014 The Astrophysical Journal
Cluster 7
Phase-resolved X-ray spectroscopy and spectral energy distribution of the X-ray soft polar RS Caeli
DOI: 10.1051/0004-6361/201321383 Bibcode: 2014A&A...562A..42T

Burwitz, V.; Walter, F. M.; Schwope, A. D. +3 more

Context. RS Cae is the third target in our series of XMM-Newton observations of soft X-ray-dominated polars.
Aims: Our observational campaign aims to better understand and describe the multiwavelength data, the physical properties of the system components, and the short- and long-term behavior of the component fluxes in RS Cae.
Methods: …

2014 Astronomy and Astrophysics
XMM-Newton 7
Cluster observations of hot He+ events in the inner magnetosphere
DOI: 10.1002/2013JA019724 Bibcode: 2014JGRA..119.2706Y

Yamauchi, M.; Dandouras, I.; Nilsson, H. +1 more

In the inner magnetosphere inside 65° invariant latitude, Cluster Ion Spectrometry detected hot He+ events of about a few tens to several hundred eV without the same types of hot H+ signature at the same energy. During the 2001-2006 period when the Cluster orbit was almost constant and approximately north-south symmetric at c…

2014 Journal of Geophysical Research (Space Physics)
Cluster 7
The young binary HD 102077: Orbit, spectral type, kinematics, and moving group membership
DOI: 10.1051/0004-6361/201323262 Bibcode: 2014A&A...564A..10W

Henning, Thomas; Reffert, Sabine; Schlieder, Joshua E. +4 more

The K-type binary star HD 102077 was proposed as a candidate member of the TW Hydrae association (TWA) which is a young (5-15 Myr) moving group in close proximity (~50 pc) to the solar system. The aim of this work is to verify this hypothesis by different means. We first combine diffraction-limited observations from the ESO NTT 3.5 m telescope in …

2014 Astronomy and Astrophysics
Hipparcos eHST 7
Constraints on Jupiter's stratospheric HCl abundance and chlorine cycle from Herschel/HIFI
DOI: 10.1016/j.pss.2014.07.015 Bibcode: 2014P&SS..103..250T

Fletcher, L. N.; Irwin, P. G. J.; Teanby, N. A. +1 more

Detection of HCl on Jupiter would provide insight into the chlorine cycle and external elemental fluxes on giant planets, yet so far has not been possible. Here we present the most sensitive search for Jupiter's stratospheric HCl to date using observations of the 625.907 and 1876.221 GHz spectral lines with Herschel's HIFI instrument. HCl was not …

2014 Planetary and Space Science
Herschel 7
Herschel SPIRE fourier transform spectrometer: calibration of its bright-source mode
DOI: 10.1007/s10686-013-9359-9 Bibcode: 2014ExA....37..239L

Valtchanov, Ivan; Hopwood, Rosalind; Naylor, David A. +10 more

The Fourier Transform Spectrometer (FTS) of the Spectral and Photometric Imaging REceiver (SPIRE) on board the ESA Herschel Space Observatory has two detector setting modes: (a) a nominal mode, which is optimized for observing moderately bright to faint astronomical targets, and (b) a bright-source mode recommended for sources significantly bright…

2014 Experimental Astronomy
Herschel 7
Signals of solar cosmic ray flux variations inferred from the noise in raw CCD solar images taken by SOHO/EIT
DOI: 10.1002/2013JA019142 Bibcode: 2014JGRA..119...88O

Chae, Jongchul; Oh, Suyeon; Yi, Yu +1 more

The noise embedded in the raw data in one scientific discipline has sometimes been proven to be a valuable signal for another discipline, and there are examples throughout science history. The solar images taken by the solid state detectors (CCDs) of the Sun monitoring satellites are usually cleaned by removing the traces of cosmic rays on the raw…

2014 Journal of Geophysical Research (Space Physics)
SOHO 7