Search Publications

Survey of caveats in low-energy particle measurements: Ulysses/HI-SCALE and ACE/EPAM Instruments
DOI: 10.1016/j.pss.2015.06.010 Bibcode: 2015P&SS..117..192M

Malandraki, O. E.; Anagnostopoulos, G. C.; Marhavilas, P. K.

"Heliosphere Instrument for Spectra, Composition, and Anisotropy at Low Energies" (HI-SCALE) onboard the ULYSSES spacecraft, and "Electron, Proton, and Alpha Monitor" (EPAM) onboard the ACE spacecraft, are very similar instruments and were designed to make measurements of ions and electrons over a broad range of energy and intensity. The ions (E

2015 Planetary and Space Science
Ulysses 13
Discovery of a nearby early-phase major cluster merger CIZA J1358.9-4750
DOI: 10.1093/pasj/psv029 Bibcode: 2015PASJ...67...71K

Makishima, Kazuo; Nakazawa, Kazuhiro; Gu, Liyi +4 more

CIZA J1358.9-4750 is a nearby (z = 0.074) pair of clusters of galaxies located close to the Galactic plane. It consists of two X-ray extended humps at the northwest and the southeast separated by 14' (∼ 1.2 Mpc), and an X-ray bright bridgelike structure in between. With Suzaku, the south east hump was shown to have a temperature of 5.6 ± 0.2 keV a…

2015 Publications of the Astronomical Society of Japan
Suzaku XMM-Newton 13
Line-depth-ratio temperatures for the close binary ν Octantis: new evidence supporting the conjectured circumstellar retrograde planet
DOI: 10.1093/mnras/stv533 Bibcode: 2015MNRAS.449.4428R

Ramm, D. J.

We explore the possibly that either star-spots or pulsations are the cause of a periodic radial velocity (RV) signal (P ∼ 400 d) from the K-giant binary ν Octantis (P ∼ 1050 d, e ∼ 0.25), alternatively conjectured to have a retrograde planet. Our study is based on temperatures derived from 22 line-depth ratios (LDRs) for ν Oct and 20 calibration s…

2015 Monthly Notices of the Royal Astronomical Society
Hipparcos 13
Corrugated velocity patterns in the spiral galaxies: NGC 278, NGC 1058, NGC 2500 & UGC 3574
DOI: 10.1093/mnras/stv2206 Bibcode: 2015MNRAS.454.3376S

Pérez, Enrique; Alfaro, Emilio J.; Sánchez-Gil, M. Carmen

We address the study of the H α vertical velocity field in a sample of four nearly face-on galaxies using long-slit spectroscopy taken with the Intermediate dispersion Spectrograph and Imaging System (ISIS), attached to the William Herschel Telescope (WHT) at the Roque de los Muchachos Observatory (Spain). The spatial structure of the velocity ver…

2015 Monthly Notices of the Royal Astronomical Society
eHST 13
Permittivity measurements of porous matter in support of investigations of the surface and interior of 67P/Churyumov-Gerasimenko
DOI: 10.1051/0004-6361/201526099 Bibcode: 2015A&A...583A..39B

Thomas, N.; Brouet, Y.; Encrenaz, P. +4 more


Aims: Permittivity measurements on porous samples of volcanic origin have been performed in the 0.05-190 GHz range under laboratory conditions in support of the Rosetta mission to comet 67P/Churyumov-Gerasimenko, specifically with the MIRO radiometric experiment and CONSERT radar experiment.
Methods: The samples were split into several s…

2015 Astronomy and Astrophysics
Rosetta 13
A Multiwavelength Study of Tadpole Galaxies in the Hubble Ultra Deep Field
DOI: 10.1088/0004-637X/814/2/97 Bibcode: 2015ApJ...814...97S

Ravindranath, Swara; de Mello, Duilia; Gardner, Jonathan P. +6 more

Multiwavelength data are essential in order to provide a complete picture of galaxy evolution and to inform studies of galaxies’ morphological properties across cosmic time. Here we present the results of a multiwavelength investigation of the morphologies of “tadpole” galaxies at intermediate redshift (0.314 < z < 3.175) in the Hubble Ultra…

2015 The Astrophysical Journal
eHST 13
Non-LTE modelling of prominence fine structures using hydrogen Lyman-line profiles
DOI: 10.1051/0004-6361/201425138 Bibcode: 2015A&A...577A..92S

Curdt, W.; Gunár, S.; Schwartz, P.


Aims: We perform a detailed statistical analysis of the spectral Lyman-line observations of the quiescent prominence observed on May 18, 2005.
Methods: We used a profile-to-profile comparison of the synthetic Lyman spectra obtained by 2D single-thread prominence fine-structure model as a starting point for a full statistical analysis of …

2015 Astronomy and Astrophysics
SOHO 13
Simulating Deep Hubble Images with Semi-empirical Models of Galaxy Formation
DOI: 10.1088/0004-637X/801/1/14 Bibcode: 2015ApJ...801...14T

White, Richard L.; Fall, S. Michael; Szalay, Alexander S. +1 more

We simulate deep images from the Hubble Space Telescope (HST) using semi-empirical models of galaxy formation with only a few basic assumptions and parameters. We project our simulations all the way to the observational domain, adding cosmological and instrumental effects to the images, and analyze them in the same way as real HST images ("forward…

2015 The Astrophysical Journal
eHST 13
A Multiwavelength Study of Three Hybrid Blazars
DOI: 10.1088/0004-637X/807/1/48 Bibcode: 2015ApJ...807...48S

Marshall, H. L.; Kharb, P.; Lister, M. L. +3 more

We present multiwavelength imaging observations of PKS 1045-188, 8C 1849+670, and PKS 2216-038, three radio-loud active galactic nuclei from the MOJAVE-Chandra Sample that straddle the Fanaroff-Riley (FR) boundary between low- and high-power jets. These hybrid sources provide an excellent opportunity to study jet emission mechanisms and the influe…

2015 The Astrophysical Journal
eHST 13
The naked nuclei of low ionization nuclear emission line regions
DOI: 10.1051/0004-6361/201526496 Bibcode: 2015A&A...581A..76B

Capetti, Alessandro; Balmaverde, Barbara

We analyze HST spectra and Chandra observations of a sample of 21 low ionization nuclear emission line regions (LINERs), at least 18 of which genuine active galactic nuclei. We find a correlation between the X-rays and emission lines luminosities, extending over three orders of magnitude and with a dispersion of 0.36 dex; no differences emerge bet…

2015 Astronomy and Astrophysics
eHST 13