Search Publications

X-Ray Spectral Properties of Seyfert I Galaxy LEDA 168563
DOI: 10.3847/1538-4357/aae309 Bibcode: 2018ApJ...868...11L

Fabian, Andrew C.; Tsuruta, Sachiko; Liebmann, Andrew C. +2 more

Interesting among possible mechanisms responsible for X-ray emission from active galactic nuclei (AGNs) is ionized relativistic reflection (IRR). Since it arises close to the central black hole it can test strong gravity. Its characteristic features include a high energy Compton hump, a broad Fe Kα line, and a soft excess. Therefore, using the Swi…

2018 The Astrophysical Journal
Suzaku XMM-Newton 6
The Catalogues Analysis of Stars Equatorial Coordinates and B-Magnitude of the FON Project
DOI: 10.18524/1810-4215.2018.31.144734 Bibcode: 2018OAP....31..199A

Andruk, V. M.; Akhmetov, V. S.; Protsyuk, Yu. I. +1 more

FON project was expected a catalogue of stellar positions and B magnitude of Northern sky from combination six astronomical observatories of the former USSR were equipped with the same wide-angle astrographs: Goloseevo (Ukraine), Zvenigorod, Zelenchuk (Russia), Abastumani (Georgia), Kitab (Uzbekistan) and HisorAO (Tajikistan). This paper has been …

2018 Odessa Astronomical Publications
Gaia Hipparcos 6
A Hubble Space Telescope imaging study of four FeLoBAL quasar host galaxies
DOI: 10.1093/mnras/stx3203 Bibcode: 2018MNRAS.475.3213L

Vestergaard, M.; Fan, X.; Lawther, D.

We study the host galaxies of four Iron Low-Ionization Broad Absorption-line Quasars (FeLoBALs), using Hubble Space Telescope imaging data, investigating the possibility that they represent a transition between an obscured active galactic nucleus (AGN) and an ordinary optical quasar. In this scenario, the FeLoBALs represent the early stage of merg…

2018 Monthly Notices of the Royal Astronomical Society
eHST 6
Herschel-PACS photometry of faint stars for sensitivity performance assessment and establishment of faint FIR primary photometric standards
DOI: 10.1051/0004-6361/201731812 Bibcode: 2018A&A...613A..40K

Balog, Z.; Müller, T. G.; Klaas, U. +3 more


Aims: Our aims are to determine flux densities and their photometric accuracy for a set of seventeen stars that range in flux from intermediately bright (≲2.5 Jy) to faint (≳5 mJy) in the far-infrared (FIR). We also aim to derive signal-to-noise dependence with flux and time, and compare the results with predictions from the Herschel exposure…

2018 Astronomy and Astrophysics
AKARI Herschel ISO 6
Study on the Curvature and Gradient of the Magnetic Field in Earth's Cusp Region Based on the Magnetic Curvature Analysis Method
DOI: 10.1029/2017JA025028 Bibcode: 2018JGRA..123.3794X

Rong, Zhaojin; Shen, Chao; Xiao, Chao +2 more

This paper uses the multiple-point magnetic measurements from the Cluster mission to investigate the curvature and gradient of the magnetic field as well as their relations with the current density inside the cusp region under different interplanetary magnetic field (IMF) conditions. From two event studies, it is shown that the curvature radius of…

2018 Journal of Geophysical Research (Space Physics)
Cluster 6
A Statistical Study of Ionospheric Boundary Wave Formation at Venus
DOI: 10.1029/2018JA025644 Bibcode: 2018JGRA..123.7668C

Zhang, Tielong; Futaana, Yoshifumi; Frahm, Rudy A. +3 more

Previous missions to Venus have revealed that encounters with plasma irregularities of atmospheric origin outside the atmosphere are not uncommon. A number of mechanisms have been proposed to discuss their origins as well as their roles in the atmospheric evolution of Venus. One such mechanism involves an ionopause with a wavelike appearance. By u…

2018 Journal of Geophysical Research (Space Physics)
VenusExpress 6
Studies of Modern Star Catalogs Based on Photoelectric Observations of Lunar Occultations of Stars
DOI: 10.1134/S1063772918120016 Bibcode: 2018ARep...62.1042C

Churkin, K. O.; Andreev, A. O.; Nefedyev, Yu. A. +2 more

An important area of investigation in astronomy is the relationship between fundamental and dynamical coordinate systems. Valuable material for such studies is provided by photoelectric occultation observations of stars by the Moon, which can provide high precision of detecting rapidly occurring processes and have been carried out over a long time…

2018 Astronomy Reports
Hipparcos 6
Dating the Tidal Disruption of Globular Clusters with GAIA Data on Their Stellar Streams
DOI: 10.3847/2041-8213/aac48c Bibcode: 2018ApJ...859L..13B

Loeb, Abraham; Bose, Sownak; Ginsburg, Idan

The Gaia mission promises to deliver precision astrometry at an unprecedented level, heralding a new era for discerning the kinematic and spatial coordinates of stars in our Galaxy. Here, we present a new technique for estimating the age of tidally disrupted globular cluster streams using the proper motions and parallaxes of tracer stars. We evolv…

2018 The Astrophysical Journal
Gaia 6
Faint γ-ray sources at low redshift: the radio galaxy IC 1531
DOI: 10.1093/mnras/sty2622 Bibcode: 2018MNRAS.481.5236B

Vignali, C.; Grandi, P.; Siemiginowska, A. +6 more

We present a multiwavelength study of IC 1531 (z = 0.02564), an extragalactic radio source associated with the γ-ray object 3FGL J0009.9 - 3206 and classified as a blazar of uncertain type in the Third Fermi-Large Area Telescope AGN catalog (3LAC). A core-jet structure, visible in radio and X-rays, is enclosed within a ∼220 kpc wide radio structur…

2018 Monthly Notices of the Royal Astronomical Society
XMM-Newton 6
Measurement of coronal properties of Seyfert galaxies from NuSTAR's hard X-ray spectrum
DOI: 10.1007/s12036-017-9502-5 Bibcode: 2018JApA...39...15R

Stalin, C. S.; Rani, Priyanka

Precise measurement of the coronal properties of Active Galactic Nuclei (AGN) requires the availability of high signal-to-noise ratio data covering a wide range of X-ray energies. The Nuclear Spectroscopic Telescope Array (NuSTAR) which is highly sensitive to earlier missions in its operational energy range of 3–79 keV, allows us to arrive at prec…

2018 Journal of Astrophysics and Astronomy
INTEGRAL 6