Search Publications

Predicted properties of multiple images of the strongly lensed supernova SN Refsdal.
DOI: 10.1093/mnrasl/slv025 Bibcode: 2015MNRAS.449L..86O

Oguri, M.

We construct a mass model of the cluster MACS J1149.6+2223 to study the expected properties of multiple images of SN Refsdal, the first example of a gravitationally lensed supernova with resolved multiple images recently reported by Kelly et al. We find that the best-fitting model predicts six supernova images in total, i.e. two extra images in ad…

2015 Monthly Notices of the Royal Astronomical Society
eHST 40
A spectroscopic investigation of the O-type star population in four Cygnus OB associations. II. Determination of the fundamental parameters
DOI: 10.1051/0004-6361/201321985 Bibcode: 2015A&A...577A..23M

Rauw, G.; De Becker, M.; Mahy, L. +2 more


Aims: Having established the binary status of nineteen O-type stars located in four Cygnus OB associations, we now determine their fundamental parameters to constrain their properties and their evolutionary status. We also investigate their surface nitrogen abundances, which we compare with other results from the literature obtained for galac…

2015 Astronomy and Astrophysics
IUE 40
The Multi-layer Variable Absorbers in NGC 1365 Revealed by XMM-Newton and NuSTAR
DOI: 10.1088/0004-637X/804/2/107 Bibcode: 2015ApJ...804..107R

Harrison, F.; Stern, D.; Zhang, W. W. +15 more

Between 2012 July and 2013 February, NuSTAR and XMM-Newton performed four long-look joint observations of the type 1.8 Seyfert, NGC 1365. We have analyzed the variable absorption seen in these observations in order to characterize the geometry of the absorbing material. Two of the observations caught NGC 1365 in an unusually low absorption state, …

2015 The Astrophysical Journal
XMM-Newton 40
Active-region Tilt Angles: Magnetic versus White-light Determinations of Joy's Law
DOI: 10.1088/0004-637X/798/1/50 Bibcode: 2015ApJ...798...50W

Li, J.; Wang, Y. -M.; Baranyi, T. +1 more

The axes of solar active regions are inclined relative to the east-west direction, with the tilt angle tending to increase with latitude ("Joy's law"). Observational determinations of Joy's law have been based either on white-light images of sunspot groups or on magnetograms, where the latter have the advantage of measuring directly the physically…

2015 The Astrophysical Journal
SOHO 40
Relations Between Microwave Bursts and Near-Earth High-Energy Proton Enhancements and Their Origin
DOI: 10.1007/s11207-015-0797-6 Bibcode: 2015SoPh..290.2827G

Grechnev, V. V.; Chertok, I. M.; Kiselev, V. I. +1 more

We further study the relations between parameters of bursts at 35 GHz recorded with the Nobeyama Radio Polarimeters during 25 years and solar proton events (Grechnev et al. in Publ. Astron. Soc. Japan65, S4, 2013a). Here we address the relations between the microwave fluences at 35 GHz and near-Earth proton fluences above 100 MeV to find informati…

2015 Solar Physics
SOHO 40
Gaia's potential for the discovery of circumbinary planets
DOI: 10.1093/mnras/stu2428 Bibcode: 2015MNRAS.447..287S

Sahlmann, J.; Martin, D. V.; Triaud, A. H. M. J.

The abundance and properties of planets orbiting binary stars - circumbinary planets - are largely unknown because they are difficult to detect with currently available techniques. Results from the Kepler satellite and other studies indicate a minimum occurrence rate of circumbinary giant planets of ∼10 per cent, yet only a handful are presently k…

2015 Monthly Notices of the Royal Astronomical Society
Gaia 40
Constraints on the Nambu-Goto cosmic string contribution to the CMB power spectrum in light of new temperature and polarisation data
DOI: 10.1088/1475-7516/2015/02/024 Bibcode: 2015JCAP...02..024L

Lazanu, Andrei; Shellard, Paul

Cosmic strings generate vector and tensor modes in the B-channel of polarisation, as well as the usual temperature power spectrum and E-mode polarisation spectrum. We use the power spectrum obtained from high-resolution Nambu-Goto cosmic string simulations together with the Planck and BICEP2 likelihoods to explore the degeneracies appearing betwee…

2015 Journal of Cosmology and Astroparticle Physics
Planck 40
Dependence of the dayside magnetopause reconnection rate on local conditions
DOI: 10.1002/2015JA021524 Bibcode: 2015JGRA..120.6386W

Kistler, Lynn M.; Wang, Shan; Mouikis, Christopher G. +1 more

We estimate the reconnection rates for eight dayside magnetopause reconnection events observed by the Cluster spacecraft and compare them with the predictions of the Cassak-Shay Formula (Rcs) Cassak and Shay (2007). The measured reconnection rate is determined by calculating the product of the inflow velocity and magnetic field in the m…

2015 Journal of Geophysical Research (Space Physics)
Cluster 40
The WEBT campaign on the BL Lac object PG 1553+113 in 2013. An analysis of the enigmatic synchrotron emission
DOI: 10.1093/mnras/stv1884 Bibcode: 2015MNRAS.454..353R

Lähteenmäki, A.; Umana, G.; Giroletti, M. +59 more

A multifrequency campaign on the BL Lac object PG 1553+113 was organized by the Whole Earth Blazar Telescope (WEBT) in 2013 April-August, involving 19 optical, two near-IR, and three radio telescopes. The aim was to study the source behaviour at low energies during and around the high-energy observations by the Major Atmospheric Gamma-ray Imaging …

2015 Monthly Notices of the Royal Astronomical Society
XMM-Newton eHST 40
Predicting CME Ejecta and Sheath Front Arrival at L1 with a Data-constrained Physical Model
DOI: 10.1088/0004-637X/812/2/144 Bibcode: 2015ApJ...812..144H

Hess, Phillip; Zhang, Jie

We present a method for predicting the arrival of a coronal mass ejection (CME) flux rope in situ, as well as the sheath of solar wind plasma accumulated ahead of the driver. For faster CMEs, the front of this sheath will be a shock. The method is based upon geometrical separate measurement of the CME ejecta and sheath. These measurements are used…

2015 The Astrophysical Journal
SOHO 40