Search Publications

GALEX far-ultraviolet observations of metal-poor subdwarfs
DOI: 10.1007/s10509-018-3455-2 Bibcode: 2018Ap&SS.363..235S

Smith, Graeme H.

Far-ultraviolet photometry derived from the GALEX satellite observatory has been compiled for a sample of metal-poor subdwarfs with [Fe/

2018 Astrophysics and Space Science
Gaia 2
The detection of ultra-relativistic electrons in low Earth orbit
DOI: 10.1051/swsc/2017041 Bibcode: 2018JSWSC...8A...1K

Dammasch, Ingolf E.; Berghmans, David; Dominique, Marie +6 more


Aims: To better understand the radiation environment in low Earth orbit (LEO), the analysis of in-situ observations of a variety of particles, at different atmospheric heights, and in a wide range of energies, is needed.
Methods: We present an analysis of energetic particles, indirectly detected by the large yield radiometer (LYRA) instr…

2018 Journal of Space Weather and Space Climate
PROBA-2 2
Titan's Variable Ionosphere During the T118 and T119 Cassini Flybys
DOI: 10.1029/2018GL078436 Bibcode: 2018GeoRL..45.8721E

Wahlund, J. -E.; Edberg, N. J. T.; Andrews, D. J. +6 more

We report on unusual dynamics in Titan's ionosphere as a significant difference in ionospheric electron density is observed between the T118 and T119 Cassini nightside flybys. Two distinct nightside electron density peaks were present during T118, at 1,150 and 1,200 km, and the lowest density ever observed in Titan's ionosphere at altitudes 1,000-…

2018 Geophysical Research Letters
Cassini 2
Synthetic photometry of globular clusters: Uncertainties on synthetic colors
DOI: 10.1051/0004-6361/201833083 Bibcode: 2018A&A...616A.164M

Martins, F.

Context. Synthetic photometry is a great tool for studying globular clusters, especially for understanding the nature of their multiple populations.
Aims: Our goal is to quantify the errors on synthetic photometry that are caused by uncertainties on stellar and observational/calibration parameters. These errors can be taken into account when …

2018 Astronomy and Astrophysics
eHST 2
Observing Galaxy Mergers at the Epoch of Reionization
DOI: 10.3847/1538-4357/aaa196 Bibcode: 2018ApJ...853...81C

Kaurov, Alexander A.; Chaikin, Evgenii A.; Tyulneva, Nadezda V.

The galaxies with photometric redshifts observed in a close angular proximity might be either projection coincidences, strongly lensed images of the same galaxy, or separate galaxies that are in a stage of merging. We search for the groups of galaxies in the Hubble Ultra Deep Field (HUDF09) in z ∼ 7 and z ∼ 8 drop-out samples. We find no close pai…

2018 The Astrophysical Journal
eHST 2
A Spatially Resolved Study of the GRB 020903 Host Galaxy
DOI: 10.3847/1538-4357/aab093 Bibcode: 2018ApJ...856...36T

Levesque, Emily M.; Thorp, Mallory D.

GRB 020903 is a long-duration gamma-ray burst with a host galaxy close enough and extended enough for spatially resolved observations, making it one of less than a dozen GRBs where such host studies are possible. GRB 020903 lies in a galaxy host complex that appears to consist of four interacting components. Here we present the results of spatiall…

2018 The Astrophysical Journal
eHST 2
The broad-band SEDs of four `hypervariable' AGN
DOI: 10.1093/mnras/stx2992 Bibcode: 2018MNRAS.474.3565C

Done, Chris; Elvis, Martin; Marshall, Philip J. +6 more

We present an optical-to-X-ray spectral analysis of four `hypervariable' AGN (HVAs) discovered by comparing Pan-STARRS data to that from the Sloan Digital Sky Survey over a 10 yr baseline (Lawrence et al.). There is some evidence that these objects are X-ray loud for their corresponding UV luminosities, but given that we measured them in a histori…

2018 Monthly Notices of the Royal Astronomical Society
XMM-Newton 2
Improved model of the triple system V746 Cassiopeiae that has a bipolar magnetic field associated with the tertiary
DOI: 10.1051/0004-6361/201628363 Bibcode: 2018A&A...609A...5H

Harmanec, P.; Zasche, P.; Korčáková, D. +9 more

V746 Cas is known to be a triple system composed of a close binary with an alternatively reported period of either 25.^d4 or 27.^d8 and a distant third component in a 170 yr (62 000 d) orbit. The object was also reported to exhibit multiperiodic light variations with periods from 0.^d83 to 2.^d50, on the basis of which it was classified as a slowl…

2018 Astronomy and Astrophysics
Hipparcos 2
Velocity-resolved [O I] 63 µm Emission in the HD 50138 Circumstellar Disk
DOI: 10.3847/1538-4357/aad639 Bibcode: 2018ApJ...864..104S

de Wit, W. -J.; Güsten, R.; Wiesemeyer, H. +5 more

HD 50138 is one of the brightest B[e] stars and is located at a distance of ∼380 pc with strong infrared excess. The star was observed in [O I] 63 µm and [C II] 158 µm with high velocity resolution with upGREAT on SOFIA. The velocity-resolved [O I] emission provides evidence for a large gas disk, ∼760 au in size, around HD 50138. Where…

2018 The Astrophysical Journal
Gaia Herschel 2
Spatial distribution of ion polytropic index joint-modulated by temperature anisotropy and MHD disturbances in the southern high latitude magnetosheath
DOI: 10.1007/s11431-017-9095-x Bibcode: 2018ScChE..61..381P

Cao, J. B.; Pang, X. X.; Deng, Z. +1 more

2018 Science in China E: Technological Sciences
Cluster 2