Search Publications

Dark Energy Survey Year 1 results: the impact of galaxy neighbours on weak lensing cosmology with IM3SHAPE
DOI: 10.1093/mnras/stx3282 Bibcode: 2018MNRAS.475.4524S

Benoit-Lévy, A.; Bechtol, K.; Smith, M. +69 more

We use a suite of simulated images based on Year 1 of the Dark Energy Survey to explore the impact of galaxy neighbours on shape measurement and shear cosmology. The HOOPOE image simulations include realistic blending, galaxy positions, and spatial variations in depth and point spread function properties. Using the IM3SHAPE maximum-likelihood shap…

2018 Monthly Notices of the Royal Astronomical Society
eHST 49
Galaxies Probing Galaxies in PRIMUS. I. Sample, Spectroscopy, and Characteristics of the z\sim 0.5 Mg II-absorbing Circumgalactic Medium
DOI: 10.3847/1538-4357/aa9792 Bibcode: 2018ApJ...853...95R

Moustakas, John; Coil, Alison L.; Diamond-Stanic, Aleksandar M. +2 more

The spectroscopy of background QSO sightlines passing close to foreground galaxies is a potent technique for studying the circumgalactic medium (CGM). However, QSOs are effectively point sources, limiting their potential to constrain the size of circumgalactic gaseous structures. Here we present the first large Keck/Low-resolution Imaging Spectrom…

2018 The Astrophysical Journal
eHST 49
Formation of dipolarization fronts after current sheet thinning
DOI: 10.1063/1.5030200 Bibcode: 2018PhPl...25g2123X

Xu, Y.; Fu, H. S.; Liu, C. M. +2 more

Dipolarization front (DF)—a sharp boundary separating hot tenuous plasmas from cold dense plasmas—is a key structure responsible for particle acceleration and energy transport in the magnetotail. How such a structure is formed has been unclear so far. Two possible mechanisms suggested in previous studies are magnetic reconnection and spontaneous f…

2018 Physics of Plasmas
Cluster 49
Modelling high-resolution ALMA observations of strongly lensed highly star-forming galaxies detected by Herschel
DOI: 10.1093/mnras/sty513 Bibcode: 2018MNRAS.476.4383D

Cooray, A.; Farrah, D.; Marchetti, L. +12 more

We have modelled ∼0.1 arcsec resolution Atacama Large Millimetre/submillimeter Array imaging of six strong gravitationally lensed galaxies detected by the Herschel Space Observatory. Our modelling recovers mass properties of the lensing galaxies and, by determining magnification factors, intrinsic properties of the lensed submillimetre sources. We…

2018 Monthly Notices of the Royal Astronomical Society
Herschel 49
The Araucaria Project: High-precision Cepheid Astrophysics from the Analysis of Variables in Double-lined Eclipsing Binaries
DOI: 10.3847/1538-4357/aacb32 Bibcode: 2018ApJ...862...43P

Udalski, Andrzej; Soszyński, Igor; Thompson, Ian B. +15 more

Based on new observations and improved modeling techniques, we have reanalyzed seven Cepheids in the Large Magellanic Cloud. Improved physical parameters have been determined for the exotic system OGLE LMC-CEP-1718 composed of two first-overtone Cepheids and a completely new model was obtained for the OGLE LMC-CEP-1812 classical Cepheid. This is n…

2018 The Astrophysical Journal
eHST 49
A tale of two periods: determination of the orbital ephemeris of the super-Eddington pulsar NGC 7793 P13
DOI: 10.1051/0004-6361/201833292 Bibcode: 2018A&A...616A.186F

Harrison, F. A.; Fabian, A. C.; Pinto, C. +10 more

We present a timing analysis of multiple XMM-Newton and NuSTAR observations of the ultra-luminous pulsar NGC 7793 P13 spread over its 65 d variability period. We use the measured pulse periods to determine the orbital ephemeris, confirm a long orbital period with Porb = 63.9+0.5-0.6 d, and find an eccentricity of e…

2018 Astronomy and Astrophysics
XMM-Newton 49
Does Circumgalactic O VI Trace Low-pressure Gas Beyond the Accretion Shock? Clues from H I and Low-ion Absorption, Line Kinematics, and Dust Extinction
DOI: 10.3847/1538-4357/aac884 Bibcode: 2018ApJ...865...91S

Stern, Jonathan; Faucher-Giguère, Claude-André; Hennawi, Joseph F. +3 more

Large O VI columns are observed around star-forming low-redshift ∼ {L}* galaxies, with a dependence on impact parameter indicating that most {{{O}}}5+ particles reside beyond half the halo virial radius (≳ 100 {kpc}). In order to constrain the nature of the gas traced by {{O}} {{vi}}, we analyze additional observables of the…

2018 The Astrophysical Journal
eHST 49
Predicting Stellar-mass Black Hole Populations in Globular Clusters
DOI: 10.3847/1538-4357/aad63d Bibcode: 2018ApJ...864...13W

Rodriguez, Carl L.; Chatterjee, Sourav; Weatherford, Newlin C. +1 more

Recent discoveries of black hole (BH) candidates in Galactic and extragalactic globular clusters (GCs) have ignited interest in understanding how BHs dynamically evolve in a GC and the number of BHs ({N}BH}) that may still be retained by today’s GCs. Numerical models show that even if stellar-mass BHs are retained in today’s GCs, they a…

2018 The Astrophysical Journal
eHST 49
A 20-year record (1998-2017) of permafrost, active layer and meteorological conditions at a high Arctic permafrost research site (Bayelva, Spitsbergen)
DOI: 10.5194/essd-10-355-2018 Bibcode: 2018ESSD...10..355B

Hauber, Ernst; Boike, Julia; Juszak, Inge +10 more

Most permafrost is located in the Arctic, where frozen organic carbon makes it an important component of the global climate system. Despite the fact that the Arctic climate changes more rapidly than the rest of the globe, observational data density in the region is low. Permafrost thaw and carbon release to the atmosphere are a positive feedback m…

2018 Earth System Science Data
MEx 49
On the accuracy of mass measurement for microlensing black holes as seen by Gaia and OGLE
DOI: 10.1093/mnras/sty356 Bibcode: 2018MNRAS.476.2013R

Rybicki, Krzysztof A.; Wyrzykowski, Łukasz; Klencki, Jakub +3 more

We investigate the impact of combining Gaia astrometry from space with precise, high cadence OGLE photometry from the ground. For the archival event OGLE3-ULENS-PAR-02, which is likely a black hole, we simulate a realistic astrometric time series of Gaia measurements and combine it with the real photometric data collected by the OGLE project. We p…

2018 Monthly Notices of the Royal Astronomical Society
Gaia 49