Search Publications

Wavelet reconstruction of E and B modes for CMB polarization and cosmic shear analyses
DOI: 10.1093/mnras/stw3176 Bibcode: 2017MNRAS.466.3728L

Leistedt, Boris; Peiris, Hiranya V.; McEwen, Jason D. +1 more

We present new methods for mapping the curl-free (E-mode) and divergence-free (B-mode) components of spin 2 signals using spin directional wavelets. Our methods are equally applicable to measurements of the polarization of the cosmic microwave background (CMB) and the shear of galaxy shapes due to weak gravitational lensing. We derive pseudo- and …

2017 Monthly Notices of the Royal Astronomical Society
Planck 16
High signal-to-noise spectral characterization of the planetary-mass object HD 106906 b
DOI: 10.1051/0004-6361/201731527 Bibcode: 2017A&A...608A..71D

Fortney, Jonathan J.; Meyer, Michael R.; Quanz, Sascha P. +4 more

Context. Directly imaged planets are ideal candidates for spectroscopic characterization of their atmospheres. The angular separations that are typically close to their host stars, however, reduce the achievable contrast and thus signal-to-noise ratios (S/N).
Aims: We spectroscopically characterize the atmosphere of HD 106906 b, which is a yo…

2017 Astronomy and Astrophysics
Gaia 16
Gas inflows towards the nucleus of the Seyfert 2 galaxy NGC 1667
DOI: 10.1093/mnras/stx018 Bibcode: 2017MNRAS.466.4370S

Schnorr-Müller, Allan; Storchi-Bergmann, Thaisa; Nagar, Neil M. +1 more

We use optical spectra from the inner 2 × 3 kpc2 of the Seyfert 2 galaxy NGC 1667, obtained with the Gemini Multi-Object Spectrograph integral field spectrograph on the Gemini South telescope at a spatial resolution of ≈240 pc, to assess the feeding and feedback processes in this nearby active galactic nucleus (AGN). We have identified …

2017 Monthly Notices of the Royal Astronomical Society
eHST 16
X-ray orbital modulation of a white dwarf accreting from an L dwarf. The system SDSS J121209.31+013627.7
DOI: 10.1051/0004-6361/201630038 Bibcode: 2017A&A...598L...6S

de Martino, D.; Stelzer, B.; Wynn, G. A. +2 more

In an XMM-Newton observation of the binary SDSS J121209.31+013627.7, consisting of a white dwarf and an L dwarf, we detect X-ray orbital modulation as proof of accretion from the substellar companion onto the magnetic white dwarf. We constrain the system geometry (inclination as well as magnetic and pole-cap angle) through modelling of the X-ray l…

2017 Astronomy and Astrophysics
XMM-Newton 16
"TNOs are Cool": A survey of the trans-Neptunian region. XIII. Statistical analysis of multiple trans-Neptunian objects observed with Herschel Space Observatory
DOI: 10.1051/0004-6361/201730588 Bibcode: 2017A&A...608A..19K

Lellouch, E.; Stansberry, J.; Doressoundiram, A. +3 more

Context. Gravitationally bound multiple systems provide an opportunity to estimate the mean bulk density of the objects, whereas this characteristic is not available for single objects. Being a primitive population of the outer solar system, binary and multiple trans-Neptunian objects (TNOs) provide unique information about bulk density and intern…

2017 Astronomy and Astrophysics
Herschel 16
The stellar mass-size relation for cluster galaxies at z = 1 with high angular resolution from the Gemini/GeMS multiconjugate adaptive optics system
DOI: 10.1093/mnras/stw2411 Bibcode: 2017MNRAS.464.2910S

Glazebrook, Karl; Abraham, Roberto; Bayliss, Matthew +7 more

We present the stellar mass-size relation for 49 galaxies within the z = 1.067 cluster SPT-CL J0546-5345, with full width at half-maximum ∼80-120 mas Ks-band data from the Gemini multiconjugate adaptive optics system (GeMS/GSAOI). This is the first such measurement in a cluster environment, performed at sub-kpc resolution at rest-frame …

2017 Monthly Notices of the Royal Astronomical Society
eHST 16
Simultaneous optical/X-ray study of GS 1354-64 (=BW Cir) during hard outburst: evidence for optical cyclo-synchrotron emission from the hot accretion flow
DOI: 10.1093/mnras/stx840 Bibcode: 2017MNRAS.469..193P

Gandhi, Poshak; Altamirano, Diego; Misra, Ranjeev +3 more

We present results from simultaneous optical [South African Large Telescope (SALT)] and X-ray (Swift and INTEGRAL) observations of GS 1354-64/BW Cir during the 2015 hard state outburst. During the rising phase, optical/X-ray time series shows a strong anti-correlation with X-ray photons lagging optical. Optical and X-ray power spectra show quasi-p…

2017 Monthly Notices of the Royal Astronomical Society
INTEGRAL 16
Soft extragalactic X-ray binaries at the Eddington Threshold
DOI: 10.1093/mnras/stx308 Bibcode: 2017MNRAS.467.2690E

Roberts, Timothy P.; Earnshaw, Hannah M.

The luminosity range at and just below the 1039 erg s-1 cut-off for defining ultraluminous X-ray sources (ULXs) is a little-explored regime. It none the less hosts a large number of X-ray sources, and has great potential for improving our understanding of sources with ∼Eddington accretion rates. We select a sample of four sou…

2017 Monthly Notices of the Royal Astronomical Society
XMM-Newton eHST 16
Listing of 502 Times When the Ulysses Magnetic Fields Instrument Observed Waves Due to Newborn Interstellar Pickup Protons
DOI: 10.3847/1538-4357/aa6c2f Bibcode: 2017ApJ...840...13C

Isenberg, Philip A.; Murphy, Neil; Cannon, Bradford E. +4 more

In two earlier publications we analyzed 502 intervals of magnetic waves excited by newborn interstellar pickup protons that were observed by the Ulysses spacecraft. Due to the considerable effort required in identifying these events, we provide a list of the times for the 502 wave event intervals previously identified. In the process, we provide a…

2017 The Astrophysical Journal
Ulysses 16
The final year of the Rosetta mission
DOI: 10.1016/j.actaastro.2017.03.027 Bibcode: 2017AcAau.136..354A

Ferri, Paolo; Accomazzo, Andrea; Hubault, Armelle +6 more

The International Rosetta Mission was launched on 2nd March 2004 on its 10 year journey to rendezvous with comet 67P Churyumov-Gerasimenko. Rosetta performed comet orbit insertion on the 6th of August 2014, after which it characterised the nucleus and orbited it at altitudes as low as a few kilometres. In November 2014 Rosetta delivered the lander…

2017 Acta Astronautica
Rosetta 16