Search Publications

High-precision optical polarimetry of the accreting black hole V404 Cyg during the 2015 June outburst
DOI: 10.1093/mnras/stx779 Bibcode: 2017MNRAS.468.4362K

Miles-Páez, Paulo A.; Piirola, Vilppu; Tsygankov, Sergey S. +4 more

Our simultaneous three-colour (BVR) polarimetric observations of the low-mass black hole X-ray binary V404 Cyg show a small but statistically significant change of polarization degree (Δp ∼ 1 per cent) between the outburst in 2015 June and the quiescence. The polarization of V404 Cyg in the quiescent state agrees within the errors with that of the…

2017 Monthly Notices of the Royal Astronomical Society
INTEGRAL 27
An atlas of exotic variability in IGR J17091-3624: a comparison with GRS 1915+105
DOI: 10.1093/mnras/stx773 Bibcode: 2017MNRAS.468.4748C

Court, J. M. C.; Altamirano, D.; Belloni, T. +5 more

We performed an analysis of all Rossi X-ray Timing Explorer observations of the low-mass X-ray binary (LMXB) and black hole candidate IGR J17091-3624 during the 2011-2013 outburst of the source. By creating light curves, hardness-intensity diagrams and power density spectra of each observation, we have created a set of nine variability 'classes' t…

2017 Monthly Notices of the Royal Astronomical Society
INTEGRAL XMM-Newton 27
Modelling the ArH+ emission from the Crab nebula
DOI: 10.1093/mnras/stx2327 Bibcode: 2017MNRAS.472.4444P

Barlow, M. J.; Viti, S.; Priestley, F. D.

We have performed combined photoionization and photodissociation region (PDR) modelling of a Crab nebula filament subjected to the synchrotron radiation from the central pulsar wind nebula, and to a high flux of charged particles; a greatly enhanced cosmic-ray ionization rate over the standard interstellar value, ζ0, is required to acco…

2017 Monthly Notices of the Royal Astronomical Society
Herschel 27
The opposition effect of 67P/Churyumov-Gerasimenko on post-perihelion Rosetta images
DOI: 10.1093/mnras/stx1834 Bibcode: 2017MNRAS.469S.550H

Jorda, L.; Lamy, P. L.; Bertaux, J. -L. +45 more

High-resolution OSIRIS/Rosetta images of 67P/Churyumov-Gerasimenko acquired on the night run of 2016 April 9-10 show, at large scale, an opposition effect (OE) spot sweeping across Imhotep as the phase angle ranges from 0° to 17°. In this work, we fitted the phase curve of the whole surface imaged as well as three particular features using both th…

2017 Monthly Notices of the Royal Astronomical Society
Rosetta 27
A study of halo and relic radio emission in merging clusters using the Murchison Widefield Array
DOI: 10.1093/mnras/stx155 Bibcode: 2017MNRAS.467..936G

Callingham, J. R.; Johnston-Hollitt, M.; Intema, H. T. +18 more

We have studied radio haloes and relics in nine merging galaxy clusters using the Murchison Widefield Array (MWA). The images used for this study were obtained from the GaLactic and Extragalactic All-sky MWA (GLEAM) Survey which was carried out at five frequencies, viz. 88, 118, 154, 188 and 215 MHz. We detect diffuse radio emission in eight of th…

2017 Monthly Notices of the Royal Astronomical Society
XMM-Newton 27
ALMA constraints on star-forming gas in a prototypical z = 1.5 clumpy galaxy: the dearth of CO(5-4) emission from UV-bright clumps
DOI: 10.1093/mnras/stx1112 Bibcode: 2017MNRAS.469.4683C

Daddi, E.; Elbaz, D.; Rujopakarn, W. +13 more

We present deep ALMA CO(5-4) observations of a main-sequence, clumpy galaxy at z = 1.5 in the HUDF. Thanks to the ∼0{^''.}5 resolution of the ALMA data, we can link stellar population properties to the CO(5-4) emission on scales of a few kiloparsec. We detect strong CO(5-4) emission from the nuclear region of the galaxy, consistent with…

2017 Monthly Notices of the Royal Astronomical Society
eHST 27
Alignments of parity even/odd-only multipoles in CMB
DOI: 10.1093/mnras/stx2112 Bibcode: 2017MNRAS.472.2410A

Aluri, Pavan K.; Ralston, John P.; Weltman, Amanda

We compare the statistics of parity even and odd multipoles of the cosmic microwave background (CMB) sky from Planck full mission temperature measurements. An excess power in odd multipoles compared to even multipoles has previously been found on large angular scales. Motivated by this apparent parity asymmetry, we evaluate directional statistics …

2017 Monthly Notices of the Royal Astronomical Society
Planck 27
Quasar lenses and galactic streams: outlier selection and Gaia multiplet detection
DOI: 10.1093/mnras/stx1650 Bibcode: 2017MNRAS.471.2013A

Agnello, Adriano

I describe two novel techniques originally devised to select strongly lensed quasar candidates in wide-field surveys. The first relies on outlier selection in optical and mid-infrared magnitude space; the second combines mid-infrared colour selection with Gaia spatial resolution, to identify multiplets of objects with quasar-like colours. Both met…

2017 Monthly Notices of the Royal Astronomical Society
Gaia 27
Statistics of the fractional polarization of compact radio sources in Planck maps
DOI: 10.1093/mnras/stx1020 Bibcode: 2017MNRAS.469.2401B

Toffolatti, Luigi; Bonavera, Laura; González-Nuevo, Joaquin +1 more

In this work, we apply the stacking technique to estimate the average fractional polarization from 30 to 353 GHz of a primary sample of 1560 compact sources - essentially all radio sources - detected in the 30 GHz Planck all-sky map and listed in the second version of the Planck Catalogue of Compact Sources (PCCS2). We divide our primary sample in…

2017 Monthly Notices of the Royal Astronomical Society
Planck 27
Multiband study of RX J0838-2827 and XMM J083850.4-282759: a new asynchronous magnetic cataclysmic variable and a candidate transitional millisecond pulsar
DOI: 10.1093/mnras/stx1560 Bibcode: 2017MNRAS.471.2902R

D'Avanzo, P.; Campana, S.; Ribas, I. +23 more

In a search for the counterpart to the Fermi-LAT source 3FGL J0838.8-2829, we performed a multiwavelength campaign: in the X-ray band with Swift and XMM-Newton; in the infrared and optical with OAGH, ESO-NTT and IAC80; and in the radio with ATCA observations. We also used archival hard X-ray data obtained by INTEGRAL. We report on three X-ray sour…

2017 Monthly Notices of the Royal Astronomical Society
INTEGRAL XMM-Newton 27