papers

Publications (11)

astro-ph.SR2015

Spitzer Microlens Measurement of a Massive Remnant in a Well-Separated Binary

Y. Shvartzvald, A. Udalski, A. Gould +63

We report the detection and mass measurement of a binary lens OGLE-2015-BLG-1285La,b, with the more massive component having (80% probability). A main-sequence…

astro-ph2007

Silicate dust in the environment of RS Ophiuchi following the 2006 eruption

A. Evans, C. E. Woodward, L. A. Helton +20

We present further Spitzer Space Telescope observations of the recurrent nova RS Ophiuchi, obtained over the period 208-430 days after the 2006 eruption. The later Spitzer IRS data…

astro-ph2006

Infrared observations of the 2006 outburst of the recurrent nova RS Ophiuchi: the early phase

A. Evans, T. Kerr, Bin Yang +20

We present infrared spectroscopy of the recurrent nova RS Ophiuchi, obtained 11.81, 20.75 and 55.71 days following its 2006 eruption. The spectra are dominated by hydrogen recombin…

astro-ph.HE2011

An extremely luminous panchromatic outburst from the nucleus of a distant galaxy

A. J. Levan, N. R. Tanvir, S. B. Cenko +58

Variable X-ray and gamma-ray emission is characteristic of the most extreme physical processes in the Universe, and studying the sources of these energetic photons has been a major…

astro-ph2008

Metallicity and effective temperature of the secondary of RS Oph

Ya. V. Pavlenko, A. Evans, T. Kerr +6

The recurrent nova RS Oph undergoes nova eruptions every ~ 10-20years as a result of thermonuclear runaway on the surface of a white dwarf close to the Chandrasekhar limit. Both th…

astro-ph2003

A search for the optical and near-infrared counterpart of the accreting millisecond X-ray pulsar XTE J1751-305

P. G. Jonker, G. Nelemans, Z. Wang +14

We have obtained optical and near-infrared images of the field of the accreting millisecond X-ray pulsar XTE J1751-305. There are no stars in the 0.7'' error circle (0.7'' is the o…

astro-ph.SR2009

Changes in the red giant and dusty environment of the recurrent nova RS Ophiuchi following the 2006 eruption

M. T. Rushton, B. Kaminsky, D. K. Lynch +8

We present near infrared spectroscopy of the recurrent nova RS Oph obtained on several occasions after its latest outburst in 2006 February. The 1-5 mircon spectra are dominated by…

astro-ph2007

Spitzer and ground-based infrared observations of the 2006 eruption of RS Ophiuchi

A. Evans, C. E. Woodward, L. A. Helton +18

We present Spitzer Space Telescope and complementary ground-based infrared observations of the recurrent nova RS Ophiuchi, obtained over the period 64-111 days after the 2006 erupt…

astro-ph2000

Optical and Infrared Spectroscopy of the type IIn SN 1998S : Days 3-127

A. Fassia, W. P. S. Meikle, N. Chugai +14

We present contemporary infrared and optical spectroscopic observations of the type IIn SN 1998S for the period between 3 and 127 days after discovery. In the first week the spectr…

astro-ph.IM2017

The UKIRT Hemisphere Survey: Definition and J-band Data Release

S. Dye, A. Lawrence, M. A. Read +23

This paper defines the UK Infra-Red Telescope (UKIRT) Hemisphere Survey (UHS) and release of the remaining ~12,700 sq.deg of J-band survey data products. The UHS will provide conti…

astro-ph.CO2009

A glimpse of the end of the dark ages: the gamma-ray burst of 23 April 2009 at redshift 8.3

N. R. Tanvir, D. B. Fox, A. J. Levan +59

It is thought that the first generations of massive stars in the Universe were an important, and quite possibly dominant, source of the ultra-violet radiation that reionized the hy…