The globaljetwatch spectrographs: A fibre-fed spectrograph for small telescopes

Proceedings of SPIE - The International Society for Optical Engineering 7014 (2008)

Authors:

FJ Clarke, AJ Gosling, S Doolin, P Goodall, S Perez, P Pattinson, R Makin, KM Blundell

Abstract:

The GlobalJetWatch project (www.globaljetwatch.net) will place small (0.5-metre) commerical telescopes in four schools around the world. Each telescope will be equipped with a custom designed spectrograph, currently being built by the Astrophysics sub-department of the University of Oxford. The scientific goal of the project is to provide continual monitoring of a rosetta stone object, the micro-quasar SS433. In addition,the project has a significant out-reach element, aiming to involve school children on four-continents in front-line astronomical research. The spectrograph is a fibre-fed fixed format cross-dispersed echellete design providing R 6000 spectra from 4300-8500Å in a single exposure. The spectrograph is built almost entirely from off-the-shelf components. The four GlobalJetWatch sites (Australia, India, South Africa,Chile) will be commissioned in 2008/09. Here we present the baseline design of the spectrograph, and initial results from the prototype on-sky commissioning in Oxford.

VLT Detection of a Red Supergiant Progenitor of the Type II-P Supernova 2008bk

The Astrophysical Journal American Astronomical Society 688:2 (2008) l91-l94

Authors:

S Mattila, SJ Smartt, JJ Eldridge, JR Maund, RM Crockett, IJ Danziger

X-ray jets from the X-ray binary cir X-1

International Conference Recent Advances in Natural Language Processing, RANLP (2008)

Authors:

P Soleri, S Heinz, R Fender, R Wijnands, V Tudose, D Altamirano, PG Jonker, M Van Der Klis, L Kuiper, C Kaiser, P Casella

Abstract:

We present the results of the analysis of two Chandra observations of Circinus X-1 performed in 2007, for a total exposure time of ∼50 ks. The source was observed with the High Resolution Camera during a long X-ray low-flux state of the source. Cir X-1 is an accreting neutron-star binary system that exhibits ultra-relativistic arcsec-scale radio jets and an extended arcmin-scale radio nebula. Furthermore, a recent paper has shown an X-ray excess on arcmin-scale prominent on the side of the receding radio jet. In our images we clearly detect X-ray structures both on the side of the receding and the approaching radio jet. The X-ray emission is consistent with being from synchrotron origin. Our detection is consistent with neutron-star binaries being as efficient as black-hole binaries in producing X-ray outflows, despite their shallower gravitational potential. © Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-ShareAlike Licence.

Supernova 1996cr: SN 1987A’s Wild Cousin?

The Astrophysical Journal American Astronomical Society 688:2 (2008) 1210-1234

Authors:

FE Bauer, VV Dwarkadas, WN Brandt, S Immler, S Smartt, N Bartel, MF Bietenholz

An anti-correlation between X-ray luminosity and H-alpha equivalent width in X-ray binaries

(2008)

Authors:

RP Fender, DM Russell, C Knigge, R Soria, RI Hynes, M Goad