Rubin-LSST

Research group

Research theme

Sub department

About

The Nature of the Mid-Infrared Population from Optical Identifications of the ELAIS-S1 Sample

The Astronomical Journal American Astronomical Society 127:6 (2004) 3075-3088

Authors:

F La Franca, C Gruppioni, I Matute, F Pozzi, C Lari, M Mignoli, G Zamorani, DM Alexander, F Cocchia, L Danese, A Franceschini, P Héraudeau, JK Kotilainen, MJD Linden-Vørnle, S Oliver, M Rowan-Robinson, S Serjeant, L Spinoglio, A Verma
More details from the publisher

Using MgII to Investigate Quasars and Their Black-hole Masses

AGN Physics with the Sloan Digital Sky Survey 311 (2004) 79-79

Authors:

M Jarvis, R McLure
More details
Details from ArXiV

GRS 1915+105: The first three months with INTEGRAL

(2004)

Authors:

DC Hannikainen, O Vilhu, J Rodriguez, NJ Westergaard, S Shaw, GG Pooley, T Belloni, AA Zdziarski, RW Hunstead, K Wu, S Brandt, A Castro-Tirado, PA Charles, AJ Dean, Ph Durouchoux, RP Fender, P Hakala, CR Kaiser, AR King, N Lund, IF Mirabel, J Poutanen
More details from the publisher

Quenched millimetre emission from Cygnus X-1 in a soft X-ray state

(2004)

Authors:

SP Tigelaar, RP Fender, RPJ Tilanus, E Gallo, GG Poo ley
More details from the publisher

"Soft X-ray transient" outbursts which are not soft

New Astronomy 9:4 (2004) 249-264

Authors:

C Brocksopp, RM Bandyopadhyay, RP Fender

Abstract:

We have accumulated multiwavelength (X-ray, optical, radio) lightcurves for the eight black hole X-ray binaries which have been observed to enter a supposed 'soft X-ray transient' outburst, but remained in the low/hard state throughout the outburst. Comparison of the lightcurve morphologies, spectral behaviour, properties of the quasi-periodic oscillations and the radio jet provides the first study of such objects as a sub-class of X-ray transients. However, rather than assuming that these hard state X-ray transients are different from the 'canonical' soft X-ray transient, we prefer to consider the possibility that new analysis of both soft and hard state X-ray transients in a spectral context will provide a model capable of explaining the outburst mechanisms of (almost) all black hole X-ray binaries. © 2003 Elsevier B.V. All rights reserved.
More details from the publisher
Details from ArXiV