Possible arcminute-separation gravitational lensed QSOs in the 2dF QSO survey

ArXiv astro-ph/0210644 (2002)

Authors:

L Miller, AM Lopes, RJ Smith, SM Croom, BJ Boyle, T Shanks, P Outram

Abstract:

We report the possible discovery of multiple gravitationally-lensed images of QSOs with angular separations on arcminute scales. The QSOs were selected from the completed 2dF QSO survey as having redshifts and optical colours which are statistically consistent. In this paper we present higher-quality optical spectra of the candidates and discuss the likelihood of their genuinely being systems lensed by massive clusters of galaxies. From a comparison of the spectra it appears that up to six pairs of QSOs may be lensed multiple images, although the true number may be less than that and further observations should be undertaken to amass more evidence and to detect the lensing clusters. Two of the candidates may be associated with low redshift clusters of galaxies.

Collision-induced galaxy formation: semi-analytical model and multi-wavelength predictions

(2002)

Authors:

Christophe Balland, Julien EG Devriendt, Joe Silk

On the black hole mass-radio luminosity relation for flat-spectrum radio-loud quasars

\mnras 336 (2002) L38-L42-L38-L42

Authors:

MJ Jarvis, RJ McLure

Non-Standard Structure Formation Scenarios

(2002)

Authors:

Alexander Knebe, Brett Little, Ranty Islam, Julien Devriendt, Asim Mahmood, Joe Silk

White dwarfs in the 2dF QSO redshift survey - I. Hydrogen-rich (DA) stars

Monthly Notices of the Royal Astronomical Society 335:3 (2002) 673-686

Authors:

S Vennes, RJ Smith, BJ Boyle, SM Croom, A Kawka, T Shanks, L Miller, N Loaring

Abstract:

We report the spectroscopic identification of close to 1000 hydrogen-rich (DA) white dwarfs discovered in the course of the Anglo-Australian 2dF QSO Redshift Survey (2QZ). We measured the atmospheric parameters of a subsample of 201 stars based on good-quality Balmer line spectra and we determine the 2QZ population characteristics. Over ten per cent of the sample are potential ZZ Ceti variables. We estimate the DA white dwarf birthrate (bDA = 0.5-1.0 × 10-12 yr-1 pc-3) and the scaleheight (h = 220-300 pc) of the population in the thin disc of the Galaxy by combining information acquired in the Palomar-Green, AAT-UVX and new 2QZ surveys. White dwarfs appear related to G and late-F progenitors. A catalogue of 201 DA white dwarfs is presented.