activity
20002007
most citedThe XMM-LSS survey. Survey design and first results

181 citations · 309 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph2007★ 43 cited

The XMM large scale structure survey: optical vs. X-ray classifications of active galactic nuclei and the unified scheme

O. Garcet, P. Gandhi, E. Gosset +25

Our goal is to characterize AGN populations by comparing their X-ray and optical classifications. We present a sample of 99 spectroscopically identified X-ray point sources in the…

astro-ph2003★ 181 cited

The XMM-LSS survey. Survey design and first results

M. Pierre, I. Valtchanov, B. Altieri +36

We have designed a medium deep large area X-ray survey with XMM - the XMM Large Scale Structure survey, XMM-LSS - with the scope of extending the cosmological tests attempted using…

astro-ph2002★ 12 cited

VLT near-infrared spectra of hard serendipitous Chandra sources

P. Gandhi, C. S. Crawford, A. C. Fabian

We present near-infrared long-slit spectra of eight optically-dim X-ray sources obtained with ISAAC on the Very Large Telescope. Six of the sources have hard X-ray emission with a…

astro-ph2001★ 29 cited

Multi-wavelength observations of serendipitous Chandra X-ray sources in the field of A2390

C. S. Crawford, P. Gandhi, A. C. Fabian +4

We present optical spectra and near-infrared imaging of a sample of serendipitous X-ray sources detected in the field of Chandra observations of the A2390 cluster of galaxies. The…

astro-ph2000★ 18 cited

Hot dust in two hard Chandra X-ray sources

R. J. Wilman, A. C. Fabian, P. Gandhi

The two brightest hard X-ray sources discovered serendipitously by Chandra in the field of the lensing cluster A2390 are found to have ISOCAM counterparts at 6.7 and 15 micron. We…

astro-ph2000★ 26 cited

Infrared observations of serendipitous hard Chandra X-ray sources

C. S. Crawford, A. C. Fabian, P. Gandhi +2

We present observations of a sample of optically-faint, hard X-ray sources of the kind likely to be responsible for much of the hard X-ray background. We confirm that such sources…