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most citedThe XMM-Newton Serendipitous Survey. V. The Second XMM-Newton Serendipitous Source Catalogue

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astro-ph2008489 cited

The XMM-Newton Serendipitous Survey. V. The Second XMM-Newton Serendipitous Source Catalogue

M. G. Watson, A. C. Schröder, D. Fyfe +47

Aims: Pointed observations with XMM-Newton provide the basis for creating catalogues of X-ray sources detected serendipitously in each field. This paper describes the creation and…

astro-ph200756 cited

The XMM-Newton bright serendipitous survey. Identification and optical spectral properties

A. Caccianiga, P. Severgnini, R. Della Ceca +12

AIMS: We present the optical classification and redshift of 348 X-ray selected sources from the XMM-Newton Bright Serendipitous Survey (XBS) which contains a total of 400 objects (…

astro-ph200789 cited

The XMM-Newton Serendipitous Survey V. Optical identification of the XMM-Newton Medium sensitivity Survey (XMS)

X. Barcons, F. J. Carrera, M. T. Ceballos +53

We present the XMM-Newton Medium sensitivity Survey (XMS), including a total of 318 X-ray sources found among the serendipitous content of 25 XMM-Newton target fields. The XMS comp…

astro-ph2005

Gemini Spectroscopy of Supernovae from SNLS: Improving High Redshift SN Selection and Classification

D. A. Howell, M. Sullivan, K. Perrett +22

We present new techiques for improving the efficiency of supernova (SN) classification at high redshift using 64 candidates observed at Gemini North and South during the first year…

astro-ph2004

Discovery of high-amplitude X-ray variability in the Seyfert-LINER transition galaxy NGC7589

W. Yuan, St. Komossa, D. Xu +3

We present the first result of a programme to search for large flux variations in the X-ray sources of the XMM Serendipitous Survey compared to previous ROSAT observations. An incr…

astro-ph2002

The Hubble Diagram of Type Ia Supernovae as a Function of Host Galaxy Morphology

M. Sullivan, R. S. Ellis, G. Aldering +41

(Abridged) We present new results on the Hubble diagram of distant type Ia supernovae (SNe Ia) segregated according to the type of host galaxy. This makes it possible to check earl…