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THE BARYON OSCILLATION SPECTROSCOPIC SURVEY OF SDSS-III
The Baryon Oscillation Spectroscopic Survey (BOSS) is designed to measure the scale of baryon acoustic oscillations (BAO) in the clustering of matter over a larger volume than the combined efforts ofExpand
TOWARD THE STANDARD POPULATION SYNTHESIS MODEL OF THE X-RAY BACKGROUND: EVOLUTION OF X-RAY LUMINOSITY AND ABSORPTION FUNCTIONS OF ACTIVE GALACTIC NUCLEI INCLUDING COMPTON-THICK POPULATIONS
We present the most up-to-date X-ray luminosity function (XLF) and absorption function of Active Galactic Nuclei (AGNs) over the redshift range from 0 to 5, utilizing the largest, highly completeExpand
The XMM-Newton serendipitous survey. V. The Second XMM-Newton serendipitous source catalogue
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 characteristics ofExpand
Using the Bright Ultrahard XMM-Newton survey to define an IR selection of luminous AGN based on WISE colours
We present a highly complete and reliable mid-infrared (MIR) colour selection of luminous active galactic nucleus (AGN) candidates using the 3.4, 4.6 and 12 µm bands of the Widefield Infrared SurveyExpand
The XMM-Newton serendipitous survey - VII. The third XMM-Newton serendipitous source catalogue
© ESO, 2016.Context. Thanks to the large collecting area (3 × ∼1500 cm2 at 1.5 keV) and wide field of view (30′ across in full field mode) of the X-ray cameras on board the European Space AgencyExpand
An accreting pulsar with extreme properties drives an ultraluminous x-ray source in NGC 5907
TLDR
Observations showing that NGC 5907 ULX is instead an x-ray accreting neutron star (NS) with a spin period evolving from 1.43 seconds in 2003 to 1.13 seconds in 2014 suggest that other extreme ULXs (x-ray luminosity ≥ 1041 erg second−1) might harbor NSs. Expand
The Subaru/XMM-Newton Deep Survey (SXDS). III. X-Ray Data
TLDR
The X-ray source catalog in the Subaru/XMM-Newton deep survey is presented, bridging the flux range between Chandra deep surveys and brighter surveys and the averaged -->log N–log S relations are in good agreement with previous results. Expand
The evolution of the near-infrared galaxy luminosity function and colour bimodality up to z = 2 from the UKIDSS Ultra Deep Survey Early Data Release
We present new results on the cosmological evolution of the near-infrared (near-IR) galaxy luminosity function (LF), derived from the analysis of a new sample of ∼22 000 KAB≤ 22.5 galaxies selectedExpand
The Hot and Energetic Universe: A White Paper presenting the science theme motivating the Athena+ mission
This White Paper, submitted to the recent ESA call for science themes to define its future large missions, advocates the need for a transformational leap in our understanding of two key questions inExpand
The XMM-Newton Serendipitous Survey I. The role of XMM-Newton Survey Science Centre
This paper describes the performance of XMM-Newton for serendipitous surveys and summarises the scope and potential of the XMM-Newton Serendipitous Survey. The role of the Survey Science Centre (SSC)Expand
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