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Star forming galaxies represent a small yet sizable fraction of the X-ray sky (1%-20%, depending on the flux). X-ray surveys allow to derive their luminosity function and evolution, free from uncertainties due to absorption. However, much…

天体物理仪器与方法 · 物理学 2010-05-03 Piero Ranalli

I present the science goals and give a brief summary of the Wide Angle X-ray survey with a Wide Field X-ray Telescope (WAXS/WFXT) mission proposal (Phase A) which will be submitted to the Italian Space Agency (ASI) following the call for…

天体物理学 · 物理学 2007-05-23 Guido Chincarini

The Wide-Field X-ray Telescope (WFXT) is a proposed NASA mission dedicated to performing surveys of the sky in the soft X-ray band (0.3-6 keV). The key characteristics of this missions are a constant point spread function with Half Energy…

高能天体物理现象 · 物理学 2010-11-04 Sergio Campana

The Wide Field X-Ray Telescope (WFXT) is a medium-class mission designed to be 2-orders-of-magnitude more sensitive than any previous or planned X-ray mission for large area surveys and to match in sensitivity the next generation of…

宇宙学与河外天体物理 · 物理学 2010-11-01 P. Rosati , S. Borgani , R. Gilli , M. Paolillo , P. Tozzi , S. Murray , R. Giacconi , A. Ptak , M. Weisskopf , W. Forman , C. Jones , the WFXT Team

My Ph.D. Thesis is devoted to the study of groups and clusters of galaxies in the X-ray band. This field has been very active in the last ten years, thanks to the data gathered from the Chandra and XMM satellites. Clusters of galaxies are…

宇宙学与河外天体物理 · 物理学 2010-07-13 Andrea Bignamini

The Wide Field X-ray Telescope (WFXT) is a proposed mission with a high survey speed, due to the combination of large field of view (FOV) and effective area, i.e. grasp, and sharp PSF across the whole FOV. These characteristics make it…

We investigate the scientific impact of the Wide Field X-ray Telescope mission. We present simulated images and spectra of X-ray sources as observed from the three surveys planned for the nominal 5-year WFXT lifetime. The goal of these…

宇宙学与河外天体物理 · 物理学 2010-11-01 P. Tozzi , J. Santos , H. Yu , A. Bignamini , P. Rosati , S. Borgani , S. Campana , P. Conconi , R. Gilli , M. Paolillo , A. Ptak , the WFXT Team

Sensitive, wide-area X-ray surveys which would be possible with the WFXT will detect huge samples of virialized objects spanning the mass range from sub-groups to the most massive clusters, and extending in redshift to beyond z=2. These…

Observations of star-forming galaxies in the distant Universe have confirmed the importance of massive stars in shaping galaxy emission and evolution. Distant stellar populations are unresolved, and the limited data available must be…

星系天体物理 · 物理学 2020-06-10 E R Stanway , J J Eldridge

The stellar populations of galaxies contain a wealth of detailed information. From the youngest, most massive stars, to almost invisible remnants, the history of star formation is encoded in the stars that make up a galaxy. Extracting some,…

宇宙学与河外天体物理 · 物理学 2015-05-14 Jarle Brinchmann

Observations of star-forming galaxies in the distant Universe (z > 2) are starting to confirm the importance of massive stars in shaping galaxy emission and evolution. Inevitably, these distant stellar populations are unresolved, and the…

星系天体物理 · 物理学 2017-11-15 Elizabeth R. Stanway

We discuss some of the main open issues in the evolution of Active Galactic Nuclei which can be solved by the sensitive, wide area surveys to be performed by the proposed Wide Field X-ray Telescope mission.

宇宙学与河外天体物理 · 物理学 2010-11-01 R. Gilli , P. Tozzi , P. Rosati , M. Paolillo , S. Borgani , M. Brusa , A. Comastri , E. Lusso , F. Marulli , C. Vignali

This review aims to give a summary of our understanding of galaxy evolution as infered from studies of nearby galaxies; how observations made with the Hubble Space Telescope have contributed significantly to our detailed understanding of…

天体物理学 · 物理学 2007-05-23 Eline Tolstoy

One of the aims of LSST is to perform a systematic survey of star clusters and star forming regions (SFRs) in our Galaxy. In particular, the observations obtained with LSST will make a big difference in Galactic regions that have been…

Rapid progress is now being made in the study of stellar populations of galaxies at large lookback times, both in dense clusters and the field. Dramatic transformations in star formation histories (even morphologies) appear to prevail among…

天体物理学 · 物理学 2009-10-31 Robert W. O'Connell

In this short survey of the applications of wide-field, multi-object spectroscopy to galaxy evolution, large-scale structure and cosmology, I interleave summaries of the general goals and state of play in these fields with specific examples…

天体物理学 · 物理学 2016-01-27 Matthew Colless

What the future holds for the stellar populations of the Milky Way Galaxy may (optimistically) be predicted by study of their past histories, as written in the chemical abundance distributions, angular momentum distributions, velocity…

天体物理学 · 物理学 2007-05-23 Rosemary F. G. Wyse

The last decade has seen enormous progress in understanding the structure of the Milky Way and neighboring galaxies via the production of large-scale digital surveys of the sky like 2MASS and SDSS, as well as specialized, counterpart…

星系天体物理 · 物理学 2015-05-18 Steven R. Majewski

Galaxies are essential building blocks in the Universe. However they are faint and complex X-ray sources and require high performance instrumentation to be properly studied. Yet they are fundamental for our understanding of the Universe,…

宇宙学与河外天体物理 · 物理学 2010-11-15 G. Trinchieri , A. Wolter
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