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Radiation from a Charged Particle in Periodic Media: Classical Theory
The method of pseudophotons, considered in the previous chapter, is convenient for qualitative analysis of parametric X-ray radiation (PXR). PXR in...
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Prospective Applications of PXR
The previous chapters concern the fundamental properties of PXR, which have been experimentally observed and theoretically explained. The most recent...
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14 Quantum Fields at Non-zero Temperature
The general structure discussed above provides a neat and unique prescription for the quantization of relativistic fields at non-zero temperature...
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8 Examples
The model describes the simplest non-linear field theory and it can be regarded as a prototype of field theories in one space dimension (s=1). The...
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Electromagnetic Radiation from a Charged Particle in Crystals: Qualitative Consideration
Electromagnetic radiation caused by motion of a charged particle has been studied for more than 100 years. It was firmly believed for an appreciable...
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The RASS-SDSS Galaxy Cluster Survey
Solid observational evidences indicate a strong dependence of the galaxy formation and evolution on the environment. In order to study in particular...
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SED Diagnostics of Submillimetre Galaxies
We apply an evolutionary SED model of starbursts to submm galaxies, in order to predict the present-day colour, magnitude, and size of submm...
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High Redshift Lyman Break Galaxies
Two of the most outstanding issues in modern astrophysics are what reionized the Universe and how did the first objects form. Observations of...
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Extremely Red Galaxies: Dust Attenuation and Classification
The “extremely red galaxies” (ERGs) constitute a controversial population in deep near-IR surveys. Their extremely-red observed colours (I...
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The Deepest Near-Infrared View of the Universe
We present very deep near-infrared imaging in the J s , H and K s -bands of the HDF-S and...
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A Spectroscopic Survey of the Submillimeter Galaxy Population: 85 Redshifts Using Keck/LRIS-B
We present spectroscopic identifications for a sample of 85 millimeter and submillimeter galaxies detected with the SCUBA/JCMT and MAMBO/IRAM30m...
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Galaxy Evolution in Three Dimensions: Time, Space and Mass
There are three major axes to describe the evolution of galaxies, namely, time (redshift), space (environment) and mass (stellar mass). In this...
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Chemo-Photometric Models of Ring Galaxies
The peculiar ring galaxies are formed as a result of cosmic interaction. An intruder galaxy plunges through the center of a disk galaxy triggering...
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Deep Submillimetre Imaging of Distant AGN: Visualising the Formation of Cluster Ellipticals
We Rob Ivison, Jason Stevens, James Dunlop, Ian Smail, Wil Percival, David Hughes, Huub Röttgering, Wil van Breugel and Michel...
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The Rest-Frame Optical Properties of Star-Forming Galaxies at z~2
We present preliminary results from Hα spectroscopy and deep K-band imaging of UV-selected star-forming galaxies at z~2. We see evidence for...
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Tracing the Evolution of Massive Galaxies up to z ~ 3
Objects with unusual red near-IR color J-K > 3 are extremely rare at magnitude brighter than K=20, while their surface density increases at fainter...
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Brightest Cluster Galaxy Formation in the Cluster C0037-2522: Flattening of the Dark Matter Cusp
The X-ray cluster C0337-2522 at redshift z = 0.59 hosts in its core a group of five elliptical galaxies. Using N-body simulations we show that a...
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Multiwavelength Maps of Simulations of Galaxy Formation
We performed smoothed particle hydro-dynamical simulations of isolated collapsing triaxial systems initially composed of dark matter (DM) and gas...
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Multiwavelength Study of the NEPR Sample. The 60 μm Luminosity Function
We present the 60 μm luminosity function (LF) of the deepest complete IRAS selected sample [1] so far available, in the North Ecliptic Polar Region...
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T-ReCS and Michelle: The Mid-Infrared Spectroscopic Capabilities of the Gemini Observatory
Gemini Observatory’s northern and southern telescopes are both presently being outfitted with facility mid-infrared imagers/spectrometers. This will...