Catálogo de publicaciones - libros
Scientific detectors for astronomy 2005: Explorers of the Photon Odyssey
Jenna E. Beletic ; James W. Beletic ; Paola Amico (eds.)
Resumen/Descripción – provisto por la editorial
No disponible.
Palabras clave – provistas por la editorial
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Disponibilidad
Institución detectada | Año de publicación | Navegá | Descargá | Solicitá |
---|---|---|---|---|
No detectada | 2006 | SpringerLink |
Información
Tipo de recurso:
libros
ISBN impreso
978-1-4020-4329-1
ISBN electrónico
978-1-4020-4330-7
Editor responsable
Springer Nature
País de edición
Reino Unido
Fecha de publicación
2006
Información sobre derechos de publicación
© Springer 2006
Cobertura temática
Tabla de contenidos
– Science, Technology and Detectors for Extremely Large Telescopes
Roberto Gilmozzi
The Earth is the most geologically active of the terrestrial planets and it has retained the poorest sample of the record of hypervelocity impact by interplanetary bodies throughout geologic time. Although the surviving sample of impact structures is small, the terrestrial impact record has played a major role in understanding and constraining cratering processes, as well as providing important ground-truth information on the three dimensional lithological and structural character of impact structures (). Recently, there has been a growing awareness in the earth-science community that impact is also potentially important as a stochastic driving force for changes to the terrestrial environment. This has stemmed largely from: the discovery of chemical and physical evidence for the involvement of impact at the Cretaceous-Tertiary (K/T) boundary and the associated mass extinction event (e.g. ; ; ), and their relation to the Chicxulub impact structure in the Yucatan Peninsula, Mexico (), the recognition of the resource potential of impact structures, some of which are related to world-class ore deposits, both spatially and genetically (; ), and the recognition of the potentially disastrous consequences of impacts for human civilization ().
Section I - Observatory Status and Plans | Pp. 3-12
- Instruments, Detectors and the Future of Astronomy with Large Ground Based Telescopes
Douglas A. Simons; Paola Amico; Dietrich Baade; Sam Barden; Randall D. Campbell; Gert Finger; Kirk Gilmore; Roland Gredel; Paul Hickson; Steve Howell; Norbert Hubin; Andreas Kaufer; Ralf Kohley; Phillip J. MacQueen; Sergej Markelov; Mike Merrill; Satoshi Miyazaki; Hidehiko Nakaya; Darragh O'Donoghue; Tino Oliva; Andrea Richichi; Derrick Salmon; Ricardo Schmidt; Hongjun Su; Simon Tulloch; Maria Luisa García Vargas; R. Mark Wagner; Olivier Wiecha; Binxun Ye
The Earth is the most geologically active of the terrestrial planets and it has retained the poorest sample of the record of hypervelocity impact by interplanetary bodies throughout geologic time. Although the surviving sample of impact structures is small, the terrestrial impact record has played a major role in understanding and constraining cratering processes, as well as providing important ground-truth information on the three dimensional lithological and structural character of impact structures (). Recently, there has been a growing awareness in the earth-science community that impact is also potentially important as a stochastic driving force for changes to the terrestrial environment. This has stemmed largely from: the discovery of chemical and physical evidence for the involvement of impact at the Cretaceous-Tertiary (K/T) boundary and the associated mass extinction event (e.g. ; ; ), and their relation to the Chicxulub impact structure in the Yucatan Peninsula, Mexico (), the recognition of the resource potential of impact structures, some of which are related to world-class ore deposits, both spatially and genetically (; ), and the recognition of the potentially disastrous consequences of impacts for human civilization ().
Section I - Observatory Status and Plans | Pp. 13-44
Requirements on Array Detectors from OWL Instrument Studies
Sandro D'Odorico
The Earth is the most geologically active of the terrestrial planets and it has retained the poorest sample of the record of hypervelocity impact by interplanetary bodies throughout geologic time. Although the surviving sample of impact structures is small, the terrestrial impact record has played a major role in understanding and constraining cratering processes, as well as providing important ground-truth information on the three dimensional lithological and structural character of impact structures (). Recently, there has been a growing awareness in the earth-science community that impact is also potentially important as a stochastic driving force for changes to the terrestrial environment. This has stemmed largely from: the discovery of chemical and physical evidence for the involvement of impact at the Cretaceous-Tertiary (K/T) boundary and the associated mass extinction event (e.g. ; ; ), and their relation to the Chicxulub impact structure in the Yucatan Peninsula, Mexico (), the recognition of the resource potential of impact structures, some of which are related to world-class ore deposits, both spatially and genetically (; ), and the recognition of the potentially disastrous consequences of impacts for human civilization ().
Section I - Observatory Status and Plans | Pp. 45-52
Pan-STARRS and Gigapixel Cameras
John L. Tonry; Peter M. Onaka; Barry Burke; Gerard A. Luppino
The Earth is the most geologically active of the terrestrial planets and it has retained the poorest sample of the record of hypervelocity impact by interplanetary bodies throughout geologic time. Although the surviving sample of impact structures is small, the terrestrial impact record has played a major role in understanding and constraining cratering processes, as well as providing important ground-truth information on the three dimensional lithological and structural character of impact structures (). Recently, there has been a growing awareness in the earth-science community that impact is also potentially important as a stochastic driving force for changes to the terrestrial environment. This has stemmed largely from: the discovery of chemical and physical evidence for the involvement of impact at the Cretaceous-Tertiary (K/T) boundary and the associated mass extinction event (e.g. ; ; ), and their relation to the Chicxulub impact structure in the Yucatan Peninsula, Mexico (), the recognition of the resource potential of impact structures, some of which are related to world-class ore deposits, both spatially and genetically (; ), and the recognition of the potentially disastrous consequences of impacts for human civilization ().
Section I - Observatory Status and Plans | Pp. 53-62
The Large Synoptic Survey Telescope
D. Kirk Gilmore
The Earth is the most geologically active of the terrestrial planets and it has retained the poorest sample of the record of hypervelocity impact by interplanetary bodies throughout geologic time. Although the surviving sample of impact structures is small, the terrestrial impact record has played a major role in understanding and constraining cratering processes, as well as providing important ground-truth information on the three dimensional lithological and structural character of impact structures (). Recently, there has been a growing awareness in the earth-science community that impact is also potentially important as a stochastic driving force for changes to the terrestrial environment. This has stemmed largely from: the discovery of chemical and physical evidence for the involvement of impact at the Cretaceous-Tertiary (K/T) boundary and the associated mass extinction event (e.g. ; ; ), and their relation to the Chicxulub impact structure in the Yucatan Peninsula, Mexico (), the recognition of the resource potential of impact structures, some of which are related to world-class ore deposits, both spatially and genetically (; ), and the recognition of the potentially disastrous consequences of impacts for human civilization ().
Section I - Observatory Status and Plans | Pp. 63-72
Optical Detector Systems at the European Southern Observatory
Dietrich Baade;
The Earth is the most geologically active of the terrestrial planets and it has retained the poorest sample of the record of hypervelocity impact by interplanetary bodies throughout geologic time. Although the surviving sample of impact structures is small, the terrestrial impact record has played a major role in understanding and constraining cratering processes, as well as providing important ground-truth information on the three dimensional lithological and structural character of impact structures (). Recently, there has been a growing awareness in the earth-science community that impact is also potentially important as a stochastic driving force for changes to the terrestrial environment. This has stemmed largely from: the discovery of chemical and physical evidence for the involvement of impact at the Cretaceous-Tertiary (K/T) boundary and the associated mass extinction event (e.g. ; ; ), and their relation to the Chicxulub impact structure in the Yucatan Peninsula, Mexico (), the recognition of the resource potential of impact structures, some of which are related to world-class ore deposits, both spatially and genetically (; ), and the recognition of the potentially disastrous consequences of impacts for human civilization ().
Section I - Observatory Status and Plans | Pp. 73-80
The UKIRT Wide Field Camera
Derek Ives
The Earth is the most geologically active of the terrestrial planets and it has retained the poorest sample of the record of hypervelocity impact by interplanetary bodies throughout geologic time. Although the surviving sample of impact structures is small, the terrestrial impact record has played a major role in understanding and constraining cratering processes, as well as providing important ground-truth information on the three dimensional lithological and structural character of impact structures (). Recently, there has been a growing awareness in the earth-science community that impact is also potentially important as a stochastic driving force for changes to the terrestrial environment. This has stemmed largely from: the discovery of chemical and physical evidence for the involvement of impact at the Cretaceous-Tertiary (K/T) boundary and the associated mass extinction event (e.g. ; ; ), and their relation to the Chicxulub impact structure in the Yucatan Peninsula, Mexico (), the recognition of the resource potential of impact structures, some of which are related to world-class ore deposits, both spatially and genetically (; ), and the recognition of the potentially disastrous consequences of impacts for human civilization ().
Section I - Observatory Status and Plans | Pp. 81-86
System Design of Detector Systems for a Major Chinese Multi-Object Spectroscopic Sky Surveyor
Binxun Ye; Binhua Li
The Earth is the most geologically active of the terrestrial planets and it has retained the poorest sample of the record of hypervelocity impact by interplanetary bodies throughout geologic time. Although the surviving sample of impact structures is small, the terrestrial impact record has played a major role in understanding and constraining cratering processes, as well as providing important ground-truth information on the three dimensional lithological and structural character of impact structures (). Recently, there has been a growing awareness in the earth-science community that impact is also potentially important as a stochastic driving force for changes to the terrestrial environment. This has stemmed largely from: the discovery of chemical and physical evidence for the involvement of impact at the Cretaceous-Tertiary (K/T) boundary and the associated mass extinction event (e.g. ; ; ), and their relation to the Chicxulub impact structure in the Yucatan Peninsula, Mexico (), the recognition of the resource potential of impact structures, some of which are related to world-class ore deposits, both spatially and genetically (; ), and the recognition of the potentially disastrous consequences of impacts for human civilization ().
Section I - Observatory Status and Plans | Pp. 87-92
Near Diffraction Limited Visible Imaging on 10 m class Telescopes with EMCCDs
Craig D. Mackay
The Earth is the most geologically active of the terrestrial planets and it has retained the poorest sample of the record of hypervelocity impact by interplanetary bodies throughout geologic time. Although the surviving sample of impact structures is small, the terrestrial impact record has played a major role in understanding and constraining cratering processes, as well as providing important ground-truth information on the three dimensional lithological and structural character of impact structures (). Recently, there has been a growing awareness in the earth-science community that impact is also potentially important as a stochastic driving force for changes to the terrestrial environment. This has stemmed largely from: the discovery of chemical and physical evidence for the involvement of impact at the Cretaceous-Tertiary (K/T) boundary and the associated mass extinction event (e.g. ; ; ), and their relation to the Chicxulub impact structure in the Yucatan Peninsula, Mexico (), the recognition of the resource potential of impact structures, some of which are related to world-class ore deposits, both spatially and genetically (; ), and the recognition of the potentially disastrous consequences of impacts for human civilization ().
Section I - Observatory Status and Plans | Pp. 93-98
Nod & Shuffle 3D Spectroscopy
Martin M. Roth; Nicolas Cardiel; Javier Cenarro; Detlef Schönberner; Matthias Steffen
The Earth is the most geologically active of the terrestrial planets and it has retained the poorest sample of the record of hypervelocity impact by interplanetary bodies throughout geologic time. Although the surviving sample of impact structures is small, the terrestrial impact record has played a major role in understanding and constraining cratering processes, as well as providing important ground-truth information on the three dimensional lithological and structural character of impact structures (). Recently, there has been a growing awareness in the earth-science community that impact is also potentially important as a stochastic driving force for changes to the terrestrial environment. This has stemmed largely from: the discovery of chemical and physical evidence for the involvement of impact at the Cretaceous-Tertiary (K/T) boundary and the associated mass extinction event (e.g. ; ; ), and their relation to the Chicxulub impact structure in the Yucatan Peninsula, Mexico (), the recognition of the resource potential of impact structures, some of which are related to world-class ore deposits, both spatially and genetically (; ), and the recognition of the potentially disastrous consequences of impacts for human civilization ().
Section I - Observatory Status and Plans | Pp. 99-108