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Deep millimeter surveys : implications for galaxy formation and evolution, 19-21 June, 2000, University of Massachusetts, Amherst, USA /

The arrival of large submillimeter and millimeter-wave detector arrays opened a new window on galaxy formation and evolution. The major new facilities now being designed or constructed, such as ALMA (MMA) and the Large Millimeter Telescope (LMT), will soon be expanding the horizons even farther.The...

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Detalles Bibliográficos
Clasificación:Libro Electrónico
Autores Corporativos: UMass/INAOE Conference Amherst, Mass., Instituto Nacional de Astrofísica, Optica y Electrónica (Mexico), University of Massachusetts (Amherst campus)
Otros Autores: Hughes, David H., Lowenthal, James D.
Formato: Electrónico Congresos, conferencias eBook
Idioma:Inglés
Publicado: River Edge, N.J. : World Scientific, 2001.
Temas:
Acceso en línea:Texto completo

MARC

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245 1 0 |a Deep millimeter surveys :  |b implications for galaxy formation and evolution, 19-21 June, 2000, University of Massachusetts, Amherst, USA /  |c editors, James D. Lowenthal, David H. Hughes. 
260 |a River Edge, N.J. :  |b World Scientific,  |c 2001. 
300 |a 1 online resource 
336 |a text  |b txt  |2 rdacontent 
337 |a computer  |b c  |2 rdamedia 
338 |a online resource  |b cr  |2 rdacarrier 
500 |a "The UMass/INAOE Conference on 'Deep Millimeter Surveys: Implications For Galaxy Formation And Evolution' gathered together for the first time an international field of about 70 experts at the University of Massachusetts campus in Amherst from 19-21 June 2000 to compare notes ..."--Preface. 
504 |a Includes bibliographical references and index. 
505 0 |a Conference Organizing Committee; Preface; Contents; 1. Continuum Sub/mm Surveys; The Nature of Faint Submillimeter Galaxies; Sub-mm Clues to Elliptical Galaxy Formation; Multi-Wavelength Observations of Obscured Regions; Wide Field Imaging at 250 GHz; 2. Templates at Low Redshift; Molecular Gas in Galaxies in the Local Universe; The SCUBA Local Universe Galaxy Survey -- A low Redshift Benchmark for the Deep Submm Survey; The High-Resolution CO Survey of M31; 3. Facilities and Instrumentation; Millimeter Observations Using the Green Bank Telescope 
505 8 |a Some Prospects for High Redshift Galaxy Observations with the Submillimeter ArrayBLAST -- A Balloon-Borne Large Aperture Submillimeter Telescope; SCUBA-2 the Next Generation Wide-Field Submillimetre Camera for the JCMT; Semi Rigid and Adjustable CFRP Membrane for Radio Telescope Applications; An Instrument for Studying Galaxy Evolution on the 9.2-Meter Hobby-Eberly Telescope; 4. Source Counts and Counterparts of Submm Sources; Study of Lockman Hole ISOPHOT Sources; The Brighter Side of Sub-mm Source Counts: A SCUBA Scan-Map of the Hubble Deep Field; Sub-mm Counterparts to Lyman Break Galaxies 
505 8 |a Can Dusty Lyman Break Galaxies Produce the Submillimeter Counts and Background? Lessons from Lensed Lyman Break Galaxies5. Molecular Emission Lines at High Redshift; High Redshift CO Line Emission: Perspectives; CO and Near-Infrared Observations of High-Redshift Submillimeter Galaxies; 6. Clustering; The FIR-Radio Correlation in Nearby Clusters: Implications for the Radio-to-Submm Index Redshift Estimator; Clustering in Deep (Submillimetre) Surveys; Cluster Environments in the Early Universe: Probing Obscured Proto-Ellipticals with SCUBA 
505 8 |a 7. Sub-mm/mm Observations of Known (Low- and) High-Redshift SourcesThe SCUBA-Bright Quasar Survey (SBQS): The z > 4 Sample; High Resolution Imaging of ULIRGS; Known and Unknown SCUBA Sources; A Submillimeter Selected Quasar in the Field of Abell 478; 8. The Future of Deep Sub-mm and mm Serveys; Simulated Submillimetre Galaxy Surveys; SZ Effect in Young Massive Ellipticals?; FIR/Sub-mm Line Emission from the First Objects: Testing the Stellar Feedback; Numerical Simulation of the Sub-mm Galaxies; Selection Effects in High-Redshift Submillimeter Surveys and Pointed Observations 
520 |a The arrival of large submillimeter and millimeter-wave detector arrays opened a new window on galaxy formation and evolution. The major new facilities now being designed or constructed, such as ALMA (MMA) and the Large Millimeter Telescope (LMT), will soon be expanding the horizons even farther.The Conference on "Deep Millimeter Surveys: Implications for Galaxy Formation and Evolution" drew together the major international groups working on submillimeter and millimeter-wave galaxies to discuss their relation to other galaxies both near by and in the early Universe, the role of the LMT and othe. 
590 |a eBooks on EBSCOhost  |b EBSCO eBook Subscription Academic Collection - Worldwide 
650 0 |a Galaxies  |x Evolution  |v Congresses. 
650 0 |a Galaxies  |x Formation  |v Congresses. 
650 0 |a Millimeter astronomy  |v Congresses. 
650 0 |a Millimeter waves  |v Congresses. 
650 6 |a Galaxies  |x Évolution  |v Congrès. 
650 6 |a Galaxies  |x Formation  |v Congrès. 
650 6 |a Astronomie millimétrique  |v Congrès. 
650 6 |a Ondes millimétriques  |v Congrès. 
650 7 |a SCIENCE  |x Cosmology.  |2 bisacsh 
650 7 |a Galaxies  |x Evolution  |2 fast 
650 7 |a Galaxies  |x Formation  |2 fast 
650 7 |a Millimeter astronomy  |2 fast 
650 7 |a Millimeter waves  |2 fast 
655 7 |a Conference papers and proceedings  |2 fast 
700 1 |a Hughes, David H. 
700 1 |a Lowenthal, James D. 
710 2 |a Instituto Nacional de Astrofísica, Optica y Electrónica (Mexico) 
710 2 |a University of Massachusetts (Amherst campus) 
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