Gravitational lensing: strong, weak and micro:
Saved in:
| Format: | Conference Proceeding Book |
|---|---|
| Language: | English |
| Published: |
Berlin [u.a.]
Springer
2006
|
| Edition: | [Überarb. Ausg.] |
| Subjects: | |
| Online Access: | Inhaltsverzeichnis |
| Item Description: | Literaturangaben |
| Physical Description: | XIII, 552 S. Ill., graph. Darst. |
| ISBN: | 9783540303091 354030309X |
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| 245 | 1 | 0 | |a Gravitational lensing: strong, weak and micro |c Saas Fee Advanced Course 33. P. Schneider ; C. Kochanek ; J. Wambsganss. Swiss Society for Astrophysics and Astronomy. Ed. by G. Meylan ... |
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| adam_text | P. SCHNEIDER C. KOCHANEK J. WAMBSGANSS GRAVITATIONAL LENSING: STRONG,
WEAK AND MICRO SAAS-FEE ADVANCED COURSE 33 SWISS SOCIETY FOR
ASTROPHYSICS AND ASTRONOMY EDITED BY G. MEYLAN, P. JETZER AND P. NORTH
WITH 196 ILLUSTRATIONS, 36 IN COLOR ^Y SPRINGER CONTENTS PART 1:
INTRODUCTION TO GRAVITATIONAL LENSING AND COSMOLOGY P. SCHNEIDER 1 1
INTRODUCTION 1 1.1 HISTORY OF GRAVITATIONAL LIGHT DEFLECTION 2 1.2
DISCOVERIES 5 1.3 WHAT IS LENSING GOOD FOR? 14 2 GRAVITATIONAL LENS
THEORY 18 2.1 THE DEFLECTION ANGLE 18 2.2 THE LENS EQUATION 20 2.3
MAGNIFICATION AND DISTORTION 23 2.4 CRITICAL CURVES AND CAUSTICS, AND
GENERAL PROPERTIES OF LENSES 25 2.5 THE MASS-SHEET DEGENERACY 29 3
SIMPLE LENS MODELS 31 3.1 AXIALLY SYMMETRIC LENSES 31 3.2 THE POINT-MASS
LENS 34 3.3 THE SINGULAR ISOTHERMAL SPHERE 36 3.4 NON-SYMMETRIC LENSES
38 4 THE COSMOLOGICAL STANDARD MODEL I: THE HOMOGENEOUS UNIVERSE ... 44
4.1 THE COSMIC EXPANSION 44 4.2 DISTANCES AND VOLUMES 49 4.3
GRAVITATIONAL LENSING IN COSMOLOGY 52 5 BASICS OF LENSING STATISTICS 54
5.1 CROSS-SECTIONS 55 5.2 LENSING PROBABILITIES; OPTICAL DEPTH 57 5.3
MAGNIFICATION BIAS 58 6 THE COSMOLOGICAL STANDARD MODEL II: THE
INHOMOGENEOUS UNIVERSE . 61 6.1 STRUCTURE FORMATION 61 6.2 HALO
ABUNDANCE AND PROFILE 71 X CONTENTS 6.3 THE CONCORDANCE MODEL 77 6.4
CHALLENGES 81 7 FINAL REMARKS 83 REFERENCES 84 PART 2: STRONG
GRAVITATIONAL LENSING C. S. KOCHANEK 91 1 INTRODUCTION 91 2 AN
INTRODUCTION TO THE DATA 92 3 BASIC PRINCIPLES 97 3.1 SOME NOMENCLATURE
98 3.2 CIRCULAR LENSES 101 3.3 NON-CIRCULAR LENSES 112 4 THE MASS
DISTRIBUTIONS OF GALAXIES 121 4.1 COMMON MODELS FOR THE MONOPOLE 125 4.2
THE EFFECTIVE SINGLE SCREEN LENS 129 4.3 CONSTRAINING THE MONOPOLE 130
4.4 THE ANGULAR STRUCTURE OF LENSES 136 4.5 CONSTRAINING ANGULAR
STRUCTURE 140 4.6 MODEL FITTING AND THE MASS DISTRIBUTION OF LENSES 143
4.7 NON-PARAMETRIC MODELS .. ... 150 4.8 STATISTICAL CONSTRAINTS ON MASS
DISTRIBUTIONS 152 4.9 STELLAR DYNAMICS AND LENSING 158 5 TIME DELAYS 163
5.1 A. GENERAL THEORY OF TIME DELAYS 165 5.2 TIME DELAY LENSES IN GROUPS
OR CLUSTERS 169 5.3 OBSERVING TIME DELAYS AND TIME.DELAY LENSES ....,
170 5.4 RESULTS: THE HUBBLE CONSTANT AND DARK MATTER . . . . . 174 5.5
THE FUTURE OF TIME DELAY MEASUREMENTS 181 6 GRAVITATIONAL LENS
STATISTICS . . . 182 6.1 THE MECHANICS OF SURVEYS : . . . 182 6.2 THE
LENS POPULATION 185 6.3 CROSS SECTIONS . . . . 192 6.4 OPTICAL DEPTH .
* 193 6.5 SPIRAL GALAXY LENSES ..;........ 196 6.6 MAGNIFICATION BIAS
197 6.7 COSMOLOGY WITH LENS STATISTICS 205 6.8 THE CURRENT STATE . .. .
-. 206 7 WHAT HAPPENED TO THE CLUSTER LENSES? 210 7.1 THE EFFECTS OF
HALO STRUCTURE AND THE POWER SPECTRUM ....... 216 7.2 BINARY QUASARS
.........:.. .. 218 8 THE ROLE OF SUBSTRUCTURE 221 8.1 LOW MASS DARK
HALOS . ..:* .. .;: 230 9 THE OPTICAL PROPERTIES OF LENS GALAXIES 232
9.1 THE INTERSTELLAR MEDIUM OF LENS GALAXIES 238 CONTENTS XI 10 EXTENDED
SOURCES AND QUASAR HOST GALAXIES 243 10.1 AN ANALYTIC MODEL FOR EINSTEIN
RINGS 243 10.2 NUMERICAL MODELS OF EXTENDED LENSED SOURCES 248 10.3
LENSED QUASAR HOST GALAXIES 251 11 DOES STRONG LENSING HAVE A FUTURE?
... . 255 REFERENCES 256 PART 3: WEAK GRAVITATIONAL LENSING P.
SCHNEIDER 269 1 INTRODUCTION 269 2 THE PRINCIPLES OF WEAK GRAVITATIONAL
LENSING 272 2.1 DISTORTION OF FAINT GALAXY IMAGES 272 2.2 MEASUREMENTS
OF SHAPES AND SHEAR 274 2.3 TANGENTIAL AND CROSS COMPONENT OF SHEAR 277
2.4 MAGNIFICATION EFFECTS 280 3 OBSERVATIONAL ISSUES AND CHALLENGES 281
3.1 STRATEGY 282 3.2 DATA REDUCTION: INDIVIDUAL FRAMES 284 3.3 DATA
REDUCTION: COADDITION 288 3.4 IMAGE ANALYSIS 292 3.5 SHAPE MEASUREMENTS
295 4 CLUSTERS OF GALAXIES: INTRODUCTION, AND STRONG LENSING 298 4.1
INTRODUCTION 298 4.2 GENERAL PROPERTIES OF CLUSTERS 299 4.3 THE MASS OF
GALAXY CLUSTERS 301 4.4 LUMINOUS ARCS AND MULTIPLE IMAGES 304 4.5
RESULTS FROM STRONG LENSING IN CLUSTERS 309 5 MASS RECONSTRUCTIONS FROM
WEAK LENSING 315 5.1 THE KAISER-SQUIRES INVERSION 316 5.2 IMPROVEMENTS
AND GENERALIZATIONS 317 5.3 INVERSE METHODS 324 5.4 PARAMETERIZED MASS
MODELS 327 5.5 PROBLEMS OF WEAK LENSING CLUSTER MASS RECONSTRUCTION AND
MASS DETERMINATION 330 5.6 RESULTS 333 5.7 APERTURE MASS AND OTHER
APERTURE MEASURES 343 5.8 MASS DETECTION OF CLUSTERS 346 6 COSMIC SHEAR
- LENSING BY THE LSS : 355 6.1 LIGHT PROPAGATION IN AN INHOMOGENEOUS
UNIVERSE 356 6.2 COSMIC SHEAR: THE PRINCIPLE 358 6.3 SECOND-ORDER COSMIC
SHEAR MEASURES 360 6.4 COSMIC SHEAR AND COSMOLOGY 366 6.5 E-MODES,
B-MODES 371 6.6 PREDICTIONS; RAY-TRACING SIMULATIONS 377 XII CONTENTS 7
LARGE-SCALE STRUCTURE LENSING: RESULTS 382 7.1 EARLY DETECTIONS OF
COSMIC SHEAR 383 7.2 INTEGRITY OF THE RESULTS 384 7.3 RECENT COSMIC
SHEAR SURVEYS 386 7.4 DETECTION OF B-MODES 392 7.5 COSMOLOGICAL
CONSTRAINTS 394 7.6 3-D LENSING 397 7.7 DISCUSSION 400 8 THE MASS OF,
AND ASSOCIATED WITH GALAXIES 404 8.1 INTRODUCTION 404 8.2 GALAXY-GALAXY
LENSING 405 8.3 GALAXY BIASING: SHEAR METHOD 416 8.4 GALAXY BIASING:
MAGNIFICATION METHOD 427 9 ADDITIONAL ISSUES IN COSMIC SHEAR 430 9.1
HIGHER-ORDER STATISTICS 430 9.2 INFLUENCE OF LSS LENSING ON LENSING BY
CLUSTERS AND GALAXIES 436 10 CONCLUDING REMARKS 439 REFERENCES 442 PART
4: GRAVITATIONAL MICROLENSING J. WAMBSGANSS 453 1 LENSING OF SINGLE
STARS BY SINGLE STARS 454 1.1 BRIEF HISTORY 454 1.2 THEORETICAL
BACKGROUND 454 1.3 HOW GOOD IS THE POINT LENS - POINT SOURCE
APPROXIMATION? 458 1.4 STATISTICAL ENSEMBLES 460 2 BINARY LENSES 461 2.1
THEORY AND BASICS OF BINARY LENSING 462 2.2 FIRST MICROLENSING
LIGHTCURVE OF A BINARY LENS: OGLE-7. . . . . . 466 2.3 BINARY LENS MACHO
1998-SMC-L 467 2.4 BINARY LENS MACHO 1999-BLG-047 471 2.5 BINARY LENS
EROS BLG-2000-005 472 3 MICROLENSING AND DARK MATTER: IDEAS, SURVEYS AND
RESULTS 475 3.1 WHY WE NEED DARK MATTER: FLAT ROTATION CURVES (1970S)
,475 3.2 HOW TO SEARCH FOR COMPACT DARK MATTER (AS OF 1986) 477 3.3 JUST
DO IT: MACHO, EROS, OGLE ET AL. (AS OF 1989) 477 3.4 PIXEL -LENSING:
ADVANTAGE ANDROMEDA! 478 3.5 CURRENT INTERPRETATION OF MICROLENSING
SURVEYS WITH RESPECT TO HALO DARK MATTER (AS OF 2004) 479 3.6
MICROLENSING TOWARD THE GALACTIC BULGE 484 4 MICROLENSING SURVEYS IN
SEARCH OF EXTRASOLAR PLANETS 486 4.1 HOW DOES THE MICROLENSING SEARCH
FOR EXTRASOLAR PLANET WORK? THE METHOD 486 CONTENTS XIII 4.2 WHY SEARCH
FOR EXTRASOLAR PLANETS WITH MICROLENSING? - ADVANTAGES AND DISADVANTAGES
488 4.3 WHO IS SEARCHING? THE TEAMS: OGLE, MOA, PLANET, MICROFUN 492 4.4
WHAT IS THE STATUS OF MICROLENSING PLANET SEARCHES SO FAR? THE RESULTS
493 4.5 WHEN WILL PLANETS BE DETECTED WITH MICROLENSING? THE PROSPECTS
496 4.6 NOTE ADDED IN APRIL 2004 (ABOUT ONE YEAR AFTER THE 33RD SAAS FEE
ADVANCED COURSE) 497 4.7 SUMMARY 497 5 HIGHER ORDER EFFECTS IN
MICROLENSING: 499 6 ASTROMETRIC MICROLENSING 516 7 QUASAR MICROLENSING
520 7.1 MICROLENSING MASS, LENGTH AND TIME SCALES 521 7.2 EARLY AND
RECENT THEORETICAL WORK ON QUASAR MICROLENSING. . . 524 7.3
OBSERVATIONAL EVIDENCE FOR QUASAR MICROLENSING 526 7.4 QUASAR
MICROLENSING: NOW AND FOREVER? 534 REFERENCES -. 536 INDE;C 541
|
| adam_txt |
P. SCHNEIDER C. KOCHANEK J. WAMBSGANSS GRAVITATIONAL LENSING: STRONG,
WEAK AND MICRO SAAS-FEE ADVANCED COURSE 33 SWISS SOCIETY FOR
ASTROPHYSICS AND ASTRONOMY EDITED BY G. MEYLAN, P. JETZER AND P. NORTH
WITH 196 ILLUSTRATIONS, 36 IN COLOR ^Y SPRINGER CONTENTS PART 1:
INTRODUCTION TO GRAVITATIONAL LENSING AND COSMOLOGY P. SCHNEIDER 1 1
INTRODUCTION 1 1.1 HISTORY OF GRAVITATIONAL LIGHT DEFLECTION 2 1.2
DISCOVERIES 5 1.3 WHAT IS LENSING GOOD FOR? 14 2 GRAVITATIONAL LENS
THEORY 18 2.1 THE DEFLECTION ANGLE 18 2.2 THE LENS EQUATION 20 2.3
MAGNIFICATION AND DISTORTION 23 2.4 CRITICAL CURVES AND CAUSTICS, AND
GENERAL PROPERTIES OF LENSES 25 2.5 THE MASS-SHEET DEGENERACY 29 3
SIMPLE LENS MODELS 31 3.1 AXIALLY SYMMETRIC LENSES 31 3.2 THE POINT-MASS
LENS \ 34 3.3 THE SINGULAR ISOTHERMAL SPHERE 36 3.4 NON-SYMMETRIC LENSES
38 4 THE COSMOLOGICAL STANDARD MODEL I: THE HOMOGENEOUS UNIVERSE . 44
4.1 THE COSMIC EXPANSION 44 4.2 DISTANCES AND VOLUMES 49 4.3
GRAVITATIONAL LENSING IN COSMOLOGY 52 5 BASICS OF LENSING STATISTICS 54
5.1 CROSS-SECTIONS 55 5.2 LENSING PROBABILITIES; OPTICAL DEPTH 57 5.3
MAGNIFICATION BIAS 58 6 THE COSMOLOGICAL STANDARD MODEL II: THE
INHOMOGENEOUS UNIVERSE . 61 6.1 STRUCTURE FORMATION 61 6.2 HALO
ABUNDANCE AND PROFILE 71 X CONTENTS 6.3 THE CONCORDANCE MODEL 77 6.4
CHALLENGES 81 7 FINAL REMARKS 83 REFERENCES 84 PART 2: STRONG
GRAVITATIONAL LENSING C. S. KOCHANEK 91 1 INTRODUCTION 91 2 AN
INTRODUCTION TO THE DATA 92 3 BASIC PRINCIPLES 97 3.1 SOME NOMENCLATURE
98 3.2 CIRCULAR LENSES 101 3.3 NON-CIRCULAR LENSES 112 4 THE MASS
DISTRIBUTIONS OF GALAXIES 121 4.1 COMMON MODELS FOR THE MONOPOLE 125 4.2
THE EFFECTIVE SINGLE SCREEN LENS 129 4.3 CONSTRAINING THE MONOPOLE 130
4.4 THE ANGULAR STRUCTURE OF LENSES 136 4.5 CONSTRAINING ANGULAR
STRUCTURE 140 4.6 MODEL FITTING AND THE MASS DISTRIBUTION OF LENSES 143
4.7 NON-PARAMETRIC MODELS .'. 150 4.8 STATISTICAL CONSTRAINTS ON MASS
DISTRIBUTIONS 152 4.9 STELLAR DYNAMICS AND LENSING 158 5 TIME DELAYS 163
5.1 A. GENERAL THEORY OF TIME DELAYS 165 5.2 TIME DELAY LENSES IN GROUPS
OR CLUSTERS 169 5.3 OBSERVING TIME DELAYS AND TIME.DELAY LENSES .,
170 5.4 RESULTS: THE HUBBLE CONSTANT AND DARK MATTER .". . . . 174 5.5
THE FUTURE OF TIME DELAY MEASUREMENTS 181 6 GRAVITATIONAL LENS
STATISTICS . . . 182 6.1 THE MECHANICS OF SURVEYS : . . . 182 6.2 THE
LENS POPULATION 185 6.3 CROSS SECTIONS '. . . .' 192 6.4 OPTICAL DEPTH .
* 193 6.5 SPIRAL GALAXY LENSES .;. 196 6.6 MAGNIFICATION BIAS
197 6.7 COSMOLOGY WITH LENS STATISTICS 205 6.8 THE CURRENT STATE . . .
-. 206 7 WHAT HAPPENED TO THE CLUSTER LENSES? 210 7.1 THE EFFECTS OF
HALO STRUCTURE AND THE POWER SPECTRUM . 216 7.2 BINARY QUASARS
.:. '. 218 8 THE ROLE OF SUBSTRUCTURE 221 8.1 LOW MASS DARK
HALOS '. .:* .'.;: 230 9 THE OPTICAL PROPERTIES OF LENS GALAXIES 232
9.1 THE INTERSTELLAR MEDIUM OF LENS GALAXIES 238 CONTENTS XI 10 EXTENDED
SOURCES AND QUASAR HOST GALAXIES 243 10.1 AN ANALYTIC MODEL FOR EINSTEIN
RINGS 243 10.2 NUMERICAL MODELS OF EXTENDED LENSED SOURCES 248 10.3
LENSED QUASAR HOST GALAXIES 251 11 DOES STRONG LENSING HAVE A FUTURE?
."." 255 REFERENCES 256 PART 3: WEAK GRAVITATIONAL LENSING P.
SCHNEIDER 269 1 INTRODUCTION 269 2 THE PRINCIPLES OF WEAK GRAVITATIONAL
LENSING 272 2.1 DISTORTION OF FAINT GALAXY IMAGES 272 2.2 MEASUREMENTS
OF SHAPES AND SHEAR 274 2.3 TANGENTIAL AND CROSS COMPONENT OF SHEAR 277
2.4 MAGNIFICATION EFFECTS 280 3 OBSERVATIONAL ISSUES AND CHALLENGES 281
3.1 STRATEGY 282 3.2 DATA REDUCTION: INDIVIDUAL FRAMES 284 3.3 DATA
REDUCTION: COADDITION 288 3.4 IMAGE ANALYSIS 292 3.5 SHAPE MEASUREMENTS
295 4 CLUSTERS OF GALAXIES: INTRODUCTION, AND STRONG LENSING 298 4.1
INTRODUCTION 298 4.2 GENERAL PROPERTIES OF CLUSTERS 299 4.3 THE MASS OF
GALAXY CLUSTERS 301 4.4 LUMINOUS ARCS AND MULTIPLE IMAGES 304 4.5
RESULTS FROM STRONG LENSING IN CLUSTERS 309 5 MASS RECONSTRUCTIONS FROM
WEAK LENSING 315 5.1 THE KAISER-SQUIRES INVERSION 316 5.2 IMPROVEMENTS
AND GENERALIZATIONS 317 5.3 INVERSE METHODS 324 5.4 PARAMETERIZED MASS
MODELS 327 5.5 PROBLEMS OF WEAK LENSING CLUSTER MASS RECONSTRUCTION AND
MASS DETERMINATION 330 5.6 RESULTS 333 5.7 APERTURE MASS AND OTHER
APERTURE MEASURES 343 5.8 MASS DETECTION OF CLUSTERS 346 6 COSMIC SHEAR
- LENSING BY THE LSS : 355 6.1 LIGHT PROPAGATION IN AN INHOMOGENEOUS
UNIVERSE 356 6.2 COSMIC SHEAR: THE PRINCIPLE 358 6.3 SECOND-ORDER COSMIC
SHEAR MEASURES 360 6.4 COSMIC SHEAR AND COSMOLOGY 366 6.5 E-MODES,
B-MODES 371 6.6 PREDICTIONS; RAY-TRACING SIMULATIONS 377 XII CONTENTS 7
LARGE-SCALE STRUCTURE LENSING: RESULTS 382 7.1 EARLY DETECTIONS OF
COSMIC SHEAR 383 7.2 INTEGRITY OF THE RESULTS 384 7.3 RECENT COSMIC
SHEAR SURVEYS 386 7.4 DETECTION OF B-MODES 392' 7.5 COSMOLOGICAL
CONSTRAINTS 394 7.6 3-D LENSING 397 7.7 DISCUSSION 400 8 THE MASS OF,
AND ASSOCIATED WITH GALAXIES 404 8.1 INTRODUCTION 404 8.2 GALAXY-GALAXY
LENSING 405 8.3 GALAXY BIASING: SHEAR METHOD 416 8.4 GALAXY BIASING:
MAGNIFICATION METHOD 427 9 ADDITIONAL ISSUES IN COSMIC SHEAR 430 9.1
HIGHER-ORDER STATISTICS 430 9.2 INFLUENCE OF LSS LENSING ON LENSING BY
CLUSTERS AND GALAXIES 436 10 CONCLUDING REMARKS 439 REFERENCES 442 PART
4: GRAVITATIONAL MICROLENSING J. WAMBSGANSS 453 1 LENSING OF SINGLE
STARS BY SINGLE STARS 454 1.1 BRIEF HISTORY 454 1.2 THEORETICAL
BACKGROUND 454 1.3 HOW GOOD IS THE POINT LENS - POINT SOURCE
APPROXIMATION? 458 1.4 STATISTICAL ENSEMBLES 460 2 BINARY LENSES 461 2.1
THEORY AND BASICS OF BINARY LENSING 462 2.2 FIRST MICROLENSING
LIGHTCURVE OF A BINARY LENS: OGLE-7. . .\. . . 466 2.3 BINARY LENS MACHO
1998-SMC-L 467 2.4 BINARY LENS MACHO 1999-BLG-047 471 2.5 BINARY LENS
EROS BLG-2000-005 472 3 MICROLENSING AND DARK MATTER: IDEAS, SURVEYS AND
RESULTS 475 3.1 WHY WE NEED DARK MATTER: FLAT ROTATION CURVES (1970S)
,475 3.2 HOW TO SEARCH FOR COMPACT DARK MATTER (AS OF 1986) 477 3.3 JUST
DO IT: MACHO, EROS, OGLE ET AL. (AS OF 1989) 477 3.4 "PIXEL"-LENSING:
ADVANTAGE ANDROMEDA! 478 3.5 CURRENT INTERPRETATION OF MICROLENSING
SURVEYS WITH RESPECT TO HALO DARK MATTER (AS OF 2004) 479 3.6
MICROLENSING TOWARD THE GALACTIC BULGE 484 4 MICROLENSING SURVEYS IN
SEARCH OF EXTRASOLAR PLANETS 486 4.1 HOW DOES THE MICROLENSING SEARCH
FOR EXTRASOLAR PLANET WORK? THE METHOD 486 CONTENTS XIII 4.2 WHY SEARCH
FOR EXTRASOLAR PLANETS WITH MICROLENSING? - ADVANTAGES AND DISADVANTAGES
488 4.3 WHO IS SEARCHING? THE TEAMS: OGLE, MOA, PLANET, MICROFUN 492 4.4
WHAT IS THE STATUS OF MICROLENSING PLANET SEARCHES SO FAR? THE RESULTS
493 4.5 WHEN WILL PLANETS BE DETECTED WITH MICROLENSING? THE PROSPECTS
496 4.6 NOTE ADDED IN APRIL 2004 (ABOUT ONE YEAR AFTER THE 33RD SAAS FEE
ADVANCED COURSE) 497 4.7 SUMMARY 497 5 HIGHER ORDER EFFECTS IN
MICROLENSING: 499 6 ASTROMETRIC MICROLENSING 516 7 QUASAR MICROLENSING
520 7.1 MICROLENSING MASS, LENGTH AND TIME SCALES 521 7.2 EARLY AND
RECENT THEORETICAL WORK ON QUASAR MICROLENSING. . . 524 7.3
OBSERVATIONAL EVIDENCE FOR QUASAR MICROLENSING 526 7.4 QUASAR
MICROLENSING: NOW AND FOREVER? 534 REFERENCES -. 536 INDE;C 541 |
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| any_adam_object_boolean | 1 |
| author_GND | (DE-588)121313336 (DE-588)115068163 |
| building | Verbundindex |
| bvnumber | BV021804687 |
| classification_rvk | UH 8700 |
| classification_tum | PHY 928f |
| ctrlnum | (OCoLC)181577228 (DE-599)BVBBV021804687 |
| dewey-full | 523.11 |
| dewey-hundreds | 500 - Natural sciences and mathematics |
| dewey-ones | 523 - Specific celestial bodies and phenomena |
| dewey-raw | 523.11 |
| dewey-search | 523.11 |
| dewey-sort | 3523.11 |
| dewey-tens | 520 - Astronomy and allied sciences |
| discipline | Physik Geographie |
| discipline_str_mv | Physik Geographie |
| edition | [Überarb. Ausg.] |
| format | Conference Proceeding Book |
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| genre | (DE-588)1071861417 Konferenzschrift 2003 Les Diablerets gnd-content |
| genre_facet | Konferenzschrift 2003 Les Diablerets |
| id | DE-604.BV021804687 |
| illustrated | Illustrated |
| index_date | 2024-07-02T15:48:57Z |
| indexdate | 2024-07-09T20:45:01Z |
| institution | BVB |
| institution_GND | (DE-588)10136711-9 |
| isbn | 9783540303091 354030309X |
| language | English |
| oai_aleph_id | oai:aleph.bib-bvb.de:BVB01-015017095 |
| oclc_num | 181577228 |
| open_access_boolean | |
| owner | DE-19 DE-BY-UBM DE-20 DE-91G DE-BY-TUM DE-11 |
| owner_facet | DE-19 DE-BY-UBM DE-20 DE-91G DE-BY-TUM DE-11 |
| physical | XIII, 552 S. Ill., graph. Darst. |
| publishDate | 2006 |
| publishDateSearch | 2006 |
| publishDateSort | 2006 |
| publisher | Springer |
| record_format | marc |
| spelling | Gravitational lensing: strong, weak and micro Saas Fee Advanced Course 33. P. Schneider ; C. Kochanek ; J. Wambsganss. Swiss Society for Astrophysics and Astronomy. Ed. by G. Meylan ... [Überarb. Ausg.] Berlin [u.a.] Springer 2006 XIII, 552 S. Ill., graph. Darst. txt rdacontent n rdamedia nc rdacarrier Literaturangaben Gravitationslinse (DE-588)4210687-4 gnd rswk-swf (DE-588)1071861417 Konferenzschrift 2003 Les Diablerets gnd-content Gravitationslinse (DE-588)4210687-4 s DE-604 Schneider, Peter 1958- Sonstige (DE-588)121313336 oth Meylan, Georges Sonstige (DE-588)115068163 oth Saas Fee Advanced Course 33 2003 Les Diablerets Sonstige (DE-588)10136711-9 oth GBV Datenaustausch application/pdf http://bvbr.bib-bvb.de:8991/F?func=service&doc_library=BVB01&local_base=BVB01&doc_number=015017095&sequence=000001&line_number=0001&func_code=DB_RECORDS&service_type=MEDIA Inhaltsverzeichnis |
| spellingShingle | Gravitational lensing: strong, weak and micro Gravitationslinse (DE-588)4210687-4 gnd |
| subject_GND | (DE-588)4210687-4 (DE-588)1071861417 |
| title | Gravitational lensing: strong, weak and micro |
| title_auth | Gravitational lensing: strong, weak and micro |
| title_exact_search | Gravitational lensing: strong, weak and micro |
| title_exact_search_txtP | Gravitational lensing: strong, weak and micro |
| title_full | Gravitational lensing: strong, weak and micro Saas Fee Advanced Course 33. P. Schneider ; C. Kochanek ; J. Wambsganss. Swiss Society for Astrophysics and Astronomy. Ed. by G. Meylan ... |
| title_fullStr | Gravitational lensing: strong, weak and micro Saas Fee Advanced Course 33. P. Schneider ; C. Kochanek ; J. Wambsganss. Swiss Society for Astrophysics and Astronomy. Ed. by G. Meylan ... |
| title_full_unstemmed | Gravitational lensing: strong, weak and micro Saas Fee Advanced Course 33. P. Schneider ; C. Kochanek ; J. Wambsganss. Swiss Society for Astrophysics and Astronomy. Ed. by G. Meylan ... |
| title_short | Gravitational lensing: strong, weak and micro |
| title_sort | gravitational lensing strong weak and micro |
| topic | Gravitationslinse (DE-588)4210687-4 gnd |
| topic_facet | Gravitationslinse Konferenzschrift 2003 Les Diablerets |
| url | http://bvbr.bib-bvb.de:8991/F?func=service&doc_library=BVB01&local_base=BVB01&doc_number=015017095&sequence=000001&line_number=0001&func_code=DB_RECORDS&service_type=MEDIA |
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