Publications, Ian Dell Antonio
|
|
- Shanon Thompson
- 6 years ago
- Views:
Transcription
1 Publications, Ian Dell Antonio Refereed Journal Articles: Schmidt, B.P., et al., 1993, The Unusual Supernova SN1993J in the galaxy M81, Nature, 364, 600 Dell Antonio, I.P., Geller, M.J., & Fabricant, D.G., 1994, X-Ray and Optical Properties of Groups of Galaxies, AJ, 107, 427 Rybicki, G.B., & Dell Antonio, I.P., 1994, Lyman-Alpha Trapping in Hydrogen During Recombination, ApJ, 427, 603 Dell Antonio, I.P., Geller, M.J., & Fabricant, D.G., 1995, Baryon Fractions for Poor Clusters, AJ, 110, 502 Dell Antonio, I.P., Bothun, G.D., & Geller, M.J., 1996, Peculiar Velocities for Galaxies in the Great Wall I. The Data, AJ, 112, 1759 Dell Antonio, I.P., Geller, M.J., & Bothun, G.D., 1996, Peculiar Velocities for Galaxies in the Great Wall II. Analysis, AJ, 112, 1780 Dell Antonio, I.P., & Tyson, J.A., 1996, Galaxy Dark Matter: Galaxy-Galaxy Lensing in the Hubble Deep Field, ApJL, 473, 17 Tyson, J.A., Kochanski, G.P., & Dell Antonio, I.P., 1998, Detailed Mass Map of CL from Strong Lensing, ApJL, 498, 107 Wittman, D.M., et al., 1998, Big Throughput Camera: the First Year, SPIE, 3355, 626 Riess, A.G., et al., 1999, BVRI Light Curves for 22 Type IA Supernovae, AJ, 117, 707 Wittman, D.M., et al., 2000, Detection of Weak Gravitational Lensing Distortions in Distant Galaxies by Cosmic Dark Matter at Large Scales, Nature, 405, 143 Wittman, D.M., et al., 2001, Discovery of a Galaxy Cluster via Weak Lensing, ApJL, 557, 89 Platais, I., et al., 2002, WIYN Open Cluster Study VIII: The Geometry and Stability of the NOAO CCD Mosaic Imager, AJ, 124, 601 Wittman, D., et al., 2003, Weak-Lensing Discovery and Tomography of a Cluster at z=0.68,
2 2 ApJ, 597, 218 Becker, A.C., et al., 2004, The Deep Lens Survey Transient Search. I. Short Timescale and Astrometric Variability, ApJ, 611, 418 Moretti, A., et al., 2004, The Brera Multi-scale Wavelet HRI Cluster Survey. I. Selection of the Sample and Number Counts, A&A, 428, 21 Dell Antonio, I.P., 2004, The State of Wide Field Surveys and their Contribution to the study of Cluster Peripheries, IAU Colloquium 195, A. Diaferio, editor, In press Kling, T.P., Dell Antonio, I.P., Wittman, D., Tyson, J.A., 2005, Wide-Field Weak Lensing by RXJ , ApJ, 625, 643 Geller, M.J., Dell Antonio, I.P., et al., 2005, SHELS: The Hectospec Lensing Survey, ApJL, 635, 125 Fabricant, D., et al., 2005, Hectospec, the MMT s 300 Optical Fiber-Fed Spectrograph, PASP, 117, 1411 Wittman, D., Dell Antonio, I., et al., 2006, First Results on Shear-Selected Clusters From the Deep Lens Survey: Optical Imaging, Spectroscopy, and X-Ray Followup, ApJ, accepted (astro-ph/050 Non-Refereed articles: Rybicki, G.B. & Dell Antonio, I.P., Spectral Distortions in the CMB from Recombination, 1994, In Observational Cosmology, AstronomicalSociety of the Pacific Conference Series, vol. 51, eds. G. Chincarini, A. Iovino, T. Maccacaro, and D. Maccagni, p San Francisco: Astronomical Society of the Pacific, Tyson, T., Kochanski, G., & Dell Antonio, I., Morphology of Gravitationally Lensed Galaxies, 1997, The Ultraviolet Universe at Low and High Redshift : Probing the Progress of Galaxy Evolution : College Park, MD May Edited by William H. Waller [et al.]. New York : American Institute of Physics, Also AIP Conference Proceedings, v.408., p.204 Windhorst, R.A., et al., The HST/WFPC2 B-Band Galaxy Counts vs. Type for 19 < B < 29 Mag, 1997, The Ultraviolet Universe at Low and High Redshift : Probing the Progress of Galaxy Evolution : College Park, MD May Edited by William H. Waller [et al.]. New York : American Institute of Physics, Also AIP Conference Proceedings, v.408., p.242 Dolan, C., Dell Antonio, I., Jannuzi, B., & Rhoads, J., GRB991216, Optical Observations,
3 3 1999, GCN 486, 1 Joyce, D., Rhoads, J, Ali, B., Dell Antonio, I., Jannuzi, B., GRB : j band spectrophotometry, GCN 501, 1 Wittman, D., Dell Antonio, I., et al., The Normal Cluster Weak Lensing Survey: Mass Profiles and M/L Ratios of Eight Clusters at z=0.2, 2000, In Constructing the Universe with Clusters of Galaxies. Edited by F. Durret & D. Gerbal. IAP 2000, Paris, p. 60. Tyson, J.A., et al., Mass Distribution in Normal Clusters, 2001, in Gravitational Lensing: Recent Progress and Future Prospects, ASP Conference Proceedings Vol 237. Edited by T. Brainerd & C. Kochanek. San Francisco: Astronomical Society of the Pacific, p Moretti, A., et al., The BMW Deep X-Ray Cluster Survey, 2001, in X-ray Astronomy 2000, ASP Conference Proceeding Vol. 234, Edited by Riccardo Giacconi, Salvatore Serio and Luigi Stella, San Francisco: Astronomical Society of the Pacific, p 393 Guzzo, L., et al., The BMW Deep X-Ray Cluster Survey, 2001, in Deep Fields, Proceedings of the ESO/ECF/STScI Workshop held at Garching, Germany, 9-12 October Stefano Cristiani, Alvio Renzini, Robert E. Williams (eds.). Springer, 2001, p. 207 Longhetti, M., et al., The BMW Deep X-Ray Cluster Survey, 2002, in Tracing Cosmic Evolution with Galaxy Clusters. ASP Conference Proceedings, Vol Edited by Stefano Borgani, Marino Mezzetti, and Riccardo Valdarnini. ISBN: San Francisco, Astronomical Society of the Pacific, 2002., p.399 Levan, A., et al., GRB : Possible IR counterpart, 2003, GCN 1818, 1 Wasserman, L.H., et al. Minor Planet Observations, 2003, MPC 48899, 7 Hughes, J.P., Dell Antonio, I., et al. The Chandra First Year Survey of DLS Shear-Selected Galaxy Clusters, 2004, HEAD Hughes, J.P., Dell Antonio, I., et al. X-Rays from the Most Massive DLS Shear-Selected Galaxy Clusters, 2004, 35th COSPAR Scientific Assembly, Paris, p Wang, Y., et al., Joint Efficient Dark-energy Investigation (JEDI): a Candidate Implementation of the NASA-DOE Joint Dark Energy Mission (JDEM), 2005, JEDI white paper for the Dark Energy Task Force, astro-ph/ Abstracts:
4 4 Partridge, R.B., Dell Antonio, I., & Sheth, R., 1989, AAS, Dell Antonio, I.P., Geller, M.J., & Fabricant, D., 1992, AAS, Rybicki, G.B., & Dell Antonio, I.P., 1996, AAS, Dell Antonio, I.P., Kochanski, G.P., & Tyson, J.A., 1996, AAS, Kochanski, G.P., Dell Antonio, I.P., & Tyson, J.A., 1996, AAS, Cohen, S.H., et al., 1997, AAS, Dell Antonio, I.P., 1997, AAS, Kochanski, G.P., Dell Antonio, I.P, & Tyson, J.A., 1997, AAS, Dell Antonio, I.P, et al., 1998, AAS, Tyson, J.A., et al., 1999, AAS, Kozhurina-Platais et al., 2000, AAS, Groch, H., et al., 2000, AAS, Dell Antonio, I., et al., 2001, AAS, Becker, A., et al., 2001, AAS, Tyson, J.A., et al., 2001, AAS, Hennawi, J.F., et al., 2001, AAS, Kubo, J.M., & Dell Antonio, I.P., 2004, AAS, Wittman, D., Dell Antonio, I., et al., 2004, AAS, Wang, Y., et al.., 2005, AAS, Kubo, J.M., & Dell Antonio, I.P., 2005, AAS, Khiabanian, H., & Dell Antonio, I.P., 2005, AAS,
5 5
Astro 101 Slide Set: Multiple Views of an Extremely Distant Galaxy
Astro 101 Slide Set: Multiple Views of an Extremely Distant Galaxy A Discovery from the Hubble Frontier Fields Program Topic: Distant galaxies Concepts: Galaxy development, Gravitational lensing Missions:
More informationCosmology The Road Map
Cosmology The Road Map Peter Schneider Institut für Astrophysik, Bonn University on behalf of the Astronomy Working Group Cosmology s Themes Fundamental Cosmology Probing inflation Investigating Dark Energy
More informationObservational Cosmology
(C. Porciani / K. Basu) Lecture 7 Cosmology with galaxy clusters (Mass function, clusters surveys) Course website: http://www.astro.uni-bonn.de/~kbasu/astro845.html Outline of the two lecture Galaxy clusters
More informationCosmology with Wide Field Astronomy
M. Moniez To cite this version: M. Moniez.. 35th International Conference on High Energy Physics (ICHEP2010), Jul 2010, Paris, France. Proceedings of Science, 441 (4 p.), 2010. HAL Id:
More informationAge-redshift relation. The time since the big bang depends on the cosmological parameters.
Age-redshift relation The time since the big bang depends on the cosmological parameters. Lyman Break Galaxies High redshift galaxies are red or absent in blue filters because of attenuation from the neutral
More informationDark Matter & Dark Energy. Astronomy 1101
Dark Matter & Dark Energy Astronomy 1101 Key Ideas: Dark Matter Matter we cannot see directly with light Detected only by its gravity (possible future direct detection in the lab) Most of the matter in
More informationOutline. Cosmological parameters II. Deceleration parameter I. A few others. Covers chapter 6 in Ryden
Outline Covers chapter 6 in Ryden Cosmological parameters I The most important ones in this course: M : Matter R : Radiation or DE : Cosmological constant or dark energy tot (or just ): Sum of the other
More informationarxiv: v1 [astro-ph.co] 15 Nov 2010
Highlights of Spanish Astrophysics VI, Proceedings of the IX Scientific Meeting of the Spanish Astronomical Society held on September 13-17, 2010, in Madrid, Spain. M. R. Zapatero Osorio et al. (eds.)
More information3/6/12! Astro 358/Spring 2012! Galaxies and the Universe! Dark Matter in Spiral Galaxies. Dark Matter in Galaxies!
3/6/12 Astro 358/Spring 2012 Galaxies and the Universe Dark Matter in Galaxies Figures + Tables for Lectures (Feb 16-Mar 6) Dark Matter in Spiral Galaxies Flat rotation curve of Milky Way at large radii
More informationWeak Gravitational Lensing
Weak Gravitational Lensing Sofia Sivertsson October 2006 1 General properties of weak lensing. Gravitational lensing is due to the fact that light bends in a gravitational field, in the same fashion as
More informationDark Energy. Cluster counts, weak lensing & Supernovae Ia all in one survey. Survey (DES)
Dark Energy Cluster counts, weak lensing & Supernovae Ia all in one survey Survey (DES) What is it? The DES Collaboration will build and use a wide field optical imager (DECam) to perform a wide area,
More informationGravitational Lensing: Strong, Weak and Micro
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
More informationUnderstanding the Properties of Dark Energy in the Universe p.1/37
Understanding the Properties of Dark Energy in the Universe Dragan Huterer Case Western Reserve University Understanding the Properties of Dark Energy in the Universe p.1/37 The Cosmic Food Pyramid?? Radiation
More informationA Search for High Redshift Galaxies behind Gravitationally Lensing Clusters
A Search for High Redshift Galaxies behind Gravitationally Lensing Clusters Ota et al.2011 submitted to Monthly Notices of the Royal Astronomical Society Kazuaki Ota (Kyoto U) Johan Richard (Obs.Lyon),
More informationCosmology. Introduction Geometry and expansion history (Cosmic Background Radiation) Growth Secondary anisotropies Large Scale Structure
Cosmology Introduction Geometry and expansion history (Cosmic Background Radiation) Growth Secondary anisotropies Large Scale Structure Cosmology from Large Scale Structure Sky Surveys Supernovae Ia CMB
More informationBrief Introduction to Cosmology
Brief Introduction to Cosmology Matias Zaldarriaga Harvard University August 2006 Basic Questions in Cosmology: How does the Universe evolve? What is the universe made off? How is matter distributed? How
More informationExploring the Depths of the Universe
Exploring the Depths of the Universe Jennifer Lotz Hubble Science Briefing Jan. 16, 2014 Hubble is now observing galaxies 97% of the way back to the Big Bang, during the first 500 million years 2 Challenge:
More informationLecture Outlines. Chapter 25. Astronomy Today 7th Edition Chaisson/McMillan Pearson Education, Inc.
Lecture Outlines Chapter 25 Astronomy Today 7th Edition Chaisson/McMillan Chapter 25 Galaxies and Dark Matter Units of Chapter 25 25.1 Dark Matter in the Universe 25.2 Galaxy Collisions 25.3 Galaxy Formation
More informationAstronomy. Catherine Turon. for the Astronomy Working Group
Astronomy Catherine Turon for the Astronomy Working Group Answers to the call for ideas Illustration of the strong expectation of the community from the ESA Science Programme: In astronomy 1983: Horizon
More information2. OBSERVATIONAL COSMOLOGY
2. OBSERVATIONAL COSMOLOGY 1. OBSERVATIONAL PARAMETERS i. Introduction History of modern observational Cosmology ii. Cosmological Parameters The search for 2 (or more) numbers Hubble Parameter Deceleration
More informationGalaxy Formation/Evolution and Cosmic Reionization Probed with Multi-wavelength Observations of Distant Galaxies. Kazuaki Ota
Galaxy Formation/Evolution and Cosmic Reionization Probed with Multi-wavelength Observations of Distant Galaxies Kazuaki Ota Department of Astronomy Kyoto University 2013 Feb. 14 GCOE Symposium Outline
More informationScience with the New Hubble Instruments. Ken Sembach STScI Hubble Project Scientist
Science with the New Hubble Instruments Ken Sembach STScI Hubble Project Scientist 1 Hubble Has Improved Over Time Servicing missions have improved Hubble s vision. Hubble sees farther and with greater
More informationReally, what universe do we live in? White dwarfs Supernova type Ia Accelerating universe Cosmic shear Lyman α forest
Really, what universe do we live in? White dwarfs Supernova type Ia Accelerating universe Cosmic shear Lyman α forest White dwarf Core of solar mass star No energy from fusion or gravitational contraction
More informationDISTANCES ON COSMOLOGICAL SCALES WITH VLTI. 1. Introduction
DISTANCES ON COSMOLOGICAL SCALES WITH VLTI MARGARITA KAROVSKA, MARTIN ELVIS and MASSIMO MARENGO Harvard-Smithsonian Center for Astrophysics Abstract. We present here a new method using interferometric
More informationDark Matter. Galaxy Counts Redshift Surveys Galaxy Rotation Curves Cluster Dynamics Gravitational Lenses ~ 0.3 Ω M Ω b.
Dark Matter Galaxy Counts Redshift Surveys Galaxy Rotation Curves Cluster Dynamics Gravitational Lenses Ω M ~ 0.3 2 1 Ω b 0.04 3 Mass Density by Direct Counting Add up the mass of all the galaxies per
More informationReview of Lecture 15 3/17/10. Lecture 15: Dark Matter and the Cosmic Web (plus Gamma Ray Bursts) Prof. Tom Megeath
Lecture 15: Dark Matter and the Cosmic Web (plus Gamma Ray Bursts) Prof. Tom Megeath A2020 Disk Component: stars of all ages, many gas clouds Review of Lecture 15 Spheroidal Component: bulge & halo, old
More informationDiscovery of Primeval Large-Scale Structures with Forming Clusters at Redshift z=5.7
Discovery of Primeval Large-Scale Structures with Forming Clusters at Redshift z=5.7 Sadanori Okamura Department of Astronomy, and Research Center for the Early Universe, University of Tokyo Collaborators
More informationWindows to the Past: Using Gravitational Telescopes to Study our Cosmic Origins
Windows to the Past: Using Gravitational Telescopes to Study our Cosmic Origins Austin Hoag University of California, Davis July 15, 2016 1 / 21 Collaborators Maru sa Brada c (PhD advisor; UCD), Tommaso
More informationFrom the VLT to ALMA and to the E-ELT
From the VLT to ALMA and to the E-ELT Mission Develop and operate world-class observing facilities for astronomical research Organize collaborations in astronomy Intergovernmental treaty-level organization
More informationClusters of Galaxies " High Energy Objects - most of the baryons are in a hot (kt~ k) gas." The x-ray luminosity is ergs/sec"
Clusters of Galaxies! Ch 4 Longair Clusters of galaxies are the largest gravitationally bound systems in the Universe. At optical wavelengths they appear as over-densities of galaxies with respect to the
More informationObservational Cosmology
Astr 102: Introduction to Astronomy Fall Quarter 2009, University of Washington, Željko Ivezić Lecture 15: Observational Cosmology 1 Outline Observational Cosmology: observations that allow us to test
More informationAPLUS: A Data Reduction Pipeline for HST/ACS and WFC3 Images
APLUS: A Data Reduction Pipeline for HST/ACS and WFC3 Images Wei Zheng 1,AmitSaraff 2,3,LarryBradley 4,DanCoe 4,AlexViana 4 and Sara Ogaz 4 1 Department of Physics and Astronomy, Johns Hopkins University,
More informationReally, really, what universe do we live in?
Really, really, what universe do we live in? Fluctuations in cosmic microwave background Origin Amplitude Spectrum Cosmic variance CMB observations and cosmological parameters COBE, balloons WMAP Parameters
More informationGalaxy formation and evolution. Astro 850
Galaxy formation and evolution Astro 850 Introduction What are galaxies? Systems containing many galaxies, e.g. 10 11 stars in the Milky Way. But galaxies have different properties. Properties of individual
More informationIntroduction to SDSS -instruments, survey strategy, etc
Introduction to SDSS -instruments, survey strategy, etc (materials from http://www.sdss.org/) Shan Huang 17 February 2010 Survey type Status Imaging and Spectroscopy Basic Facts SDSS-II completed, SDSS-III
More informationProbing the evolution of massive galaxies with the K20 survey
Probing the evolution of massive galaxies with the K20 survey Andrea Cimatti Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, I-50125, Firenze, Italy Abstract. The motivations and the status of the
More informationLarge-Scale Structure
Large-Scale Structure Evidence for Dark Matter Dark Halos in Ellipticals Hot Gas in Ellipticals Clusters Hot Gas in Clusters Cluster Galaxy Velocities and Masses Large-Scale Distribution of Galaxies 1
More informationarxiv:astro-ph/ v1 3 Jan 2001
The VIRMOS-VLT Deep Survey arxiv:astro-ph/0101034v1 3 Jan 2001 O. Le Fèvre 1, G. Vettolani 2, D. Maccagni 3, D. Mancini 4, A. Mazure 1, Y. Mellier 5, J.P. Picat 6, M. Arnaboldi 4, S. Bardelli 9, E. Bertin
More informationEarly Optical Afterglows of GRBs with 2-m Robotic Telescopes
Early Optical Afterglows of GRBs with 2-m Robotic Telescopes Andreja Gomboc Faculty of Mathematics and Physics University of Ljubljana on behalf of a larger collaboration led by: ARI, Liverpool John Moores
More informationEUCLID Spectroscopy. Andrea Cimatti. & the EUCLID-NIS Team. University of Bologna Department of Astronomy
EUCLID Spectroscopy Andrea Cimatti University of Bologna Department of Astronomy & the EUCLID-NIS Team Observing the Dark Universe with EUCLID, ESA ESTEC, 17 November 2009 DARK Universe (73% Dark Energy
More informationType II Supernovae as Standardized Candles
Type II Supernovae as Standardized Candles Mario Hamuy 1 2 Steward Observatory, The University of Arizona, Tucson, AZ 85721 Philip A. Pinto Steward Observatory, The University of Arizona, Tucson, AZ 85721
More informationThe First Galaxies: Evolution drivers via luminosity functions and spectroscopy through a magnifying GLASS
Charlotte Mason (UCLA) Aspen, 7 Feb 2016 The First Galaxies: Evolution drivers via luminosity functions and spectroscopy through a magnifying GLASS with Tommaso Treu (UCLA), Michele Trenti (U. Melbourne),
More informationThe Large Synoptic Survey Telescope
The Large Synoptic Survey Telescope Philip A. Pinto Steward Observatory University of Arizona for the LSST Collaboration 17 May, 2006 NRAO, Socorro Large Synoptic Survey Telescope The need for a facility
More informationThe Universe: What We Know and What we Don t. Fundamental Physics Cosmology Elementary Particle Physics
The Universe: What We Know and What we Don t Fundamental Physics Cosmology Elementary Particle Physics 1 Cosmology Study of the universe at the largest scale How big is the universe? Where What Are did
More informationDiscovery of eight lensing clusters of galaxies
. Article. SCIENCE CHINA Physics, Mechanics & Astronomy September 2014 Vol. 57 No. 9: 1809 1815 doi: 10.1007/s11433-014-5544-8 Discovery of eight lensing clusters of galaxies LIANG SuMing 1,2, WEN ZhongLue
More informationToday. Lookback time. ASTR 1020: Stars & Galaxies. Astronomy Picture of the day. April 2, 2008
ASTR 1020: Stars & Galaxies April 2, 2008 Astronomy Picture of the day Reading: Chapter 21, sections 21.3. MasteringAstronomy Homework on Galaxies and Hubble s Law is due April 7 th. Weak Lensing Distorts
More informationLecture 37 Cosmology [not on exam] January 16b, 2014
1 Lecture 37 Cosmology [not on exam] January 16b, 2014 2 Structure of the Universe Does clustering of galaxies go on forever? Looked at very narrow regions of space to far distances. On large scales the
More informationThe Mystery of Dark Matter
The Mystery of Dark Matter Maxim Perelstein, LEPP/Cornell U. CIPT Fall Workshop, Ithaca NY, September 28 2013 Introduction Last Fall workshop focused on physics of the very small - elementary particles
More informationMoment of beginning of space-time about 13.7 billion years ago. The time at which all the material and energy in the expanding Universe was coincident
Big Bang Moment of beginning of space-time about 13.7 billion years ago The time at which all the material and energy in the expanding Universe was coincident Only moment in the history of the Universe
More informationThe Multiplicity Function of groups of galaxies from CRoNaRio catalogues
The Multiplicity Function of groups of galaxies from CRoNaRio catalogues E. DE FILIPPIS 1,G.LONGO 2, S. ANDREON 2, R. SCARAMELLA 3,TESTAV. 3,R.DE CARVALHO 4,G.DJORGOVSKI 5 1 Università Federico II, Naples,
More informationInflation - a solution to the uniformity problem. include more dark matter. count up all mass in galaxies include massive dark galaxy halos
Reading: Chapter 29, Section 29.5-29.6; Chapter 30 (next week) Final Exam: Tuesday, May 1 12:00-2:00; review/practice materials posted soon COURSE EVALUATIONS - please complete these online (recitation
More informationModern Cosmology / Scott Dodelson Contents
Modern Cosmology / Scott Dodelson Contents The Standard Model and Beyond p. 1 The Expanding Universe p. 1 The Hubble Diagram p. 7 Big Bang Nucleosynthesis p. 9 The Cosmic Microwave Background p. 13 Beyond
More informationarxiv:astro-ph/ v3 3 May 2000
arxiv:astro-ph/0003014v3 3 May 2000 Detection of weak gravitational lening distortions of distant galaxies by cosmic dark matter at large scales David M. Wittman, J. Anthony Tyson, David Kirkman, Ian Dell
More informationCosmology Distinction Course
2006 HIGHER SCHOOL CERTIFICATE EXAMINATION Cosmology Distinction Course Modules 1, 2 and 3 (including Residential 1) Total marks 60 Section I Page 2 General Instructions Reading time 5 minutes Working
More informationToday: Start Ch. 18: Cosmology. Homework # 5 due next Wed. (HW #6 is online)
Today: Start Ch. 18: Cosmology Homework # 5 due next Wed. (HW #6 is online) Dark Matter! A rotation curve is a graph of how fast a something is rotating, as a function of distance from the center.! We
More informationMapping the Dark Energy Equation of State
**TITLE** ASP Conference Series, Vol. **VOLUME***, **YEAR OF PUBLICATION** **NAMES OF EDITORS** Mapping the Dark Energy Equation of State Eric V. Linder Berkeley Lab, 1 Cyclotron Road, M/S 50R5008, Berkeley,
More informationCosmology with the ESA Euclid Mission
Cosmology with the ESA Euclid Mission Andrea Cimatti Università di Bologna Dipartimento di Astronomia On behalf of the Euclid Italy Team ESA Cosmic Vision 2015-2025 M-class Mission Candidate Selected in
More informationInfrared Mass-to-Light Profile Throughout the Infall Region of the Coma Cluster
Infrared Mass-to-Light Profile Throughout the Infall Region of the Coma Cluster K. Rines 1, M.J. Geller 2, M.J. Kurtz 1, A. Diaferio 3, T.H. Jarrett 4, and J.P. Huchra 1 ABSTRACT Using a redshift survey
More informationAstronomy 330 Lecture Dec 2010
Astronomy 330 Lecture 26 10 Dec 2010 Outline Clusters Evolution of cluster populations The state of HI sensitivity Large Scale Structure Cluster Evolution Why might we expect it? What does density determine?
More informationDark Energy: Measuring the Invisible with X-Ray Telescopes
Black holes, Galactic Dark Center Matter and Galactic Center Dark Energy: Measuring the Invisible with X-Ray Telescopes Christine Jones Before 1930 -- only optical observations of the sky Intro Before
More informationChapter 23 Lecture. The Cosmic Perspective Seventh Edition. Dark Matter, Dark Energy, and the Fate of the Universe Pearson Education, Inc.
Chapter 23 Lecture The Cosmic Perspective Seventh Edition Dark Matter, Dark Energy, and the Fate of the Universe Curvature of the Universe The Density Parameter of the Universe Ω 0 is defined as the ratio
More informationWhat are the Contents of the Universe? Taking an Inventory of the Baryonic and Dark Matter Content of the Universe
What are the Contents of the Universe? Taking an Inventory of the Baryonic and Dark Matter Content of the Universe Layout of the Course Sept 4: Introduction / Overview / General Concepts Sept 11: No Class
More informationX-ray Cluster Cosmology
X-ray Cluster Cosmology A white paper submitted to the Decadal Survey Committee Authors: A. Vikhlinin 1, S. Murray 1, R. Gilli 2, P. Tozzi 3, M. Paolillo 4, N. Brandt 8, G. Tagliaferri 9, M. Bautz 12,
More informationThe shapes of faint galaxies: A window unto mass in the universe
Lecture 15 The shapes of faint galaxies: A window unto mass in the universe Intensity weighted second moments Optimal filtering Weak gravitational lensing Shear components Shear detection Inverse problem:
More informationDark Energy in Light of the CMB. (or why H 0 is the Dark Energy) Wayne Hu. February 2006, NRAO, VA
Dark Energy in Light of the CMB (or why H 0 is the Dark Energy) Wayne Hu February 2006, NRAO, VA If its not dark, it doesn't matter! Cosmic matter-energy budget: Dark Energy Dark Matter Dark Baryons Visible
More informationAstronomy 422. Lecture 15: Expansion and Large Scale Structure of the Universe
Astronomy 422 Lecture 15: Expansion and Large Scale Structure of the Universe Key concepts: Hubble Flow Clusters and Large scale structure Gravitational Lensing Sunyaev-Zeldovich Effect Expansion and age
More informationUsing Gamma Ray Bursts to Estimate Luminosity Distances. Shanel Deal
Using Gamma Ray Bursts to Estimate Luminosity Distances Shanel Deal University of Notre Dame Summer Research Experience for Undergraduate 2013 Program Dr. Peter Garnavich August 2, 2013 Abstract Gamma
More informationarxiv:astro-ph/ v1 20 Feb 2004
Discovery of Face-On Counterparts of Chain Galaxies in the Tadpole ACS Field arxiv:astro-ph/42477v1 Feb 4 Debra Meloy Elmegreen Vassar College, Dept. of Physics & Astronomy, Box 745, Poughkeepsie, NY 1264;
More informationThe Future of Cosmology
The Future of Cosmology Ay21, March 10, 2010 Announcements: final exams available beginning 9am on March 12 (Friday), from Swarnima (note that the final will not be distributed electronically). finals
More informationSVOM in the multi-messenger area
CEA-Irfu, Saclay IAP, Paris APC, Paris CNES, Toulouse NAOC, Beijing XIOPM, Xi an IHEP, Beijing SECM, Shanghai IRAP, Toulouse LAM, Marseille CPPM, Marseille GEPI, Meudon LAL, Orsay LUPM, Montpellier University
More informationGalactic Neighborhood and (Chandra-enabled) X-ray Astrophysics
Galactic Neighborhood and (Chandra-enabled) X-ray Astrophysics Q. Daniel Wang (University of Massachusetts) Frontier Science Galactic Neighborhood Panel Members: Leo Blitz, Julianne Dalcanton, Bruce Draine,
More informationThe phenomenon of gravitational lenses
The phenomenon of gravitational lenses The phenomenon of gravitational lenses If we look carefully at the image taken with the Hubble Space Telescope, of the Galaxy Cluster Abell 2218 in the constellation
More informationThe King's University College Astronomy 201 Mid-Term Exam Solutions
The King's University College Astronomy 201 Mid-Term Exam Solutions Instructions: The exam consists of two sections. Part A is 20 multiple choice questions - please record answers on the sheet provided.
More informationChapter 23 Lecture. The Cosmic Perspective Seventh Edition. Dark Matter, Dark Energy, and the Fate of the Universe Pearson Education, Inc.
Chapter 23 Lecture The Cosmic Perspective Seventh Edition Dark Matter, Dark Energy, and the Fate of the Universe Curvature of the Universe The Density Parameter of the Universe Ω 0 is defined as the ratio
More informationDark Matter -- Astrophysical Evidences and Terrestrial Searches
SFB 443 Bosen workshop 2010 Dark Matter -- Astrophysical Evidences and Terrestrial Searches Klaus Eitel, Karlsruhe Institute of Technology, KCETA, IK KIT University of the State of Baden-Württemberg and
More informationEvidence for/constraints on dark matter in galaxies and clusters
Nov 11, 2015 Evidence for/constraints on dark matter in galaxies and clusters HW#9 is due; please hand in your summaries; then you get to talk (I have slides of the different facilities/telescopes. HW#10
More informationChapter 1 Introduction. Particle Astrophysics & Cosmology SS
Chapter 1 Introduction Particle Astrophysics & Cosmology SS 2008 1 Ptolemäus (85 165 b.c.) Kopernicus (1473 1543) Kepler (1571 1630) Newton (1643 1727) Kant (1724 1630) Herschel (1738 1822) Einstein (1917)
More informationStellar Mass Estimates of Galaxies in Superclusters at z~1
Stellar Mass Estimates of Galaxies in Superclusters at z~1 Catherine Whiting The University of Iowa Advisor: Dr. Roy Gal Institute for Astronomy, University of Hawai i at Manoa Abstract. A simple method
More informationThe Expanding Universe
Cosmology Expanding Universe History of the Universe Cosmic Background Radiation The Cosmological Principle Cosmology and General Relativity Dark Matter and Dark Energy Primitive Cosmology If the universe
More informationPhysics 661. Particle Physics Phenomenology. October 2, Physics 661, lecture 2
Physics 661 Particle Physics Phenomenology October 2, 2003 Evidence for theory: Hot Big Bang Model Present expansion of the Universe Existence of cosmic microwave background radiation Relative abundance
More informationFURTHER COSMOLOGY Book page T H E M A K E U P O F T H E U N I V E R S E
FURTHER COSMOLOGY Book page 675-683 T H E M A K E U P O F T H E U N I V E R S E COSMOLOGICAL PRINCIPLE Is the Universe isotropic or homogeneous? There is no place in the Universe that would be considered
More informationIsotropy and Homogeneity
Cosmic inventory Isotropy and Homogeneity On large scales the Universe is isotropic (looks the same in all directions) and homogeneity (the same average density at all locations. This is determined from
More informationWhy Use a Telescope?
1 Why Use a Telescope? All astronomical objects are distant so a telescope is needed to Gather light -- telescopes sometimes referred to as light buckets Resolve detail Magnify an image (least important
More informationSHEAR-SELECTED CLUSTERS FROM THE DEEP LENS SURVEY
SHEAR-SELECTED CLUSTERS FROM THE DEEP LENS SURVEY David Wittman Bell Labs, Lucent Technologies 700 Mountain Avenue, Murray Hill, NJ 07974 Representing the DLS Collaboration ABSTRACT The Deep Lens Survey
More informationAstro 406 Lecture 25 Oct. 25, 2013
Astro 406 Lecture 25 Oct. 25, 2013 Announcements: PS 7 due now PS 8 due next Friday ASTR 401: draft due next Monday thanks to the Planetarium-goers alternate makeup activity posted soon Next semester:
More informationBrief update (3 mins/2 slides) on astrophysics behind final project
Nov 1, 2017 Brief update (3 mins/2 slides) on astrophysics behind final project Evidence for Dark Matter Next Wed: Prelim #2, similar to last one (30 mins). Review especially lecture slides, PEs and non-project
More informationEvidence for Supernova Light in all Gamma-Ray Burst Afterglow
Clemson University TigerPrints Publications Physics and Astronomy Winter 12-13-2004 Evidence for Supernova Light in all Gamma-Ray Burst Afterglow A. Zeh Thüringer Landessternwarte Tautenburg S. Klose Thüringer
More informationOutline: Galaxy groups & clusters
Outline: Galaxy groups & clusters Outline: Gravitational lensing Galaxy groups and clusters I Galaxy groups and clusters II Cluster classification Increasing rareness Intermission: What are you looking
More informationDark Matter. Jaan Einasto Tartu Observatory and ICRANet 16 December Saturday, December 15, 12
Dark Matter Jaan Einasto Tartu Observatory and ICRANet 16 December 2012 Local Dark Matter: invisible matter in the Galaxy in Solar vicinity Global Dark Matter: invisible matter surrounding galaxies Global
More informationNew techniques to measure the velocity field in Universe.
New techniques to measure the velocity field in Universe. Suman Bhattacharya. Los Alamos National Laboratory Collaborators: Arthur Kosowsky, Andrew Zentner, Jeff Newman (University of Pittsburgh) Constituents
More informationThe Evolution of the Cosmic SN Rate
The Evolution of the Cosmic SN Rate Massimo Della Valle Arcetri Astrophysical Observatory 1 Science cases (for OWL) Evolution of cosmological parameters Large scale structure Galaxy formation (Dark?) matter
More informationExploring Dark Matter through Gravitational Lensing. Exploring the Dark Universe Indiana University June 2007
Exploring Dark Matter through Gravitational Lensing Exploring the Dark Universe Indiana University 28-29 June 2007 What is a Gravitational Lens? A gravitational lens is formed when the light from a distant,
More informationIntroducing DENET, HSC, & WFMOS
RESCEU & JSPS core-tocore program DENET Summer School Dark energy in the universe September 1-4, 2007 Introducing DENET, HSC, & WFMOS Yasushi Suto Department of Physics, The University of Tokyo 1 International
More informationAbsolute Neutrino Mass from Cosmology. Manoj Kaplinghat UC Davis
Absolute Neutrino Mass from Cosmology Manoj Kaplinghat UC Davis Kinematic Constraints on Neutrino Mass Tritium decay (Mainz Collaboration, Bloom et al, Nucl. Phys. B91, 273, 2001) p and t decay Future
More informationAST1100 Lecture Notes
AST1100 Lecture Notes 4 Stellar orbits and dark matter 1 Using Kepler s laws for stars orbiting the center of a galaxy We will now use Kepler s laws of gravitation on much larger scales. We will study
More information5 February 2004 MEMORANDUM. To: Dan Fabricant From: Scott Kenyon Subject: Time Allocation at FLWO and the MMT
5 February 4 MEMORANDUM To: Dan Fabricant From: Scott Kenyon Subject: Time Allocation at FLWO and the MMT In the 25 years since the dedication of the MMT, CfA optical ground-based telescopes have been
More informationThe Hunt for Dark Energy
The Hunt for Dark Energy Peter Garnavich University of Notre Dame as imagination bodies forth astronomer s The forms of things unknown, the poet's pen Turns them to shapes and gives to airy nothing A local
More informationROSAT Roentgen Satellite. Chandra X-ray Observatory
ROSAT Roentgen Satellite Joint facility: US, Germany, UK Operated 1990 1999 All-sky survey + pointed observations Chandra X-ray Observatory US Mission Operating 1999 present Pointed observations How do
More informationHow do telescopes "see" on Earth and in space?
How do telescopes "see" on Earth and in space? By NASA, adapted by Newsela staff on 03.28.17 Word Count 933 Level 970L TOP IMAGE: The Hubble Space Telescope orbiting in space over Earth. SECOND IMAGE:
More informationAstro Assignment 1 on course web page (due 15 Feb) Instructors: Jim Cordes & Shami Chatterjee
Astro 2299 The Search for Life in the Universe Lecture 4 This time: Redshifts and the Hubble Law Hubble law and the expanding universe The cosmic microwave background (CMB) The elements and the periodic
More information