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Large-scale structure of the cosmos
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261	Mon. Not. R. Astron. Soc. 000, 1–17 (XXXX) Printed 22 August[removed]MN LATEX style file v2.2) Add to Reading List Source URL: www.spacetelescope.org Language: English - Date: 2012-10-15 10:45:10 Large-scale structure of the cosmos Gravitational lensing Weak gravitational lensing Galaxy clusters Gravitational lens Redshift Dark matter Galaxy groups and clusters Strong gravitational lensing Physics Astronomy Physical cosmology
262	Hindawi Publishing Corporation Advances in Astronomy Volume 2011, Article ID[removed], 17 pages doi:[removed][removed]Review Article Add to Reading List Source URL: www.kiss.caltech.edu Language: English - Date: 2014-05-14 13:48:59 Large-scale structure of the cosmos Dark matter Galaxies Galactic astronomy Cold dark matter Galaxy rotation curve Structure formation Spiral galaxy Lambda-CDM model Physics Astronomy Physical cosmology
263	New Forms of Convection in Galaxy Cluster Plasmas (i.e., how do galaxy clusters boil?) Eliot Quataert (UC Berkeley) Hydra A w/ Chandra Add to Reading List Source URL: astro.berkeley.edu Language: English - Date: 2009-01-09 15:25:02 Physical quantities Thermodynamics Heat conduction Galaxy groups and clusters Plasma Galaxy cluster Thermal conduction Star Temperature Physics Heat transfer Large-scale structure of the cosmos
264	HOW DO GALAXIES FORM AND EVOLVE? GALAXIES, GALAXIES EVERYWHERE The Hubble Ultra Deep Field is one of the most important Add to Reading List Source URL: www.cosmiccollisions.org Language: English - Date: 2009-10-21 11:15:59 Galaxies Physical cosmology Large-scale structure of the cosmos Elliptical galaxy Extragalactic astronomy Hubble Deep Field Supercluster Galaxy formation and evolution Brightest cluster galaxy Astronomy Physics Space
265	Mon. Not. R. Astron. Soc. 000, 1–[removed]Printed 13 January[removed]MN LATEX style file v2.2) Add to Reading List Source URL: www.kiss.caltech.edu Language: English - Date: 2014-05-15 12:20:32 Large-scale structure of the cosmos Galaxy clusters Particle physics Dark matter Bullet Cluster MACS J0025.4-1222 Lambda-CDM model Cold dark matter Galaxy groups and clusters Physics Astronomy Physical cosmology
266	PDF Document Add to Reading List Source URL: www.kiss.caltech.edu Language: English - Date: 2014-05-14 13:48:57 Dark matter Physical cosmology Astrophysics Large-scale structure of the cosmos Local Group Cold dark matter Galaxy formation and evolution Navarro–Frenk–White profile Modified Newtonian dynamics Physics Astronomy Extragalactic astronomy
267	Observing the Universe from the Classroom Add to Reading List Source URL: www.spacetelescope.org Language: English - Date: 2007-01-05 11:44:24 Gravitational lensing Astrophysics Hubble Space Telescope Large-scale structure of the cosmos Dark matter Weak gravitational lensing Gravitational lens Galaxy formation and evolution Galaxy Physics Astronomy Physical cosmology
268	CLASH: A2261 HST Strong Lensing Analysis Add to Reading List Source URL: www.kiss.caltech.edu Language: English - Date: 2014-05-14 13:48:57 Large-scale structure of the cosmos Gravitational lensing Galaxies Weak gravitational lensing Galaxy clusters Redshift Gravitational lens Galaxy groups and clusters Photometric redshift Physics Astronomy Physical cosmology
269	PDF Document Add to Reading List Source URL: www.princetonastronomy.org Language: English - Date: 2003-04-27 10:42:25 Theories of gravitation Physical cosmology Celestial mechanics Large-scale structure of the cosmos Modified Newtonian dynamics Dark matter Gravitation Mordehai Milgrom Galaxy formation and evolution Physics Astronomy Astrophysics
270	ASTRONOMY BEAT Number 33 • October 5, 2009 Publisher: Astronomical Society of the Pacific Editor: Andrew Fraknoi Designer: Leslie Proudfit Add to Reading List Source URL: astrosociety.org Language: English - Date: 2014-05-22 23:47:32 Astrophysics Gravitational lens Quasar Large-scale structure of the cosmos Astronomical surveys Dark matter General relativity European Southern Observatory Active galactic nucleus Physics Astronomy Gravitational lensing

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