{"id":117,"date":"2010-02-04T14:22:06","date_gmt":"2010-02-04T13:22:06","guid":{"rendered":"http:\/\/astronomy.lamost.org\/blog\/?page_id=117"},"modified":"2013-10-02T10:36:29","modified_gmt":"2013-10-02T08:36:29","slug":"galaxy","status":"publish","type":"page","link":"http:\/\/astronomy.lamost.org\/blog\/?page_id=117","title":{"rendered":"Galaxy"},"content":{"rendered":"<div id=\"_mcePaste\" style=\"overflow: hidden; left: -10000px; width: 1px; position: absolute; top: 0px; height: 1px;\">1. physical parameters<\/div>\n<h2>lecture and review<\/h2>\n<p><strong><a href=\"http:\/\/arxiv.org\/abs\/astro-ph\/0701024\" target=\"_blank\">Observations of the High Redshift Universe<\/a><\/strong><\/p>\n<p><strong><span style=\"font-family: 'Lucida Grande', helvetica, arial, verdana, sans-serif; font-weight: normal; line-height: normal; font-size: 14px;\"><a href=\"http:\/\/arxiv.org\/abs\/1006.5394\" target=\"_blank\">Galaxy Formation Theory<\/a><\/span><\/strong><\/p>\n<p><strong><span style=\"font-family: 'Lucida Grande', helvetica, arial, verdana, sans-serif; font-weight: normal; line-height: normal; font-size: 14px;\"><a href=\"http:\/\/arxiv.org\/abs\/0908.3017\" target=\"_blank\">Physical properties and environments of nearby galaxies<\/a><\/span><\/strong><\/p>\n<p><strong><span style=\"font-family: 'Lucida Grande', helvetica, arial, verdana, sans-serif; font-weight: normal; line-height: normal; font-size: 14px;\"><span style=\"font-family: Simsun; font-size: small; color: #ffffff;\"><span style=\"color: #000000;\"><a href=\"http:\/\/www.astro.ucla.edu\/~aes\/AST274\/\" target=\"_blank\">Galaxies<\/a><\/span><\/span><\/span><\/strong><\/p>\n<p><strong><span style=\"color: #000000;\"><span style=\"color: #ffffff;\"><span style=\"color: #000000;\"><a href=\"http:\/\/www.astro.ucla.edu\/~aes\/AST278\/\" target=\"_blank\">The Formation and Evolution of Galaxies and the IGM<\/a><\/span><\/span><\/span><\/strong><\/p>\n<p class=\"title\"><a href=\"http:\/\/arxiv.org\/abs\/1309.3276\">Galaxy Masses: A Review<\/a><\/p>\n<p><a href=\"http:\/\/www.mpa-garching.mpg.de\/~magpop\/\"><\/a><\/p>\n<p><a href=\"http:\/\/www.mpa-garching.mpg.de\/~magpop\/\"><\/p>\n<h2>Multiwavelength Analysis of Galaxy Populations: Lectures<\/h2>\n<p><\/a><\/p>\n<p><a href=\"http:\/\/www.mpa-garching.mpg.de\/~magpop\/\"><\/a><\/p>\n<p><a href=\"http:\/\/www.mpa-garching.mpg.de\/~magpop\/\"><\/a><\/p>\n<p><strong> <\/strong><\/p>\n<p><strong> <\/strong><\/p>\n<p><strong> <\/strong><\/p>\n<p><strong> <\/strong><\/p>\n<p><strong> <\/strong><\/p>\n<h2><strong><a href=\"http:\/\/books.google.com\/books?uid=10901955766043113897&amp;as_coll=1004&amp;hl=zh-CN&amp;source=gbs_lp_bookshelf_list\" target=\"_blank\"><span style=\"color: #000000;\">Book<\/span><\/a><\/strong><\/h2>\n<p><strong><br \/>\n<\/strong><\/p>\n<h2><span style=\"color: #000000;\">physical parameters<\/span><\/h2>\n<p>We want to know Physical parameters, but usually some of them can not be directly<br \/>\nmeasured.<\/p>\n<ul>\n<li>1. redshift,<\/li>\n<\/ul>\n<p>Photometric redshift and Spectroscopic redshift<\/p>\n<ul>\n<li>2. age<\/li>\n<li>3. mass<\/li>\n<li>4. luminosity<\/li>\n<li>5. color<\/li>\n<li>6. metallcity<\/li>\n<li>7. dust extiction<\/li>\n<li>8. star formation activity<\/li>\n<li>9.size<\/li>\n<\/ul>\n<h2><span style=\"color: #000000;\">Phenomenology<\/span><\/h2>\n<h2><span style=\"color: #000000;\">Morphology<\/span><\/h2>\n<h2><span style=\"color: #000000;\"><a href=\"http:\/\/www.mssl.ucl.ac.uk\/~ipf\/J10\/Programme.html\" target=\"_blank\">Environments<\/a><\/span><\/h2>\n<h2>Galaxy formation<\/h2>\n<p>groups :<\/p>\n<p><a href=\"http:\/\/www.galform.org\/\">http:\/\/www.galform.org\/<\/a><\/p>\n<p>methords:<\/p>\n<p><a href=\"http:\/\/astronomy.lamost.org\/blog\/?page_id=90\" target=\"_blank\">Chemcial evolution model<\/a><\/p>\n<p><a href=\"http:\/\/arxiv.org\/abs\/1104.0669\" target=\"_blank\">semi-analytical modelling<\/a><\/p>\n<p>numerical simulations<\/p>\n","protected":false},"excerpt":{"rendered":"<p>1. physical parameters lecture and review Observations &#8230;<\/p>\n","protected":false},"author":2,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"open","ping_status":"open","template":"","meta":{"footnotes":""},"class_list":["post-117","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"http:\/\/astronomy.lamost.org\/blog\/index.php?rest_route=\/wp\/v2\/pages\/117","targetHints":{"allow":["GET"]}}],"collection":[{"href":"http:\/\/astronomy.lamost.org\/blog\/index.php?rest_route=\/wp\/v2\/pages"}],"about":[{"href":"http:\/\/astronomy.lamost.org\/blog\/index.php?rest_route=\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"http:\/\/astronomy.lamost.org\/blog\/index.php?rest_route=\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"http:\/\/astronomy.lamost.org\/blog\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=117"}],"version-history":[{"count":27,"href":"http:\/\/astronomy.lamost.org\/blog\/index.php?rest_route=\/wp\/v2\/pages\/117\/revisions"}],"predecessor-version":[{"id":459,"href":"http:\/\/astronomy.lamost.org\/blog\/index.php?rest_route=\/wp\/v2\/pages\/117\/revisions\/459"}],"wp:attachment":[{"href":"http:\/\/astronomy.lamost.org\/blog\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=117"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}