{"id":500,"date":"2013-12-03T18:41:53","date_gmt":"2013-12-03T17:41:53","guid":{"rendered":"http:\/\/astronomy.lamost.org\/blog\/?page_id=500"},"modified":"2014-06-11T09:37:13","modified_gmt":"2014-06-11T07:37:13","slug":"%e6%96%87%e7%8c%ae","status":"publish","type":"page","link":"http:\/\/astronomy.lamost.org\/blog\/?page_id=500","title":{"rendered":"\u6587\u732e"},"content":{"rendered":"<h2>Binary:<\/h2>\n<h2>1. from formation\u00a0 of cbc to EM and GWsignal untill cosmology<\/h2>\n<ul>\n<li><a href=\"http:\/\/arxiv.org\/abs\/astro-ph\/0511811\" target=\"_blank\">Compact Object Modeling with the StarTrack Population Synthesis Code<\/a><\/li>\n<li>http:\/\/www.syntheticuniverse.org\/<\/li>\n<li><a href=\"http:\/\/arxiv.org\/abs\/astro-ph\/0612144\" target=\"_blank\">Formation of Double Co<\/a><a href=\"http:\/\/arxiv.org\/abs\/astro-ph\/0510379\">mpact Objects<span style=\"font-size: 17.000000pt; font-family: 'Times'\"> <\/span><\/a><\/li>\n<\/ul>\n<ul>\n<li><a href=\"http:\/\/arxiv.org\/abs\/1403.4754\">The Evolution of Compact Binary Star Systems<\/a><\/li>\n<\/ul>\n<ul><a href=\"http:\/\/arxiv.org\/abs\/astro-ph\/0510379\"> <\/a><\/p>\n<li><a href=\"http:\/\/arxiv.org\/abs\/astro-ph\/0510379\"><span style=\"font-size: 17.000000pt; font-family: 'Times'\">Evolution and merging of binaries with compact objects <\/span><\/a><\/li>\n<li><a href=\"http:\/\/iopscience.iop.org\/0264-9381\/27\/11\/114007\" target=\"_blank\"><span style=\"font-size: 17.000000pt; font-family: 'Times'\">Compact binary coalescences in the band of ground-based gravitational-wave detectors<\/span><\/a><\/li>\n<li><a href=\"http:\/\/arxiv.org\/abs\/0903.4877\" target=\"_blank\">Gravitational Waves from Merging Compact Binaries<\/a><\/li>\n<\/ul>\n<ul>\n<li><span style=\"font-size: 17.000000pt; font-family: 'Times'\"><span style=\"font-size: 11.000000pt; font-family: 'Times';\"><a href=\"http:\/\/iopscience.iop.org\/0004-637X\/746\/1\/48\">What is the Most Promising Electromagnetic Counterpart of a Neutron Star Binary Merger?<\/a><\/span><\/span><\/li>\n<li><a href=\"http:\/\/relativity.livingreviews.org\/Articles\/lrr-2012-8\/\" target=\"_blank\">Binary Neutron Star Mergers<\/a><\/li>\n<\/ul>\n<ul>\n<li><a href=\"http:\/\/arxiv.org\/abs\/1003.2480\" target=\"_blank\"><span style=\"font-size: 12.000000pt; font-family: 'Helvetica'\">Predictions for the rates of compact binary coalescences observable by ground-based gravitational-wave detectors<\/span><span style=\"font-size: 12.000000pt; font-family: 'AdvP6F01'; color: rgb(13.725000%, 12.157000%, 12.549000%)\"> <\/span><\/a><\/li>\n<li><a href=\"http:\/\/arxiv.org\/abs\/0911.3820\" target=\"_blank\"><span style=\"font-size: 12.000000pt; font-family: 'AdvP6F01'; color: rgb(13.725000%, 12.157000%, 12.549000%)\">Bayesian coherent analysis of in-spiral gravitational wave signals with a detector network<\/span><\/a><\/li>\n<li><a href=\"http:\/\/arxiv.org\/abs\/1301.5616\" target=\"_blank\">When can gravitational-wave observations distinguish between black holes  and neutron stars?<\/a><\/li>\n<\/ul>\n<ul>\n<li><a href=\"http:\/\/arxiv.org\/abs\/0911.3820\" target=\"_blank\"><span style=\"font-size: 12.000000pt; font-family: 'AdvP6F01'; color: rgb(13.725000%, 12.157000%, 12.549000%)\"> <\/span><\/a><a href=\"http:\/\/arxiv.org\/abs\/1209.3027\" target=\"_blank\"><span style=\"font-size: 12.000000pt; font-family: 'AdvP6F01'\">Electromagnetic transients as triggers in searches for gravitational waves <\/span><\/a><a href=\"http:\/\/arxiv.org\/abs\/1209.3027\" target=\"_blank\"><span style=\"font-size: 12.000000pt; font-family: 'AdvP6F01'\">from compact binary mergers <\/span><\/a><\/li>\n<li><span style=\"font-size: 12.000000pt; font-family: 'AdvP6F01'\"><a href=\"http:\/\/arxiv.org\/abs\/1209.3027\" target=\"_blank\"><span style=\"font-size: 12.000000pt; font-family: 'AdvP6F01'; color: rgb(13.725000%, 12.157000%, 12.549000%);\">Identifying the host galaxy of gravitational wave signals <\/span><\/a><\/span><\/li>\n<\/ul>\n<ul>\n<li><a href=\"http:\/\/adsabs.harvard.edu\/abs\/2014arXiv1406.1544F\" target=\"_blank\"><span style=\"font-size: 12.000000pt; font-family: 'AdvP6F01'; color: rgb(13.725000%, 12.157000%, 12.549000%)\">A Bayesian approach to multi-messenger astronomy: Identification of gravitational-wave host galaxies<\/span><\/a> \uff08my contribution\uff09<\/li>\n<li><a href=\"http:\/\/adsabs.harvard.edu\/abs\/1986Natur.323..310S\" target=\"_blank\"><span style=\"font-size: 12.000000pt; font-family: 'AdvP6F01'; color: rgb(13.725000%, 12.157000%, 12.549000%)\">Determining the Hubble constant from gravitational wave observations<\/span><\/a><\/li>\n<li><a href=\"http:\/\/adsabs.harvard.edu\/abs\/2012PhRvL.108i1101M\" target=\"_blank\"><span style=\"font-size: 12.000000pt; font-family: 'AdvP6F01'; color: rgb(13.725000%, 12.157000%, 12.549000%)\">Measuring a Cosmological Distance-Redshift Relationship Using Only  Gravitational Wave Observations of Binary Neutron Star Coalescences<\/span><\/a><\/li>\n<li><a href=\"http:\/\/adsabs.harvard.edu\/abs\/2012PhRvD..85b3535T\"><span style=\"font-size: 12.000000pt; font-family: 'AdvP6F01'; color: rgb(13.725000%, 12.157000%, 12.549000%)\">Cosmology using advanced gravitational-wave detectors alone<\/span><\/a><\/li>\n<li><a href=\"http:\/\/arxiv.org\/abs\/1209.0595\" target=\"_blank\">On the gravitational wave background from compact binary coalescences in  the band of ground-based interferometers<\/a><\/li>\n<\/ul>\n<ul>\n<li><a href=\"http:\/\/arxiv.org\/abs\/1309.5731\" target=\"_blank\">Strong gravitational lensing of gravitational waves in Einstein  Telescope<\/a> (\u5f3a\u5f15\u529b\u900f\u955c\uff0bcbc \u5f15\u529b\u6ce2\uff0b\u5b87\u5b99\u6052\u661f\u6f14\u5316\u5386\u53f2\uff0d\u300b\u5b87\u5b99\u5b66)<span> <\/span><\/li>\n<li><a href=\"http:\/\/onlinelibrary.wiley.com\/doi\/10.1111\/j.1365-2966.2010.16317.x\/abstract\" target=\"_blank\"><span>Delensing gravitational wave standard sirens with shear and flexion maps<\/span><\/a> (\u5f31\u5f15\u529b\u900f\u955c\uff0b(SMBHB) \u5f15\u529b\u6ce2\uff0b\u5b87\u5b99\u6052\u661f\u6f14\u5316\u5386\u53f2\uff0d\u300b\u5b87\u5b99\u5b66)<\/li>\n<\/ul>\n<p><a href=\"http:\/\/tangledfields.com\/gwem\/\" target=\"_blank\">Joining the GW\/EM\u00a0Skies<\/a><\/p>\n<h2>2. chemical effect- GCM<\/h2>\n<ul>\n<li><a href=\"http:\/\/www.sciencedirect.com\/science\/article\/pii\/S1384107601000902\" target=\"_blank\">The chemical evolution of the solar neighbourhood: the effect of binaries<\/a><\/li>\n<li><a href=\"http:\/\/www.sciencedirect.com\/science\/article\/pii\/S1387647310000734#\" target=\"_blank\">Binaries, galactic chemical evolution and the puzzling temporal evolution of <sup>14<\/sup>N in the solar neighbourhood<\/a><\/li>\n<\/ul>\n<h2>3. chemical effect- GW<\/h2>\n<ul>\n<li><a href=\"http:\/\/iopscience.iop.org\/2041-8205\/715\/2\/L138\">T<\/a><a href=\"http:\/\/iopscience.iop.org\/2041-8205\/715\/2\/L138\/\" target=\"_blank\">he Effect of Metallicity on the Detection Prospects for Gravitational Waves<\/a><\/li>\n<li>My paper?? with\u00a0 the help of :<\/li>\n<\/ul>\n<h2>4. GCM-GRB host<\/h2>\n<div title=\"Page 1\">\n<div>\n<ul>\n<li><a href=\"http:\/\/arxiv.org\/abs\/1007.4435http:\/\/\" target=\"_blank\">The nature of Long-GRB host galaxies from chemical abundances<\/a> (my work)<\/li>\n<\/ul>\n<\/div>\n<\/div>\n","protected":false},"excerpt":{"rendered":"<p>Binary: 1. from formation\u00a0 of cbc to EM and GWsignal un&#8230;<\/p>\n","protected":false},"author":2,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"footnotes":""},"class_list":["post-500","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"http:\/\/astronomy.lamost.org\/blog\/index.php?rest_route=\/wp\/v2\/pages\/500","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=500"}],"version-history":[{"count":22,"href":"http:\/\/astronomy.lamost.org\/blog\/index.php?rest_route=\/wp\/v2\/pages\/500\/revisions"}],"predecessor-version":[{"id":575,"href":"http:\/\/astronomy.lamost.org\/blog\/index.php?rest_route=\/wp\/v2\/pages\/500\/revisions\/575"}],"wp:attachment":[{"href":"http:\/\/astronomy.lamost.org\/blog\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=500"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}