tag:blogger.com,1999:blog-73794446267828921032024-02-19T08:40:04.057-08:00rachel's research blograchel somervillehttp://www.blogger.com/profile/05511010839959257943noreply@blogger.comBlogger1125tag:blogger.com,1999:blog-7379444626782892103.post-49068287882624415572009-11-05T13:02:00.000-08:002011-02-09T19:39:30.707-08:00very high redshift galaxies<a onblur="try {parent.deselectBloggerImageGracefully();} catch(e) {}" href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjhUWDm7AujXZ8bh23t4DXvkNh0FixExmRbjPPeayh9IzyuonQ1a_viweKAhyrxgIRwdOmePWXTLT6ePiUKxaa79wk88-EkXJ_rm1X_xuRFVHzgVkoEazbreY8PIizFZkZMfkmwQ17VAKk/s1600/magmhalofid.jpg"><img style="display: block; margin: 0px auto 10px; text-align: center; cursor: pointer; width: 320px; height: 290px;" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjhUWDm7AujXZ8bh23t4DXvkNh0FixExmRbjPPeayh9IzyuonQ1a_viweKAhyrxgIRwdOmePWXTLT6ePiUKxaa79wk88-EkXJ_rm1X_xuRFVHzgVkoEazbreY8PIizFZkZMfkmwQ17VAKk/s320/magmhalofid.jpg" alt="" id="BLOGGER_PHOTO_ID_5571899911761939858" border="0" /></a>halo mass vs. observed magnitude. UDF WFC3 observations reach a depth of ~29 in J125W.<br /><a onblur="try {parent.deselectBloggerImageGracefully();} catch(e) {}" href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjSQeIH6xTd9FZazHipebmFwczD6SXpSZahB28xJMsHf27Pp3H5gFIXmyzlGY_CbQ0qMDJHbxUK8m-J7ozNBgY0h6RNMsGdJw3R60X0Rhr_BYr4SGaYZCUrChVcqgWubpbdrSSX4p7xTMI/s1600/lfz678fidhires.jpg"><img style="display: block; margin: 0px auto 10px; text-align: center; cursor: pointer; width: 320px; height: 290px;" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjSQeIH6xTd9FZazHipebmFwczD6SXpSZahB28xJMsHf27Pp3H5gFIXmyzlGY_CbQ0qMDJHbxUK8m-J7ozNBgY0h6RNMsGdJw3R60X0Rhr_BYr4SGaYZCUrChVcqgWubpbdrSSX4p7xTMI/s320/lfz678fidhires.jpg" alt="" id="BLOGGER_PHOTO_ID_5571899144670960386" border="0" /></a>rest UV LF at z=6, 7, 8. solid=no dust, dashed=with dust. dot-dashed=observations.<br /><a onblur="try {parent.deselectBloggerImageGracefully();} catch(e) {}" href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgbDgmCLpZwp94hpr9-sKXK4euHN88gyBgWk73OobO8GiNLpbN1bKBatR6gD51r2OAaCmG5Iqau73adKMJMoGuB_JFc4jjWqZeXxNb83H3y1x3KopQXLxJezi7UQCabx-Pq58uIg9QjsOE/s1600/lfz678nfbhires.jpg"><img style="display: block; margin: 0px auto 10px; text-align: center; cursor: pointer; width: 320px; height: 290px;" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgbDgmCLpZwp94hpr9-sKXK4euHN88gyBgWk73OobO8GiNLpbN1bKBatR6gD51r2OAaCmG5Iqau73adKMJMoGuB_JFc4jjWqZeXxNb83H3y1x3KopQXLxJezi7UQCabx-Pq58uIg9QjsOE/s320/lfz678nfbhires.jpg" alt="" id="BLOGGER_PHOTO_ID_5571898712046836418" border="0" /></a><br />rest UV luminosity function, no feedback. solid=no dust, dashed=with dust. dot-dashed: observations.<br /><br /><br /><br /><a onblur="try {parent.deselectBloggerImageGracefully();} catch(e) {}" href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjjUT6fig9RSA3dK_eRMQk2_LugqvDP9fiIJUy8jyDyzWqrZhkko24Em2OKSwKhOpORS_v8qid7njj56L8c0ycfLtBYhIJf8ZKVfPvg1FTNoAyk0IJWyjF6Qx7wpp93N2p8puLk1ABZIvQ/s1600/mfstarz6_kenngk.jpg"><img style="float: left; margin: 0pt 10px 10px 0pt; cursor: pointer; width: 320px; height: 290px;" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjjUT6fig9RSA3dK_eRMQk2_LugqvDP9fiIJUy8jyDyzWqrZhkko24Em2OKSwKhOpORS_v8qid7njj56L8c0ycfLtBYhIJf8ZKVfPvg1FTNoAyk0IJWyjF6Qx7wpp93N2p8puLk1ABZIvQ/s320/mfstarz6_kenngk.jpg" alt="" id="BLOGGER_PHOTO_ID_5571897736433600178" border="0" /></a><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br />stellar mass function at z=6. points=Stark et al. observations. red dotted=Nagamine sims (no stellar FB). dot-dashed red=SAM w/ no FB.<br /><br /><br /><br /><a onblur="try {parent.deselectBloggerImageGracefully();} catch(e) {}" href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEi6k1QogBYwTWoTx2MDV-ihmRgy_emWmzg1KR0vzQO9yH3rWnnkx41gMsGedS3e6px2dpt-lOFSqBAprzdrglKL6exvQlZuSQePdE6fWkxo4U4G-qS8zgEjjhS2D-hFtDXoEPjkU3t35Ss/s1600/mhmstarfid.jpg"><img style="float: left; margin: 0pt 10px 10px 0pt; cursor: pointer; width: 320px; height: 288px;" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEi6k1QogBYwTWoTx2MDV-ihmRgy_emWmzg1KR0vzQO9yH3rWnnkx41gMsGedS3e6px2dpt-lOFSqBAprzdrglKL6exvQlZuSQePdE6fWkxo4U4G-qS8zgEjjhS2D-hFtDXoEPjkU3t35Ss/s320/mhmstarfid.jpg" alt="" id="BLOGGER_PHOTO_ID_5571897533068374306" border="0" /></a><br />halo mass vs. stellar mass relation. orange lines=Behroozi et al. relations at the indicated redshifts. blue lines = Behroozi et al. at z=0.<br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><div style="text-align: left;"><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /></div>rachel somervillehttp://www.blogger.com/profile/05511010839959257943noreply@blogger.com0