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10.1073/pnas.1315181111 http://scihub22266oqcxt.onion/10.1073/pnas.1315181111 C4603504!4603504 !25304638     free     free     free Warning: file_get_contents(https://eutils.ncbi.nlm.nih.gov/entrez/eutils/elink.fcgi?dbfrom=pubmed&id=25304638 &cmd=llinks): Failed to open stream: HTTP request failed! HTTP/1.1 429 Too Many Requests in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 215 Deprecated: Implicit conversion from float 209.6 to int loses precision in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 534 Deprecated: Implicit conversion from float 209.6 to int loses precision in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 534 Deprecated: Implicit conversion from float 209.6 to int loses precision in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 534 Warning: imagejpeg(C:\Inetpub\vhosts\kidney.de\httpdocs\phplern\25304638 .jpg): Failed to open stream: No such file or directory in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 117       Proc+Natl+Acad+Sci+U+S+A 2015 ; 112 (40 ): 12272-7 Nephropedia Template TP {{tp|p=25304638 |t=2015. Separating astrophysical sources from indirect dark matter signals |pdf=|usr=}}{{25304638 }} gab.com Text Separating astrophysical sources from indirect dark matter signals JO: Proc Natl Acad Sci U S A http://www.kidney.de/pget.php?&tw=1&pmid=25304638 #FOAvip Indirect searches for products of dark matter annihilation and decay face the challenge of identifying an uncertain and subdominant signal in the presence of uncertain backgrounds. Two valuable approaches to this problem are (i) using analysis methods which take advantage of different features in the energy spectrum and angular distribution of the signal and backgrounds and (ii) more accurately characterizing backgrounds, which allows for more robust identification of possible signals. These two approaches are complementary and can be significantly strengthened when used together. I review the status of indirect searches with gamma rays using two promising targets, the Inner Galaxy and the isotropic gamma-ray background. For both targets, uncertainties in the properties of backgrounds are a major limitation to the sensitivity of indirect searches. I then highlight approaches which can enhance the sensitivity of indirect searches using these targets. Twit Text FOAVip Separating astrophysical sources from indirect dark matter signals ????Proc Natl Acad Sci U S A http://www.kidney.de/pget.php?&tw=1&pmid=25304638 #FOAvip Twit Text # Free Paper on # # # # # LINK http://www.kidney.de/pget.php?&tw=1&pmid=25304638 #FOAvip English Wikipedia <ref>{{Cite pmid|25304638 }}</ref> Separating astrophysical sources from indirect dark matter signals #MMPMID25304638 Siegal-Gaskins JM Proc Natl Acad Sci U S A 2015[Oct]; 112 (40 ): 12272-7 PMID25304638 show ga Indirect searches for products of dark matter annihilation and decay face the challenge of identifying an uncertain and subdominant signal in the presence of uncertain backgrounds. Two valuable approaches to this problem are (i) using analysis methods which take advantage of different features in the energy spectrum and angular distribution of the signal and backgrounds and (ii) more accurately characterizing backgrounds, which allows for more robust identification of possible signals. These two approaches are complementary and can be significantly strengthened when used together. I review the status of indirect searches with gamma rays using two promising targets, the Inner Galaxy and the isotropic gamma-ray background. For both targets, uncertainties in the properties of backgrounds are a major limitation to the sensitivity of indirect searches. I then highlight approaches which can enhance the sensitivity of indirect searches using these targets. äSeparating astrophysical sources from indirect dark matter signals (epmc).pdf DeepDyve Pubget Overpricing