41![Focusing on Warm Dark Matter with Lensed High-Redshift Galaxies Fabio Pacucci Scuola Normale Superiore - Italy Ecole Internationale d’Astrophysique Daniel Chalonge Focusing on Warm Dark Matter with Lensed High-Redshift Galaxies Fabio Pacucci Scuola Normale Superiore - Italy Ecole Internationale d’Astrophysique Daniel Chalonge](https://www.pdfsearch.io/img/ec4bb6dd5b1e6801d9463609d0ddbe5d.jpg) | Add to Reading ListSource URL: chalonge.obspm.frLanguage: English - Date: 2014-06-10 03:20:56
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42![2014 SAO Summer Intern Project Abstracts Discovery of Compact Quiescent Galaxies at Intermediate Redshifts in DEEP2 Kirsten Blancato1 Igor Chilingarian2,3 , Ivana Damjanov4 , Sean Moran3 , Ivan Katkov4,3 (1 Wellesley Col 2014 SAO Summer Intern Project Abstracts Discovery of Compact Quiescent Galaxies at Intermediate Redshifts in DEEP2 Kirsten Blancato1 Igor Chilingarian2,3 , Ivana Damjanov4 , Sean Moran3 , Ivan Katkov4,3 (1 Wellesley Col](https://www.pdfsearch.io/img/31215f8e94fb557055e719126a93349e.jpg) | Add to Reading ListSource URL: hea-www.harvard.eduLanguage: English - Date: 2014-12-31 12:51:36
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43![Giant cosmic tsunami wakes up comatose galaxies Royal Astronomical Society press release RAS PRApril 2015 EMBARGOED UNTIL 0601 BST, 24 APRILGMT, 24 APRILGalaxies are often found in clusters, Giant cosmic tsunami wakes up comatose galaxies Royal Astronomical Society press release RAS PRApril 2015 EMBARGOED UNTIL 0601 BST, 24 APRILGMT, 24 APRILGalaxies are often found in clusters,](https://www.pdfsearch.io/img/795fa7aedfc368be972259f6bd3165f9.jpg) | Add to Reading ListSource URL: www.strw.leidenuniv.nlLanguage: English - Date: 2015-04-24 04:55:29
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44![Uranometria’s Galaxy Cluster Database This atlas contains 671 galaxy clusters derived from George Abell’s 1958 catalog based upon photographs from Mt. Palomar Observatory. In 1980 Abell issued a revision to th Uranometria’s Galaxy Cluster Database This atlas contains 671 galaxy clusters derived from George Abell’s 1958 catalog based upon photographs from Mt. Palomar Observatory. In 1980 Abell issued a revision to th](https://www.pdfsearch.io/img/ffa83bdf99bdae8c89908bb941250a0f.jpg) | Add to Reading ListSource URL: willbell.comLanguage: English - Date: 2008-10-21 19:04:10
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45![Uranometria’s Globular Cluster Database Some 170 globular clusters, including both Milky Way and Magellanic Cloud objects; are contained in this atlas. They are shown as a continuous-line open circle with an int Uranometria’s Globular Cluster Database Some 170 globular clusters, including both Milky Way and Magellanic Cloud objects; are contained in this atlas. They are shown as a continuous-line open circle with an int](https://www.pdfsearch.io/img/e874b715379aa80433081d0f9c4940f3.jpg) | Add to Reading ListSource URL: willbell.comLanguage: English - Date: 2008-10-21 19:15:19
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46![Microsoft Word - clusters_icrc2005.doc Microsoft Word - clusters_icrc2005.doc](https://www.pdfsearch.io/img/452b004c87ed89859dfb171d04a12ac2.jpg) | Add to Reading ListSource URL: hawc.pa.msu.eduLanguage: English - Date: 2005-08-24 14:09:12
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47![GALAXIES AND GALAXY CLUSTERS NGC 4414, credits: NASA/HST Bruno Giacomazzo www.brunogiacomazzo.org GALAXIES AND GALAXY CLUSTERS NGC 4414, credits: NASA/HST Bruno Giacomazzo www.brunogiacomazzo.org](https://www.pdfsearch.io/img/e8574bdd7d099659707a64c9cde25c7b.jpg) | Add to Reading ListSource URL: www.brunogiacomazzo.org- Date: 2014-04-11 12:24:22
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48![Dark matter is darker than once thought Dark matter is darker than once thought](https://www.pdfsearch.io/img/842624dc69fef7e09879d733f048db36.jpg) | Add to Reading ListSource URL: phys.orgLanguage: English - Date: 2015-05-31 16:22:55
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49![The X-ray luminous galaxy cluster XMMUJ1007.4+1237 at z = 1.56 The X-ray luminous galaxy cluster XMMUJ1007.4+1237 at z = 1.56](https://www.pdfsearch.io/img/177569ac99fc20df1d72747cf3e75b71.jpg) | Add to Reading ListSource URL: www.aanda.orgLanguage: English |
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50![](https://www.pdfsearch.io/img/e29ff5aaff2143b8d0bdf86c6abf839c.jpg) | Add to Reading ListSource URL: prometeo.sif.itLanguage: English - Date: 2014-08-22 06:19:00
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