1. ENE. Tallinn: Kirjastus ,,Valgus", 1988 2. JAANISTE, J. Füüsika XII klassile. Tallinn: Koolibri, 1999 3. http://www.aai.ee/~urmas/UT/A4.pdf 4. http://opik.obs.ee/osa4/ptk02/box01.html 5. http://et.wikipedia.org/wiki/Galaktika#Galaktikate_jagunemine_kuju_j.C3.A4rgi 6. http://www.slideshare.net/TriinuToon/fsika-esitlus-teised-galaktikad Pildid 1. http://en.wikipedia.org/wiki/File:HubbleTuningFork.jpg 2. http://en.wikipedia.org/wiki/File:Abell_S740,_cropped_to_ESO_325-G004.jpg 3. http://et.wikipedia.org/wiki/Pilt:M101_hires_STScI-PRC2006-10a.jpg 4. http://et.wikipedia.org/wiki/Pilt:Hubble2005-01-barred-spiral-galaxy-NGC1300.jpg 5. http://blogs.zooniverse.org/galaxyzoo/files/2010/12/NGC5866-869x1024.jpg 6. http://en.wikipedia.org/wiki/File:Magellanic_Clouds_ %E2%80%95_Irregular_Dwarf_Galaxies_.jpg 7. http://et.wikipedia.org/wiki/Pilt:Hoag%27s_object.jpg 11
detected in ITS2 were more dispersed. Substitutions occurred in where the samples were taken. The excised sponge areas were always ITS2 positions 151 (CRA), 244 (TRA) and 268 (CRG) (Table 4). smaller than the label area. Our proportion model allowed us to detect single substitutions doi:10.1371/journal.pone.0066601.g004 even in the case where they were located in the sequence following PLOS ONE | www.plosone.org 6 June 2013 | Volume 8 | Issue 6 | e66601 Intragenomic Profiling Using Multicopy Genes Table 3