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Co-orbiting satellite galaxy structures are still in conflict with the distribution of primordial dwarf galaxies

, , , , , , , , , , , , , and . (2014)cite arxiv:1406.1799Comment: 19 pages, 9 figures, 6 tables, accepted for publication in MNRAS.

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Nebular metallicities in two isolated Local Void dwarf galaxies, , , and . (2013)cite arxiv:1311.4152Comment: 37 pages, 12 figures, accepted for publication is Astrophysical Jornal.Metal-poor dwarf galaxies in the SIGRID galaxy sample. II. The electron temperature-abundance calibration and the parameters that affect it, , , , , and . (2014)cite arxiv:1405.7170Comment: Accepted for publication in The Astrophysical Journal. 17 figures, 50 pages.Co-orbiting satellite galaxy structures are still in conflict with the distribution of primordial dwarf galaxies, , , , , , , , , and 4 other author(s). (2014)cite arxiv:1406.1799Comment: 19 pages, 9 figures, 6 tables, accepted for publication in MNRAS.The intriguing HI gas in NGC 5253: an infall of a diffuse, low-metallicity HI cloud?, , , , , , and . (2011)cite arxiv:1109.0806Comment: 19 pages, 12 figures, accepted for publication in MNRAS.The Small Isolated Gas Rich Irregular Dwarf (SIGRID) Galaxy Sample: Description and First Results, , , and . (2011)cite arxiv:1107.3898Comment: 13 figures, 3 table. Accepted for publication in The Astronomical Journal.Metal-poor dwarf galaxies in the SIGRID galaxy sample. I. HII region observations and chemical abundances, , , , , and . (2014)cite arxiv:1403.6903Comment: 46 pages, 15 figures, 6 tables, 1 appendix. Accepted for publication in the Astrophysical Journal.