New Spectroscopic Redshift Places PEARLSDG in a Group at ∼124 Mpc

Timothy Carleton, Steven P. Willner, Timothy Ellsworth-Bowers, Rogier A. Windhorst, Seth H. Cohen, Christopher J. Conselice, Jose M. Diego, Adi Zitrin, Haylee N. Archer, Isabel McIntyre, Patrick Kamieneski, Rolf A. Jansen, Jake Summers, Jordan C. J. D’Silva, Anton M. Koekemoer, Dan Coe, Simon P. Driver, Brenda Frye, Norman A. Grogin, Madeline A. Marshall, Mario Nonino, Nor Pirzkal, Aaron Robotham, Russell E. Ryan, Rafael Ortiz, Scott Tompkins, Christopher N. A. Willmer, Haojing Yan and Benne W. Holwerda
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Abstract

PEARLSDG was previously reported as an isolated dwarf galaxy with a TRGB distance of 30 Mpc. New data show this to not be the case. We report a new spectroscopic redshift of 0.02809, which argues for an association with a group of galaxies at ∼124 Mpc.
新的光谱红移将 PEARLSDG 置于 ∼124 Mpc 的星团中
据报道,PEARLSDG以前是一个孤立的矮星系,其TRGB距离为30 Mpc。新的数据表明情况并非如此。我们报告了一个新的光谱红移(0.02809),证明它与∼124 Mpc处的星系群有联系。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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