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Six More Ultra-Faint Milky Way Companions Discovered in the DECam Local Volume Exploration Survey

Authors :
Cerny, W.
Martínez-Vázquez, C. E.
Drlica-Wagner, A.
Pace, A. B.
Mutlu-Pakdil, B.
Li, T. S.
Riley, A. H.
Crnojević, D.
Bom, C. R.
Carballo-Bello, J. A.
Carlin, J. L.
Chiti, A.
Choi, Y.
Collins, M. L. M.
Darragh-Ford, E
Ferguson, P. S.
Geha, M.
Martínez-Delgado, D.
Massana, P.
Mau, S.
Medina, G. E.
Muñoz, R. R.
Nadler, E. O.
Olsen, K. A. G.
Pieres, A.
Sakowska, J. D.
Simon, J. D.
Stringfellow, G. S.
Vivas, A. K.
Walker, A. R.
Wechsler, R. H.
Publication Year :
2022

Abstract

We report the discovery of six ultra-faint Milky Way satellites discovered through matched-filter searches conducted using Dark Energy Camera (DECam) data processed as part of the second data release of the DECam Local Volume Exploration (DELVE) survey. Leveraging deep Gemini/GMOS-N imaging (for four candidates) as well as follow-up DECam imaging (for two candidates), we characterize the morphologies and stellar populations of these systems. We find that these candidates all share faint absolute magnitudes ($M_{V} \geq -3.2$ mag) and old, metal-poor stellar populations ($\tau > 10$ Gyr, [Fe/H] $< -1.4$ dex). Three of these systems are more extended ($r_{1/2} > 15$ pc), while the other three are compact ($r_{1/2} < 10$ pc). From these properties, we infer that the former three systems (Bo\"{o}tes V, Leo Minor I, and Virgo II) are consistent with ultra-faint dwarf galaxy classifications, whereas the latter three (DELVE 3, DELVE 4, and DELVE 5) are likely ultra-faint star clusters. Using data from the Gaia satellite, we confidently measure the proper motion of Bo\"{o}tes V, Leo Minor I, and DELVE 4, and tentatively detect a proper motion signal from DELVE 3 and DELVE 5; no signal is detected for Virgo II. We use these measurements to explore possible associations between the newly-discovered systems and the Sagittarius dwarf spheroidal, the Magellanic Clouds, and the Vast Polar Structure, finding several plausible associations. Our results offer a preview of the numerous ultra-faint stellar systems that will soon be discovered by the Vera C. Rubin Observatory and highlight the challenges of classifying the faintest stellar systems.<br />Comment: 30 pages, 12 Figures (including Appendix). Submitted to ApJ. We encourage the reader to also review Smith et al. 2022, "Discovery of a new Local Group Dwarf Galaxy Candidate in UNIONS: Bo\"{o}tes V" (arxiv: 2209.08242), who independently present the discovery of one of the candidates reported here. We are working to make code and data products available

Details

Database :
arXiv
Publication Type :
Report
Accession number :
edsarx.2209.12422
Document Type :
Working Paper
Full Text :
https://doi.org/10.3847/1538-4357/acdd78