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          Institute: MPI für Astronomie     Collection: Publikationen_mpia     Display Documents



ID: 731942.0, MPI für Astronomie / Publikationen_mpia
A synoptic map of halo substructures from the Pan-STARRS1 3π Survey
Authors:Bernard, E. J.; Ferguson, A. M. N.; Schlafly, E. F.; Martin, N. F.; Rix, H.-W.; Bell, E. F.; Finkbeiner, D. P.; Goldman, B.; Martínez-Delgado, D.; Sesar, B.; Wyse, R. F. G.; Burgett, W. S.; Chambers, K. C.; Draper, P. W.; Hodapp, K. W.; Kaiser, N.; Kudritzki, R.-P.; Magnier, E. A.; Metcalfe, N.; Wainscoat, R. J.; Waters, C.
Date of Publication (YYYY-MM-DD):2016
Title of Journal:Monthly Notices of the Royal Astronomical Society
Volume:463
Issue / Number:2
Start Page:1759
End Page:1768
Audience:Not Specified
Abstract / Description:We present a panoramic map of the entire Milky Way halo north of δ ˜ -30° (˜ 30,000 deg2), constructed by applying the matched-filter technique to the Pan-STARRS1 3π Survey dataset. Using single-epoch photometry reaching to g ˜22, we are sensitive to stellar substructures with heliocentric distances between 3.5 and ˜35 kpc. We recover almost all previously-reported streams in this volume and demonstrate that several of these are significantly more extended than earlier datasets have indicated. In addition, we also report five new candidate stellar streams. One of these features appears significantly broader and more luminous than the others and is likely the remnant of a dwarf galaxy. The other four streams are consistent with a globular cluster origin, and three of these are rather short in projection (≲ 10°), suggesting that streams like Ophiuchus may not be that rare. Finally, a significant number of more marginal substructures are also revealed by our analysis; many of these features can also be discerned in matched-filter maps produced by other authors from SDSS data, and hence they are very likely to be genuine. However, the extant 3π data is currently too shallow to determine their properties or produce convincing CMDs. The global view of the Milky Way provided by Pan-STARRS1 provides further evidence for the important role of both globular cluster disruption and dwarf galaxy accretion in building the Milky Way's stellar halo.
Free Keywords:Hertzsprung-Russell and colour-magnitude diagrams; surveys; Galaxy: halo; Galaxy: structure
External Publication Status:published
Document Type:Article
Communicated by:N. N.
Affiliations:MPI für Astronomie
Identifiers:ISSN:0035-8711 %R 10.1093/mnras/stw2134
URL:http://adsabs.harvard.edu/abs/2016MNRAS.463.1759B
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