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A Synoptic Map of Halo Substructures from the Pan-STARRS1 3π Survey

Authors :
Nicolas F. Martin
Hans-Walter Rix
Peter W. Draper
Edouard J. Bernard
Nigel Metcalfe
Branimir Sesar
Douglas P. Finkbeiner
Rolf-Peter Kudritzki
Christopher Waters
Eric F. Bell
Richard J. Wainscoat
David Martinez-Delgado
Eugene A. Magnier
William S. Burgett
Edward F. Schlafly
K. C. Chambers
Nick Kaiser
Klaus W. Hodapp
Rosemary F. G. Wyse
Bertrand Goldman
Annette M. N. Ferguson
Observatoire astronomique de Strasbourg (ObAS)
Université de Strasbourg (UNISTRA)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)
Source :
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 2016, ' A Synoptic Map of Halo Substructures from the Pan-STARRS1 3π Survey ', Monthly Notices of the Royal Astronomical Society, vol. 463, no. 2, pp. 1759–1768 . https://doi.org/10.1093/mnras/stw2134, Monthly Notices of the Royal Astronomical Society, Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2016, 463 (2), pp.1759-1768. ⟨10.1093/mnras/stw2134⟩, Monthly notices of the Royal Astronomical Society, 2016, Vol.463(2), pp.1759-1768 [Peer Reviewed Journal]
Publication Year :
2016

Abstract

We present a panoramic map of the entire Milky Way halo north of dec~-30 degrees (~30,000 deg^2), constructed by applying the matched-filter technique to the Pan-STARRS1 3Pi 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 (<br />Comment: 12 pages, 6 figures. MNRAS, in press. The maps in FITS format for the 26 distance slices are made available to the community at http://dx.doi.org/10.5281/zenodo.60518, while full sky colour maps in various projections are provided at http://www.roe.ac.uk/~ejb/streams.html

Details

Language :
English
ISSN :
00358711 and 13652966
Database :
OpenAIRE
Journal :
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 2016, ' A Synoptic Map of Halo Substructures from the Pan-STARRS1 3π Survey ', Monthly Notices of the Royal Astronomical Society, vol. 463, no. 2, pp. 1759–1768 . https://doi.org/10.1093/mnras/stw2134, Monthly Notices of the Royal Astronomical Society, Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2016, 463 (2), pp.1759-1768. ⟨10.1093/mnras/stw2134⟩, Monthly notices of the Royal Astronomical Society, 2016, Vol.463(2), pp.1759-1768 [Peer Reviewed Journal]
Accession number :
edsair.doi.dedup.....0d00c150e97f2212ee23d70005a86571