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ZENODO
Presentation . 2019
License: CC BY
Data sources: Datacite
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ZENODO
Presentation . 2019
License: CC BY
Data sources: Datacite
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Mapping stellar streams with LSST

descriptionPublicationkeyboard_double_arrow_right Presentation 22 May 2019Publisher:Zenodo
Authors: Simpson, Jeffrey;

doi: 10.5281/zenodo.5407599 , 10.5281/zenodo.5407600

Mapping stellar streams with LSST

Abstract

Large photometric surveys like SDSS and DES have shown that the Milky Way Galaxy is littered with stellar streams; the remnants of tidally disrupted star clusters and dwarf galaxies. However these surveys were limited to either the northern sky, or only a region of the southern sky. In this talk I will discuss the power of LSST in the age of Gaia to discover and also to help characterise these streams with its broad colour photometry. I will also discuss on-going and future spectroscopic surveys of stellar streams.

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
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popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
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