Downloads provided by UsageCounts
doi: 10.5281/zenodo.44697
The science of the LSST will, in part, be driven by how it observes the sky (the footprint and cadence of the survey). I provide a brief overview of the ongoing community and Project work on LSST observing strategy, and pointers for how to join this effort.
NSF Pavilion talk presented at the American Astronomical Society meeting 227.
LSST, Astronomy, Optical Surveys
LSST, Astronomy, Optical Surveys
| 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). | 1 | |
| 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. | Average | |
| influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | Average | |
| impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network. | Average |
| views | 92 | |
| downloads | 20 |

Views provided by UsageCounts
Downloads provided by UsageCounts