Abstract | ||
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For examining possibilities and challenges in doing science with multi-band and non-simultaneous data from upcoming surveys like LSST, the Pan-STARRS1 (PS1) 3p can be used as a pilot survey. This is especially important to explore the possibilities in detection and classification of variable sources within the first years of LSST's 10-year baseline. We had explored the capabilities of PS1 3p for carrying out time-domain science in a variety of applications. We had used structure function fitting as well as period fitting, to search for and classify high-latitude as well as low-latitude variable sources, in particular RR Lyrae, Cepheids and QSOs. |
Year | DOI | Venue |
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2016 | 10.1017/S1743921316012667 | IAU Symposium Proceedings Series |
Keywords | Field | DocType |
methods: data analysis,methods: statistical,catalogs,surveys,(stars: variables:) Cepheids,stars: variables: other,(galaxies:) quasars: general | Time domain,Panopticon,Visual arts,Sociology | Conference |
Volume | Issue | ISSN |
12 | S325 | 1743-9213 |
Citations | PageRank | References |
0 | 0.34 | 0 |
Authors | ||
4 |
Name | Order | Citations | PageRank |
---|---|---|---|
Nina Hernitschek | 1 | 0 | 0.34 |
Hans-Walter Rix | 2 | 0 | 0.34 |
Branimir Sesar | 3 | 0 | 0.34 |
Edward F. Schlafly | 4 | 0 | 0.34 |