Finding, characterizing and classifying variable sources in multi-epoch sky surveys: QSOs and RR Lyrae in PS1 3π data
In area and depth, the Pan-STARRS1 (PS1) 3$\pi$ survey is unique among many-epoch, multi-band surveys and has enormous potential for all-sky identification of variable sources. PS1 has observed the sky typically seven times in each of its five bands (
Gespeichert in:
| Hauptverfasser: | , |
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| Dokumenttyp: | Article (Journal) Kapitel/Artikel |
| Sprache: | Englisch |
| Veröffentlicht: |
2015
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| In: |
Arxiv
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| Online-Zugang: | Verlag, kostenfrei, Volltext: http://arxiv.org/abs/1511.05527
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| Verfasserangaben: | Nina Hernitschek, Edward F. Schlafly, Branimir Sesar, Hans-Walter Rix, David W. Hogg, Zeljko Ivezic, Eva K. Grebel, Eric F. Bell, Nicolas F. Martin, W.S. Burgett, H. Flewelling, K.W. Hodapp, N. Kaiser, E.A. Magnier, N. Metcalfe, R.J. Wainscoat, C. Waters |
MARC
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| 520 | |a In area and depth, the Pan-STARRS1 (PS1) 3$\pi$ survey is unique among many-epoch, multi-band surveys and has enormous potential for all-sky identification of variable sources. PS1 has observed the sky typically seven times in each of its five bands ( | ||
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