Hostname: page-component-cd9895bd7-dk4vv Total loading time: 0 Render date: 2024-12-25T04:17:03.740Z Has data issue: false hasContentIssue false
  • English
  • Français

Pan-STARRS1 as pilot-survey for panoptic time-domain science

Published online by Cambridge University Press:  30 May 2017

Nina Hernitschek ,
Hans-Walter Rix ,
Branimir Sesar  and
Edward F. Schlafly
Nina Hernitschek
Affiliation:
Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany email: [email protected]
Hans-Walter Rix
Affiliation:
Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany email: [email protected]
Branimir Sesar
Affiliation:
Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany email: [email protected]
Edward F. Schlafly
Affiliation:
UC Berkeley, Berkeley, CA 94720-5800
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

For examining possibilities and challenges in doing science with multi-band and non-simultaneous data from upcoming surveys like LSST, the Pan-STARRS1 (PS1) 3π 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 3π 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.

Keywords

methods: data analysismethods: statisticalcatalogssurveys(stars: variables:) Cepheidsstars: variables: other(galaxies:) quasars: general
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S325: Astroinformatics , October 2016 , pp. 118 - 121
Copyright
Copyright © International Astronomical Union 2017 

References

Chambers, K. 2011, AAS Meeting Abstracts, 218, 113.01Google Scholar
Hernitschek, N., Rix, H.-W., Bovy, J., et al. 2016, ApJ, 817, 1, 73 CrossRefGoogle Scholar
Kaiser, N., Burgett, W., Chambers, K., et al. 2010, Proc. SPIE, 77330EGoogle Scholar
Kozłowski, S., Kochanek, Ch. S., Udalski, A., et al. 2010, ApJ, 708, 2, 927 Google Scholar
LSST Science Book, Version 2.0 2009, arXiv:0912.0201 Google Scholar
Nikutta, R., Hunt-Walker, N., Nenkova, M., et al. 2014, MNRAS, 442, 4, 3361 Google Scholar
Schlafly, E. F., Green, G., Finkbeiner, D. F., et al. 2014, ApJ, 789, 1, 15 Google Scholar
Schmidt, K. B., Marshall, P. J., Rix, H.-W., et al. 2000, ApJ, 714, 2, 1194 CrossRefGoogle Scholar
Schneider, D. P., Hall, P. B., Richards, G. T., et al. 2007, ApJ, 134, 1, 102 Google Scholar
Sesar, B., Ivezić, Ž., & Grammer, S. H. 2000, ApJ, 708, 1, 717 Google Scholar