EPJ Web of Conferences
Volume 47, 2013Hot Planets and Cool Stars
|Number of page(s)||4|
|Section||Other Transit Surveys|
|Published online||25 April 2013|
The Pan-STARRS1 Planet Survey: Overview and first results
1 University Observatory Munich, Scheinerstrasse 1, 81679 München, Germany
2 Max-Planck-Institute for Extraterrestrial Physics, Giessenbachstrasse, 85748 Garching, Germany
3 Max-Planck-Institute for Astronomy, Königstuhl 17, 69117 Heidelberg, Germany
4 University of Exeter, Stocker Road, Exeter EX4 4QL, UK
a e-mail: firstname.lastname@example.org
The Pan-STARRS1 Planet Survey (Pan-Planets) is a search for transiting extra-solar planets in the Galactic disk with a focus on planets around M-dwarfs and White dwarfs. The large field of view of the Pan-STARRS1 camera enables us to monitor ∼50 000 M-dwarfs and ∼5 000 White dwarfs brighter than iP1 = 18 in seven fields. We give a description of the science goals and observating strategy and present some early results from the first two observing campaigns conducted in 2010 and 2011.
© Owned by the authors, published by EDP Sciences, 2013
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 2.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.