Observing Period: 20 Jun 2009 - 16 Sep 2009
Release Date: 02 Feb 2011
Fig 1: The Quarter 2 light curve of KIC 6541920, also designated Kepler 11. This
system shows evidence for 6 transiting planets as described in
Lissauer
etal (2011). Gaps in the time series
occur at the monthly downlinks, when the spacecraft is not taking data. This light curve
has been processed through pipeline module PDC, in which
systematic temporal trends were removed.
The Kepler mission has released the first full quarter of data taken
by the spacecraft to the community. Quarter 2 contains photometry obtained during an 88-day
period from 20 June to 16 September 2009. All Q2 data have been released except for some Q2
Guest Observer targets due for release in April 2011, in accordance with the
2009 Kepler NASA Research Announcement. Calibrated data for individual sources can be
downloaded from the Multi-mission Archive at the Space Telescope Science Institute
Kepler archive using the
Kepler Data Search and
Retrieval form.
The Q2 data were reprocessed using Kepler Pipeline version 6.2 prior to
archiving. Both the light curves and target pixels files are now available. The target
pixel files contain the calibrated pixel images for each cadence observation, and permit
the user to customize their light curves. Investigators must read the
Release Notes #7 in order to understand the accuracy and limits of this specific data
release. Also now available for greater understanding of the Kepler data is the
Data Characteristics Handbook, which describes the phenomena
found in the data by the Kepler Data Analysis Working Group.
The Q2 data contains light curves for 166,373 stars; most are
late-type main sequence stars, brighter than 16th magnitude sampled with 30-minute cadence.
On a 1-minute cadence 1417 stars were observed for 1 month, 5 for two months, and 70 for all
three months during the quarter.
The motivation for this data release is to support the community in exploiting
the 2011 NASA
Astrophysics Data Analysis Program (ADAP),
a funding opportunity which supports the analysis and interpretation of data in the public
archives. Scientists will have access to the Q0, Q1
and Q2 light curve data and approximately 30 full-frame
images (FFIs) at the time that ADAP proposals are due on 13 May 2011.
New users of the MAST archive are requested to
register before downloading data.
Please direct questions concerning the Q2 data to the
.