CyberinfraV1, Main, Exploration, bibRecord, 000A85

Pixel-Level Calibration in the Kepler Science Operations Center Pipeline

Identifieur interne : 000A85 ( Main/Exploration ); précédent : 000A84; suivant : 000A86

Pixel-Level Calibration in the Kepler Science Operations Center Pipeline

Auteurs : Elisa V. Quintana [États-Unis] ; Jon M. Jenkins [États-Unis] ; Bruce D. Clarke [États-Unis] ; Hema Chandrasekaran [États-Unis] ; Joseph D. Twicken [États-Unis] ; Sean D. Mccauliff [États-Unis] ; Miles T. Cote [États-Unis] ; Todd C. Klaus [États-Unis] ; Christopher Allen [États-Unis] ; Douglas A. Caldwell [États-Unis] ; Stephen T. Bryson [États-Unis]

Source :

Proceedings of SPIE, the International Society for Optical Engineering [ 0277-786X ] ; 2010.

RBID : Pascal:11-0006837

Descripteurs français

Pascal (Inist)
- Processeur pipeline, Traitement pipeline, Série temporelle, Vol, Spationef, Artefact, Métrique, Archive, Etalonnage, Réduction donnée, Erreur systématique, Télescope, Astrophysique, Astronomie, ..
Wicri :
- topic : Vol, Astronomie.

English descriptors

KwdEn :
- Archive, Artefact, Astronomy, Astrophysics, Bias, Calibration, Data reduction, Flight, Metric, Pipeline processing, Pipeline processor, Spacecraft, Telescope, Time series.

Abstract

We present an overview of the pixel-level calibration of flight data from the Kepler Mission performed within the Kepler Science Operations Center Science Processing Pipeline. This article describes the calibration (CAL) module, which operates on original spacecraft data to remove instrument effects and other artifacts that pollute the data. Traditional CCD data reduction is performed (removal of instrument/detector effects such as bias and dark current), in addition to pixel-level calibration (correcting for cosmic rays and variations in pixel sensitivity), Kepler-specific corrections (removing smear signals which result from the lack of a shutter on the photometer and correcting for distortions induced by the readout electronics), and additional operations that are needed due to the complexity and large volume of flight data. CAL operates on long (˜30 min) and short (˜1 min) sampled data, as well as full-frame images, and produces calibrated pixel flux time series, uncertainties, and other metrics that are used in subsequent Pipeline modules. The raw and calibrated data are also archived in the Multi-mission Archive at Space Telescope at the Space Telescope Science Institute for use by the astronomical community.

Affiliations:

Links toward previous steps (curation, corpus...)

to stream PascalFrancis, to step Corpus: 000077
to stream PascalFrancis, to step Curation: 000168
to stream PascalFrancis, to step Checkpoint: 000091
to stream Main, to step Merge: 000A90
to stream Main, to step Curation: 000A85

Le document en format XML

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<term>Artefact</term>
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<term>Astrophysics</term>
<term>Bias</term>
<term>Calibration</term>
<term>Data reduction</term>
<term>Flight</term>
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<term>Pipeline processor</term>
<term>Spacecraft</term>
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<term>Artefact</term>
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<term>Archive</term>
<term>Etalonnage</term>
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<term>Erreur systématique</term>
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<front><div type="abstract" xml:lang="en">We present an overview of the pixel-level calibration of flight data from the Kepler Mission performed within the Kepler Science Operations Center Science Processing Pipeline. This article describes the calibration (CAL) module, which operates on original spacecraft data to remove instrument effects and other artifacts that pollute the data. Traditional CCD data reduction is performed (removal of instrument/detector effects such as bias and dark current), in addition to pixel-level calibration (correcting for cosmic rays and variations in pixel sensitivity), Kepler-specific corrections (removing smear signals which result from the lack of a shutter on the photometer and correcting for distortions induced by the readout electronics), and additional operations that are needed due to the complexity and large volume of flight data. CAL operates on long (˜30 min) and short (˜1 min) sampled data, as well as full-frame images, and produces calibrated pixel flux time series, uncertainties, and other metrics that are used in subsequent Pipeline modules. The raw and calibrated data are also archived in the Multi-mission Archive at Space Telescope at the Space Telescope Science Institute for use by the astronomical community.</div>
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<tree><country name="États-Unis"><region name="Californie"><name sortKey="Quintana, Elisa V" sort="Quintana, Elisa V" uniqKey="Quintana E" first="Elisa V." last="Quintana">Elisa V. Quintana</name>
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<name sortKey="Allen, Christopher" sort="Allen, Christopher" uniqKey="Allen C" first="Christopher" last="Allen">Christopher Allen</name>
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<name sortKey="Chandrasekaran, Hema" sort="Chandrasekaran, Hema" uniqKey="Chandrasekaran H" first="Hema" last="Chandrasekaran">Hema Chandrasekaran</name>
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<name sortKey="Jenkins, Jon M" sort="Jenkins, Jon M" uniqKey="Jenkins J" first="Jon M." last="Jenkins">Jon M. Jenkins</name>
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<name sortKey="Mccauliff, Sean D" sort="Mccauliff, Sean D" uniqKey="Mccauliff S" first="Sean D." last="Mccauliff">Sean D. Mccauliff</name>
<name sortKey="Twicken, Joseph D" sort="Twicken, Joseph D" uniqKey="Twicken J" first="Joseph D." last="Twicken">Joseph D. Twicken</name>
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Pixel-Level Calibration in the Kepler Science Operations Center Pipeline

Pixel-Level Calibration in the Kepler Science Operations Center Pipeline

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