Solar Wind Electrons Alphas and Protons (SWEAP) Science Operations Center initial design and implementation

2014 ◽  
Author(s):  
Kelly E. Korreck ◽  
Justin C. Kasper ◽  
Anthony W. Case ◽  
Peter Daigneau ◽  
Jay A. Bookbinder ◽  
...  
Keyword(s):  
Solar Wind ◽  
Design And Implementation ◽  
Initial Design ◽  
Science Operations ◽  
Operations Center

The MESSENGER Science Operations Center

2007 ◽  
Vol 131 (1-4) ◽  
pp. 601-623 ◽  
Author(s):  
Helene L. Winters ◽  
Deborah L. Domingue ◽  
Teck H. Choo ◽  
Raymond Espiritu ◽  
Christopher Hash ◽  
...  
Keyword(s):  
Science Operations ◽  
Operations Center

Virtual Science Operations Center: Concept, Deployment and Operations

2014 ◽  
Author(s):  
Ravil Nazirov ◽  
Oleg Batanov ◽  
Vladimir Nazarov ◽  
Fedor Korotkov ◽  
Natan Eysmont ◽  
...  
Keyword(s):  
Science Operations ◽  
Operations Center

scholarly journals The Kepler Science Operations Center pipeline framework extensions

2010 ◽  
Author(s):  
Todd C. Klaus ◽  
Miles T. Cote ◽  
Sean McCauliff ◽  
Forrest R. Girouard ◽  
Bill Wohler ◽  
...  
Keyword(s):  
Science Operations ◽  
Operations Center

scholarly journals TESS Data for Asteroseismology: Light-curve Systematics Correction

2021 ◽  
Vol 257 (2) ◽  
pp. 53
Author(s):  
Mikkel N. Lund ◽  
Rasmus Handberg ◽  
Derek L. Buzasi ◽  
Lindsey Carboneau ◽  
Oliver J. Hall ◽  
...  
Keyword(s):  
Light Curves ◽  
Intrinsic Variability ◽  
Space Telescopes ◽  
Noise Sources ◽  
Full Spectrum ◽  
Stellar Oscillations ◽  
Science Operations ◽  
Wide Range ◽  
Noise Statistics ◽  
Operations Center

Abstract Data from the Transiting Exoplanet Survey Satellite (TESS) have produced of the order of one million light curves at cadences of 120 s and especially 1800 s for every ∼27 day observing sector during its two-year nominal mission. These data constitute a treasure trove for the study of stellar variability and exoplanets. However, to fully utilize the data in such studies a proper removal of systematic-noise sources must be performed before any analysis. The TESS Data for Asteroseismology group is tasked with providing analysis-ready data for the TESS Asteroseismic Science Consortium, which covers the full spectrum of stellar variability types, including stellar oscillations and pulsations, spanning a wide range of variability timescales and amplitudes. We present here the two current implementations for co-trending of raw photometric light curves from TESS, which cover different regimes of variability to serve the entire seismic community. We find performance in terms of commonly used noise statistics meets expectations and is applicable to a wide range of intrinsic variability types. Further, we find that the correction of light curves from a full sector of data can be completed well within a few days, meaning that when running in steady state our routines are able to process one sector before data from the next arrives. Our pipeline is open-source and all processed data will be made available on the websites of the TESS Asteroseismic Science Operations Center and the Mikulski Archive for Space Telescopes.

scholarly journals AMS data production facilities at science operations center at CERN

2017 ◽  
Vol 898 ◽  
pp. 082019
Author(s):  
V Choutko ◽  
A Egorov ◽  
A Eline ◽  
B Shan
Keyword(s):  
Science Operations ◽  
Data Production ◽  
Operations Center ◽  
Production Facilities

Initial Design and Implementation of a Space Quadruped Crawling Robot Prototype

2021 ◽  
Author(s):  
Zhengyou Xie ◽  
Xinlong Chen ◽  
Dake Chen ◽  
Weichun Chen ◽  
Yangyang Zhao
Keyword(s):  
Design And Implementation ◽  
Initial Design
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