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The Kepler Pixel Response Function
Stephen T. Bryson, Peter Tenenbaum, Jon M. Jenkins et al., 2010.
What it's used for here
Defines the Kepler PRF models; the module 13 output 2 PRF (kplr13.2_2011265) was used to model stars A and B in the K2 pixels of HD 139139.
Cited by on this site 4 records
HD 139139, the "Random Transiter"
MYSThe mystery article
Cite it
Stephen T. Bryson, Peter Tenenbaum, Jon M. Jenkins, & et al. (2010). The Kepler Pixel Response Function. https://doi.org/10.1088/2041-8205/713/2/L97
@article{bryson2010kepler,
author = {Stephen T. Bryson} and {Peter Tenenbaum} and {Jon M. Jenkins} and {et al.},
title = {The Kepler Pixel Response Function},
year = {2010},
doi = {10.1088/2041-8205/713/2/L97}
}TY - JOUR TI - The Kepler Pixel Response Function AU - Stephen T. Bryson AU - Peter Tenenbaum AU - Jon M. Jenkins AU - et al. PY - 2010 DO - 10.1088/2041-8205/713/2/L97 ER -
et al.. “The Kepler Pixel Response Function.” 2010. https://doi.org/10.1088/2041-8205/713/2/L97.