A Physical Model-based Correction for Charge Traps in the Hubble Space Telescope’s Wide Field Camera 3 Near-IR Detector and Its Applications to Transiting Exoplanets and Brown Dwarfs

A Physical Model-based Correction for Charge Traps in the Hubble Space Telescope’s Wide Field Camera 3 Near-IR Detector and Its Applications to Transiting Exoplanets and Brown Dwarfs

The Hubble Space Telescope Wide Field Camera 3 (WFC3) near-IR channel is extensively used in time-resolved observations, especially for transiting exoplanet spectroscopy as well as. brown dwarf and directly imaged exoplanet rotational phase mapping. The ramp effect is the dominant source of systemat...

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Bibliographic Details
Main Authors: Zhou, Yifan, Apai, Dániel, Lew, Ben W. P., Schneider, Glenn
Other Authors: Univ Arizona, Dept Astron, Steward Observ
Language:en
Published: IOP PUBLISHING LTD 2017
Subjects:
brown dwarfs
instrumentation: detectors
planets and satellites: atmospheres
Online Access:http://hdl.handle.net/10150/625388
http://arizona.openrepository.com/arizona/handle/10150/625388

Internet

http://hdl.handle.net/10150/625388
http://arizona.openrepository.com/arizona/handle/10150/625388

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