Feng, FaboButler, R PaulVogt, Steven SHolden, BradfordRui, Yicheng
ABSTRACT: With its near-to-mid-infrared high-contrast imaging capabilities, JWST is ushering us into a golden age of directly imaging Jupiter-like planets. As the two closest cold Jupiters, ε Ind A b and ε Eridani b have sufficiently wide orbits and adequate infrared emissions to be detected by JWST. To detect more Jupiter-like planets for direct i...
Ade, P. A. R.Aghanim, N.Armitage-Caplan, C.Arnaud, M.Ashdown, M.Atrio-Barandela, F.Aumont, J.Baccigalupi, C.Banday, A. J.Barreiro, R. B.
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We describe the detection, interpretation, and removal of the signal resulting from interactions of high energy particles with the \Planck\ High Frequency Instrument (HFI). There are two types of interactions: heating of the 0.1\,K bolometer plate; and glitches in each detector time stream. The transient responses to detector glitch shapes are not ...