SIMBAD references

2010PASP..122..162B - Publ. Astron. Soc. Pac., 122, 162-200 (2010/February-0)

Imaging young giant planets from ground and space.

BEICHMAN C.A., KRIST J., TRAUGER J.T., GREENE T., OPPENHEIMER B., SIVARAMAKRISHNAN A., DOYON R., BOCCALETTI A., BARMAN T.S. and RIEKE M.

Abstract (from CDS):

High-contrast imaging can find and characterize gas giant planets around nearby young stars and the closest M stars, complementing radial velocity and astrometric searches by exploring orbital separations inaccessible to indirect methods. Ground-based coronagraphs are already probing within 25 AU of nearby young stars to find objects as small as. This paper contrasts near-term and future ground-based capabilities with high-contrast imaging modes of the James Webb Space Telescope (JWST). Monte Carlo modeling reveals that JWST can detect planets with masses as small as across a broad range of orbital separations. We present new calculations for planet brightness as a function of mass and age for specific JWST filters and extending to.

Abstract Copyright:

Journal keyword(s): Extrasolar Planets

VizieR on-line data: <Available at CDS (J/PASP/122/162): stars.dat model.dat detec.dat>

Simbad objects: 105

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2019.10.22-06:48:33

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