Studies of Expolanets and Solar Systems with SPICA

(10) Rutherford Appleton Laboratory); (2) National Astronomical Observatory of Japan; (3) Japan Aerospace Exploration Agency; (4) Osaka University; (5) Kanagawa University; (6) Ibaraki University; (7) University of Tokyo; (8) Centro de Astrobiologia (CSIC-INTA); (9) Cardiff University; Academia Sinica

REVIEW

Studies of Expolanets and Solar Systems with SPICA

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 0911.3974 v1 pith:JOCO4GEL submitted 2009-11-20 astro-ph.IM astro-ph.EP

Michihiro Takami (1) , Motohide Tamura (2) , Keigo Enya (3) , Takafumi Ootsubo (3) , Misato Fukagawa (4) , Mitsuhiko Honda (5) , Yoshiko Okamoto (6) , Shigehisa Sako (7)

show 19 more authors

Takuya Yamashita (2) Sunao Hasegawa (3) Hirokazu Kataza (3) Hideo Matsuhara (3) Takao Nakagawa (3) Javier R. Goicoechea (8) Kate Isaak (9) Bruce Swinyard (10) ((1) Institute of Astronomy Astrophysics Academia Sinica (2) National Astronomical Observatory of Japan (3) Japan Aerospace Exploration Agency (4) Osaka University (5) Kanagawa University (6) Ibaraki University (7) University of Tokyo (8) Centro de Astrobiologia (CSIC-INTA) (9) Cardiff University (10) Rutherford Appleton Laboratory)

This is my paper · ORCID

classification astro-ph.IMastro-ph.EP

keywords infraredinstrumentationproposedsolarspicastudiessuperiortelescope

verification ladder T0 review T1 audit T2 compute T3 formal

Signed reviews

No signed human review yet.

0 comments

read the original abstract

The SPace Infrared telescope for Cosmology and Astrophysics (SPICA) is a proposed mid-to-far infrared (4-200 um) astronomy mission, scheduled for launch in 2017. A single, 3.5m aperture telescope would provide superior image quality at 5-200 um, and its very cold (~5 K) instrumentation would provide superior sensitivity in the 25-200 um wavelength regimes. This would provide a breakthrough opportunity for studies of exoplanets, protoplanetary and debris disk, and small solar system bodies. This paper summarizes the potential scientific impacts for the proposed instrumentation.

Discussion (0). Continue with ORCID to comment.

Pith tools