Properties of Stars in the Subaru Deep Field | Zendy

M. Richmond | Zendy

AI Assistant Blog Pricing

Home ZAIA Blog

Open Access

Properties of Stars in the Subaru Deep Field

Author(s) -

M. Richmond

Publication year - 2005

Publication title -

publications of the astronomical society of japan

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 1.99

H-Index - 110

eISSN - 2053-051X

pISSN - 0004-6264

DOI - 10.1093/pasj/57.6.969

Subject(s) - physics , stars , hubble deep field , astrophysics , galaxy , stellar classification , astronomy , hubble space telescope

We investigate the properties of objects in the Subaru Deep Field (SDF),using public catalogs constructed from images in several optical passbands.Using a small subset of objects most likely to be stars, we construct a stellarlocus in three-dimensional color space. We then compare the position of allobjects relative to this locus to create larger samples of stars in the SDFwith rough spectral types. The number counts of stars defined in this way areconsistent with those of current models of the Galaxy.

The content you want is available to Zendy users.

Already have an account? Click here to sign in.

Having issues? You can contact us here

Accelerating Research