pith. sign in

arxiv: 1405.7350 · v2 · pith:EZZHRPNCnew · submitted 2014-05-28 · 🌌 astro-ph.SR

NEOWISE-R Observation of the Coolest Known Brown Dwarf

classification 🌌 astro-ph.SR
keywords wiseneowise-rbrowndwarfmotionproperveryarcsec
0
0 comments X p. Extension
pith:EZZHRPNC Add to your LaTeX paper What is a Pith Number?
\usepackage{pith}
\pithnumber{EZZHRPNC}

Prints a linked pith:EZZHRPNC badge after your title and writes the identifier into PDF metadata. Compiles on arXiv with no extra files. Learn more

read the original abstract

The Wide-field Infrared Survey Explorer (WISE) spacecraft has been reactivated as NEOWISE-R to characterize and search for Near Earth Objects. The brown dwarf WISE J085510.83-071442.5 has now been reobserved by NEOWISE-R, and we confirm the results of Luhman (2014b), who found a very low effective temperature ($\approx 250$ K), a very high proper motion (8.1 +/- 0.1 arcsec/yr) , and a large parallax (454 +/- 45 mas). The large proper motion has separated the brown dwarf from the background sources that influenced the 2010 WISE data, allowing a measurement of a very red WISE color of W1-W2 $> 3.9$ mag. A re-analysis of the 2010 WISE astrometry using only the W2 band, combined with the new NEOWISE-R 2014 position, gives an improved parallax of 448 +/- 33 mas and proper motion of 8.08 +/- 0.05\; arcsec/yr. These are all consistent with Luhman (2014b).

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.