| | |
| | |
Stat |
Members: 3645 Articles: 2'506'133 Articles rated: 2609
27 April 2024 |
|
| | | |
|
Article overview
| |
|
Spitzer Photometry of WISE-Selected Brown Dwarf and Hyper-Luminous Infrared Galaxy Candidates | Roger L. Griffith
; J. Davy Kirkpatrick
; Peter R. M. Eisenhardt
; Christopher R. Gelino
; Michael C. Cushing
; Dominic Benford
; Andrew Blain
; Carrie R. Bridge
; Martin Cohen
; Roc M. Cutri
; Emilio Donoso
; Thomas H. Jarrett
; Carol Lonsdale
; Gregory Mace
; A. Mainzer
; Ken Marsh
; Deborah Padgett
; Sara Petty
; Michael E. Ressler
; Michael F. Skrutskie
; Spencer A. Stanford
; Daniel Stern
; Chao-Wei Tsai
; Edward L. Wright
; Jingwen Wu
; Lin Yan
; | Date: |
10 Sep 2012 | Abstract: | We present Spitzer 3.6 and 4.5 $mu$m photometry and positions for a sample
of 1510 brown dwarf candidates identified by the WISE all-sky survey. Of these,
166 have been spectroscopically classified as objects with spectral types M(1),
L(7), T(146), and Y(12); Sixteen other objects are non-(sub)stellar in nature.
The remainder are most likely distant L and T dwarfs lacking spectroscopic
verification, other Y dwarf candidates still awaiting follow-up, and assorted
other objects whose Spitzer photometry reveals them to be background sources.
We present a catalog of Spitzer photometry for all astrophysical sources
identified in these fields and use this catalog to identify 7 fainter (4.5
$mu$m $sim$ 17.0 mag) brown dwarf candidates, which are possibly wide-field
companions to the original WISE sources. To test this hypothesis, we use a
sample of 919 Spitzer observations around WISE-selected high-redshift
hyper-luminous infrared galaxy (HyLIRG) candidates. For this control sample we
find another 6 brown dwarf candidates, suggesting that the 7 companion
candidates are not physically associated. In fact, only one of these 7 Spitzer
brown dwarf candidates has a photometric distance estimate consistent with
being a companion to the WISE brown dwarf candidate. Other than this there is
no evidence for any widely separated ($>$ 20 AU) ultra-cool binaries. As an
adjunct to this paper, we make available a source catalog of $sim$ 7.33
$ imes 10^5$ objects detected in all of these Spitzer follow-up fields for use
by the astronomical community. The complete catalog includes the Spitzer 3.6
and 4.5 $mu$m photometry, along with positionally matched $B$ and $R$
photometry from USNO-B; $J$, $H$, and $K_s$ photometry from 2MASS; and $W1$,
$W2$, $W3$, and $W4$ photometry from the WISE all-sky catalog. | Source: | arXiv, 1209.1855 | Services: | Forum | Review | PDF | Favorites |
|
|
No review found.
Did you like this article?
Note: answers to reviews or questions about the article must be posted in the forum section.
Authors are not allowed to review their own article. They can use the forum section.
browser Mozilla/5.0 AppleWebKit/537.36 (KHTML, like Gecko; compatible; ClaudeBot/1.0; +claudebot@anthropic.com)
|
| |
|
|
|
| News, job offers and information for researchers and scientists:
| |