Hostname: page-component-8448b6f56d-42gr6 Total loading time: 0 Render date: 2024-04-16T06:47:20.866Z Has data issue: false hasContentIssue false

Searching for Ultracool Companions with NICI

Published online by Cambridge University Press:  26 May 2016

C. Ftaclas
Affiliation:
Institute for Astronomy, Univ. of Hawaii, 2680 Woodlawn Dr., Honolulu, HI 96822
E. L. Martín
Affiliation:
Institute for Astronomy, Univ. of Hawaii, 2680 Woodlawn Dr., Honolulu, HI 96822
D. Toomey
Affiliation:
IfA-Hilo and Mauna Kea Infrared

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We present to the brown dwarf community the Near Infrared Coronographic Imager (NICI), which is being built for installation in 2005 on the Gemini South Telescope. NICI's dual channel architecture and dedicated AO system are designed to permit deep circumstellar discrimination of faint sources where some spectral key can be used to get a simultaneous estimate of the background. One of the principal science goals of NICI is to search for ultracool companions to stars and brown dwarfs.

Type
Part 9. Future Prospects
Copyright
Copyright © Astronomical Society of the Pacific 2001 

References

Close, L. M., et al. 2002, ApJ, 567, L53 CrossRefGoogle Scholar
Lane, B. F., Zapatero Osorio, M. R., Britton, M. C., Martín, E. L., & Kulkarni, S. R. 2001, ApJ, 560, 390 Google Scholar
Liu, M. C. et al. 2002, ApJ, 571, 519 CrossRefGoogle Scholar
Martín, E. L., Koresko, C. D., Kulkarni, S. R., Lane, B. F., & Wizinowich, P. L. 2000, ApJ, 529, L37 CrossRefGoogle Scholar
Potter, D., Martín, E. L., Cushing, M. C., Baudoz, P., Brandner, W., Guyon, O., & Neuhäuser, R. 2002, ApJ, 567, L133 CrossRefGoogle Scholar
Toomey, D. & Ftaclas, C. 2003, SPIE, in press Google Scholar
Vogt, S. S., Butler, P. R., Marcy, G. W., Fischer, D. A., Pourbaix, D., Apps, K., & Laughlin, G. 2002, ApJ, 568, 352 Google Scholar