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Recent progress at the Keck Interferometer: operations and V 2 science

2008; SPIE; Volume: 7013; Linguagem: Inglês

10.1117/12.788070

1996-756X

Sam Ragland, Peter Wizinowich, Rachel Akeson, M. M. Colavita, E. Appleby, B. Berkey, A. J. Booth, Andrew P. Cooper, S. Crawford, W. Dahl, C. Felizardo, Jean Garcia-Gathright, J. Gathright, J. Herstein, M. Hrynevych, C. Koresko, R. Ligon, D. Medeiros, Bertrand Mennesson, R. Millan‐Gabet, D.R.O. Morrison, Chris Paine, B. Parvin, T. Panteleeva, Eugene Serabyn, B. A. Smith, K. Summers, Kevin Tsubota, C. Tyau, Ed Wetherell, J. Woillez,

Astronomy and Astrophysical Research

The Keck Interferometer combines the two 10m diameter Keck telescopes for near-infrared fringe visibility, and mid-infrared nulling observations. We report on recent progress with an emphasis on new visibility observing capabilities, operations improvements for visibility and nulling, and on recent visibility science. New visibility observing capabilities include a grism spectrometer for higher spectral resolution. Recent improvements include a new AO output dichroic for increased infrared light throughput, and the installation of new wave-front controllers on both Keck telescopes. We also report on recent visibility results in several areas including (1) young stars and their circumstellar disks, (2) pre-main sequence star masses, and (3) Circumstellar environment of evolved stars. Details on nuller instrument and nuller science results, and the ASTRA phase referencing and astrometry upgrade, are presented in more detail elsewhere in this conference.