TY - GEN
T1 - Narrow-angle astrometry with SUSI
AU - Kok, Yitping
AU - Ireland, Michael J.
AU - Robertson, J. Gordon
AU - Tuthill, Peter G.
AU - Warrington, Benjamin A.
AU - Tango, William J.
PY - 2014
Y1 - 2014
N2 - SUSI (Sydney University Stellar Interferometer) is currently being fitted with a 2nd beam combiner, MUSCA (Micro-arcsecond University of Sydney Companion Astrometry), for the purpose of narrow-angle astrometry. With an aim to achieve similar to 10 micro-arcseconds of angular resolution at its best, MUSCA allows SUSI to search for planets around bright binary stars, which are its primary targets. While the first beam combiner, PAVO (Precision Astronomical Visible Observations), is used to track stellar fringes during an observation, MUSCA will be used to measure separations of binary stars. MUSCA is a Michelson interferometer and its setup at SUSI will be described in this poster.
AB - SUSI (Sydney University Stellar Interferometer) is currently being fitted with a 2nd beam combiner, MUSCA (Micro-arcsecond University of Sydney Companion Astrometry), for the purpose of narrow-angle astrometry. With an aim to achieve similar to 10 micro-arcseconds of angular resolution at its best, MUSCA allows SUSI to search for planets around bright binary stars, which are its primary targets. While the first beam combiner, PAVO (Precision Astronomical Visible Observations), is used to track stellar fringes during an observation, MUSCA will be used to measure separations of binary stars. MUSCA is a Michelson interferometer and its setup at SUSI will be described in this poster.
UR - http://adsabs.harvard.edu/abs/2014ASPC..487..327K
M3 - Conference proceeding contribution
SN - 9781583818589
T3 - Astronomical Society of the Pacific conference series
SP - 327
EP - 329
BT - Resolving the future of astronomy with long-baseline interferometry
A2 - Creech-Eakman, Michelle J.
A2 - Guzik, Joyce A.
A2 - Stencel, Robert E.
PB - Astronomical Society of the Pacific
CY - San Francisco, CA
T2 - Conference on Resolving the Future of Astronomy with Long-Baseline Interferometry
Y2 - 28 March 2011 through 31 March 2011
ER -