TY - JOUR
T1 - Fourstar
T2 - The near-infrared imager for the 6.5 m baade telescope at las campanas observatory
AU - Persson, S. E.
AU - Murphy, D. C.
AU - Smee, S.
AU - Birk, C.
AU - Monson, A. J.
AU - Uomoto, A.
AU - Koch, E.
AU - Shectman, S.
AU - Barkhouser, R.
AU - Orndorff, J.
AU - Hammond, R.
AU - Harding, A.
AU - Scharfstein, G.
AU - Kelson, D.
AU - Marshall, J.
AU - McCarthy, P. J.
PY - 2013/6
Y1 - 2013/6
N2 - The FourStar Infrared Camera is a 4 K×4 K near-infrared (1.0-2.4 μm) imager built for the Magellan 6.5 m Baade Telescope at Las Campanas Observatory, Chile. FourStar has an all-refractive optical system, four HAWAII-2RG detectors, and Teledyne electronics. The pixel scale of 0:159″ pixel-1 produces a 10:80 × 10:80 field of view. Ten filters are available across the Y, J,H, andKs bands.We present the optical, mechanical, thermal, electronic, and software design choices and their associated engineering implementations. The detector readout electronics, control system, and the automatic data acquisition hardware are also described. Laboratory and onsky performance data are presented. FourStar has excellent image quality, easily meeting the requirement of critically sampling the median seeing disk. The throughput is ≈0:5-0:6 across its wavelength coverage. Some early science results are presented.
AB - The FourStar Infrared Camera is a 4 K×4 K near-infrared (1.0-2.4 μm) imager built for the Magellan 6.5 m Baade Telescope at Las Campanas Observatory, Chile. FourStar has an all-refractive optical system, four HAWAII-2RG detectors, and Teledyne electronics. The pixel scale of 0:159″ pixel-1 produces a 10:80 × 10:80 field of view. Ten filters are available across the Y, J,H, andKs bands.We present the optical, mechanical, thermal, electronic, and software design choices and their associated engineering implementations. The detector readout electronics, control system, and the automatic data acquisition hardware are also described. Laboratory and onsky performance data are presented. FourStar has excellent image quality, easily meeting the requirement of critically sampling the median seeing disk. The throughput is ≈0:5-0:6 across its wavelength coverage. Some early science results are presented.
UR - http://www.scopus.com/inward/record.url?scp=84879469724&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=84879469724&partnerID=8YFLogxK
U2 - 10.1086/671164
DO - 10.1086/671164
M3 - Article
AN - SCOPUS:84879469724
SN - 0004-6280
VL - 125
SP - 654
EP - 682
JO - Publications of the Astronomical Society of the Pacific
JF - Publications of the Astronomical Society of the Pacific
IS - 928
ER -