Infrared Astronomy with Arrays
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The idea for another conference on the theme of Infrared Astronomy with Arrays actually goes back to March 1987. At a party held in my home at the end of the Hilo conference, excitement was running high and everyone present was in favor of another meeting. I recall suggesting to Al Fowler that the next meeting could be in Tucson. Despite Al's reply to the effect that Hawaii was a much nicer location, a meeting was held in Tucson three years later. That meeting focussed more on the astrophysics which had been accomplished with the detectors, rather than on techniques and methods. However, it…mehr

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Produktbeschreibung
The idea for another conference on the theme of Infrared Astronomy with Arrays actually goes back to March 1987. At a party held in my home at the end of the Hilo conference, excitement was running high and everyone present was in favor of another meeting. I recall suggesting to Al Fowler that the next meeting could be in Tucson. Despite Al's reply to the effect that Hawaii was a much nicer location, a meeting was held in Tucson three years later. That meeting focussed more on the astrophysics which had been accomplished with the detectors, rather than on techniques and methods. However, it was already apparent in February of 1990 that a new generation of larger m arrays would soon supersede the 64x64 class of devices and so, having just moved from the UK Infrared Telescope unit in Hawaii to join with Eric Becklin in his move to UCLA, it seemed to me that another Hilo-style conference was appropriate, and Eric agreed.
Autorenporträt
Dr. McLean has been a member of the faculty at UCLA and Director of the UCLA Infrared Laboratory for Astrophysics since 1989. He has served as Vice Chair for Astronomy since 2009. The IR Lab at UCLA is well-known for the development of many astronomical instruments for the Keck Observatory and other telescopes. Dr. McLean is one of the world s leading authorities on the application of electronic imaging systems to advanced astronomical instrumentation. He has written over 300 articles and his current book, Electronic Imaging in Astronomy: detectors and instrumentation, published by Springer is in its second edition.
Dr. McLean received his BSc(Hons) in Physics & Astronomy and his PhD in Astronomy from Glasgow University (UK) in 1971 and 1974 respectively. While a member of staff at the Royal Observatory Edinburgh from 1979-1989 he developed the first CCD-based imaging spectro-polarimeter and the first facility-class camera for the 3.8-m UK Infrared Telescope to use infrared arrays. Since joining UCLA, his lab has delivered or assisted in all of the currently operational infrared instruments at the W. M. Keck Observatory. Dr. McLean was the principal investigator for the NIRSPEC and MOSFIRE instruments at Keck, the twin-channel infrared camera at Lick Observatory and the FLITECAM instrument for NASA s Stratospheric Observatory for Infrared Astronomy. He served on the Science Steering Committee for the W. M. Keck Observatory for ten years and he is an Associate Director of the University of California Observatories. Dr. McLean is a former president of IAU Commission 25 (Photometry and Polarimetry) and a former president of IAU Commission 9 (Instrumentation and Techniques). He is a member of the American Astronomical Society (AAS) and the Society of Professional Instrument Engineers (SPIE). His research interests are broad. From his early career he is known for many discoveries involving the intrinsic polarization of starlight. Currently, his main research

involves the study of sub-stellar mass objects (brown dwarfs), star forming regions, the galactic center, and star-formation in high-redshift galaxies. His web site bdssarchive.org provides a public data base of infrared spectra for low-mass stars and brown dwarfs.