James R. Graham's Home Page


CURRENT PROJECTS

The Mighty Keck Telescopes

 

NIRSPEC


Adaptive Optics

IRCAL is a high resolution IR camera for the Lick Adaptive Optics system. This is a project with Jamie Lloyd, Scott Severson (UCO, Lick) and Bruce Macintosh (LLNL).
 
 

The Livermore sodium laser guide-star launched from the Lick 3-m telescope.


Astronomy From a Jet Plane - SOFIA


AY 122:  Undergraduate Infrared Lab

This infrared image of NGC 2024 from Leuschner Observatory was taken with the undergraduate IR camera. Red corresponds to K-band (2.2 microns), green is H-band (1.6 microns), and blue is J-band (1.2 microns).  NGC 2024 is a region of massive star formation in the Orion molecular cloud. Heavy foreground extinction due to interstellar dust reddens many of the stars in this cluster. Even at 2.2 microns, where the extinction is one tenth of that at visible wavelengths, prominent dark dust lanes are apparent. The field of view is 5.7 arc minutes x 5.7 arc minutes. The exposure time is 80 seconds per filter and the limiting magnitude is ~ 14.2 at J and ~ 13 at K. Construction of the infrared camera was made possible by funds from the National Science Foundation and Rockwell International and described by Graham & Treffers (2001, Pub. Astr. Soc. Pac., 113, 607) . The data were reduced using computers donated by Sun Microsystems.
 


Recent Publications and Preprints



AY 202: Astrophysical Gas Dynamics



The Next Generation Space Telescope & IFIRS.


ROSAT Newsletter article describing the HRI Cygnus Loop survey

ROSAT LINKS



Handy Calculators



Dr James R. Graham
Professor of Astronomy
601 Campbell Hall
University of California
Berkeley CA 94720-3411
 

tel:  (510) 642-8283
fax: (510) 642-3411


Click here to return to the Berkeley Astronomy Department home page. 

Last updated March 2006