PATTEN
 |

Astronomer
Harvard-Smithsonian CfA
Education
B.S. in Physics, 1986, Iowa State University
M.S. in Astrophysics, 1989, Iowa State University
Ph.D. in Astronomy, 1995, University of Hawaii
Contact Information
I am currently on a rotation as a Program Director in the Division of Astronomical Sciences at the National Science Foundation. Please contact me there as I no longer have a phone number or an office at the CfA (my e-mail still works though!).
National Science Foundation
Division of Astronomical Sciences
4201 Wilson Blvd
Arlington, VA 22230
(703) 292-4910
bpatten@cfa.harvard.edu
bpatten@nsf.gov
About
 |
I am currently on an Intergovernmental Personnel Act rotation as the Program Director for Education and Special Program as well as Program Director for Galactic Astronomy in the Division of Astronomical Sciences at the National Science Foundation. While I am at the NSF, I am still, technically, an employee of the Smithsonian Institution.
I have been an astronomer at the
Harvard-Smithsonian Center for Astrophysics since 1998. While I
am directly employed by the Smithsonian Institution's
Smithsonian
Astrophysical Observatory (SAO), I also have an appointment as
an Associate of the
Harvard College Observatory. My primary duties are to provide
support and conduct science programs as a member of the Spitzer
Space Telescope IRAC instrument team and (from 1998 - 2006) to
provide support for the SWAS mission.
For SWAS (the Submillimeter Wave Astronomy Satellite), I provided
mission operations and data analysis support for the mission at SAO.
I still act as the archive scientist now that the mission has been
completed, preparing and distributing SWAS
archival data products for the mission to the public access sites.
I also maintain the the SWAS WWW site at SAO.
For the Spitzer Space Telescope I carried out several In-Orbit
Checkout and Science Verification tasks for the Infrared Array Camera
(IRAC), an SAO project, following the Spitzer launch. I also act
as the scientific lead for several Spitzer Guaranteed Time Observer
science programs.
|
| |

Research Interests
 |
My primary research interests are in very low mass stars and brown
dwarfs and in gravitational microlensing. Brown dwarfs are objects of
sub-stellar mass made of highly
compressed hydrogen and helium (and a trace of other elements). These
objects are not massive enough to sustain nuclear fusion reactions in their
cores and thus are not considered stars, though they do glow from the heat
of their formation. Brown dwarfs may represent a kind of transition object
between stars and what we think of as planets and can probably tell us a
great deal about formation and fundamental nature of both. For gravitational
microlensing, I am interested specifically in determining the nature of the
lenses in the bone fide microlensing events seen towards the Large Magellanic
Cloud during the MACHO survey. The lenses can tell us a great deal about the
nature of the stucture of our home galaxy, the Milky Way, as well as providing
us with a probe of the contents of our galaxy's halo.
I am also interested in the evolution of coronal X-ray emission levels and
rotation rates of young, low-mass stars, similar to our own Sun.
How these stars evolve both on the main sequence and in the pre-main sequence
phase of evolution tells us about the evolution of magnetic dynamos in
these kinds of stars and something about the past history of our own
star, the Sun.
Publications
The easiest way to look at my publications is to make use of the
NASA ADS Astronomy
and Astrophysics Abstract Service.
Learn more about ...
The National Science Foundation
Harvard University
The Smithsonian Institution
The SWAS Mission
The Spitzer Space Telescope
The Infrared Array Camera on Spitzer
|