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| Address: | Space Telescope Science Institute
3700 San Martin Dr. Baltimore, MD 21218 |
Programming/Data Reduction Languages:
Fortran and IDL. Some knowledge of C (one formal course, plus ongoing
practice). VMS and Unix operating system, DCL
and IRAF scripts. Experienced user of IRAF and IDL reduction packages
for spectroscopy and imaging. Purchased Alpha 200
workstation, run under Dec/Unix.
Foreign Languages: Conversational French, written German.
Administration: See National
Science Foundation Program Director, Pre-CSC Employment
PhD in Astronomy, University of Arizona 1971
Director: Dr. Helmut Abt; Topic: Metallicism
in Am Stars.
BS (cum laude) in Astronomy 1966, Case Western Reserve University.
Walt Whitman High School, 1962; South Huntington, NY.
(click here for more detailed information)
1998-9: Elected Chair, Scientific Organizing Committee for IAU Colloq.
No. 175 on Be Stars in Alicante, Spain, June 1999.
1998: Asked to write popular article for ASP's Mercury magazine on
UV/X-ray research on the Be star gamma Cassiopeia (see June, 1998 issue).
1997: Press release requested by AAS for AAS Poster in January 1997
meeting.
1996: Elected member of American Astronomical Society Committee on
Employment (national).
1994: Elected Chair of International Astronomical Union Working Group
on Active Be Stars (> 350 members).
1993: Publicly cited for most interesting invited paper in IAU Symposium
No. 162, (International Astronomical Union conference on Rotation, Pulsation
in B stars)
1992: Outstanding Service Citation as Program Director, by NSF Director
Walter Massey.
1991: Invited contributor of 2 articles for Astronomy & Ap. Reference
Encyclopedia (Van Nostrand, 1992).
1991: First Place in CSC/SSD Division Honorarium competition for research
paper.
1990: Honorable Mention in CSC/SSD Division Honorarium Competition.
1996: Found X-ray/UV/optical link of initial outburst event in a Be
star.
1996: Resolved radiative transfer problem concerning equal emissions
of singlet & triplet lines of HeI lines in Be star spectra.
1993: Demonstration that magnetic flaring processes constitute the
most probable mechanism behind the outbursts of classical Be stars.
Late 1970's: Discovery of a new class of variables (nonradial pulsating
B stars).
Mid 1970's: Application of Fourier techniques for optimized signal
recovery of spectral line profiles. See appendix on reviews.
International Astronomical Union
American Astronomical Society (And Solar Phys, High Energy Divisions)
Astronomical Society of the Pacific
American Institute of Physics
Chair: IAU Working Group on Active B Stars
Member, Organizing Committee of IAU Variable Stars Commission #27,
1988-1997.
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