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STScI        |            FF      OO  OO   SS             | STAN - FOS
Analysis     |            FFFF    OO  OO    SS            | Number 10
News         |            FF      OO  OO     SS           | April 1996
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CONTENTS:

        - FOS NEWS 
          + New Instrument Science Report: "The FOS Dark Count-rate: Cycles
            1-4"

        - Scientific Programmer Positions Available at STScI

        - RECENT PREPRINTS

        - APPENDIX: FOS CONTACTS

================================================================================

New Instrument Science Report: "The FOS Dark Count-rate: Cycles 1-4"
----------------------------------------------------------------------

A new FOS Instrument Science Report has been issued.  It is CAL/FOS 146,
"The FOS Dark Count-rate: Cycles 1 to 4" by Jeffrey J.E. Hayes and Don J. 
Lindler, April 1996

This document gives an analysis of all FOS dark observations
taken on-orbit from Cycle 1 through Cycle 4.  We find that overall,
the FOS/RED dark count-rate is 0.0109 +/- 0.0022 counts/sec/diode, while
for the FOS/BLUE, the count-rate is 0.0064 +/- 0.00083 counts/sec/diode.  
We confirm the finding of Rosenblatt et.al. (1992) of the correlation between
dark count-rate and geo-magnetic latitude, but see no evidence for any
correlation between geo-magnetic longitude, solar position angle, or solar
cycle.

Copies of this report may be requested from the Help Desk, help@stsci.edu.

================================================================================

Scientific Programmer Positions Available at STScI
---------------------------------------------------

The Space Telescope Science Institute has two openings for the position
of Scientific Programmer in the Science Software Branch.  The
programmers are responsible for design, coding, testing, and
maintenance of the software used by the international astronomical
community for the calibration and analysis of data from the Hubble
Space Telescope.  Programmers within the group work closely with
astronomers on the ST ScI staff in developing software requirements and
algorithms for instrument-specific tasks (including data analysis
pipelines for new HST instruments).  They also participate in larger
development projects, often in collaboration with programming staff at
other astronomical institutions, to enhance the system-level
environment.

Proficiency in C and Fortran and a working knowledge of the Unix and
VMS operating systems are required.  Experience with object-oriented
languages such as C++ is desirable, as is experience with the IRAF data
analysis system.  A background in research data analysis and algorithm
development for image or spectral data is required; an astronomical
background is highly desirable.  Excellent verbal and written
communications skills are necessary.

A Bachelor's Degree in Astronomy, Physics, Computer Science, or related
field is required; an advanced degree is preferred.  The successful
candidate will have a minimum of two years experience in scientific
software development.  Substitution of additional relevant education or
experience for stated qualifications may be considered.  Females and
minorities are encouraged to apply.  These positions will remain open
until suitable candidates have been found.  Send a curriculum vitae,
letter of application, and samples of C or Fortran code to:

	Human Resources Manager
	Space Telescope Science Institute
	3700 San Martin Drive
	Baltimore, MD 21218

================================================================================

                         RECENT PREPRINTS
                         ----------------

We draw your attention to these papers, based on FOS data, that will appear in
the next few months. This list includes all preprints received by the STScI
Library not yet published in the journals.  Please remember to include our 
Library in your preprint distribution list.

AYRES, T.R.  "Stellar spectroscopy with the HST"  Cool
Stars, Stellar Systems and the Sun 9 - in Linsky preprint

KHERSONSKY, V.K.; TURNSHEK, D.A.; BRIGGS, F.H.  "Some
recent results on QSO absorption line studies with HST"
Sci. with the HST 2

TURNSHEK, D.A.  "Recent results from HST observations of
BAL QSOs"  Sci. with the HST 2 - in Khersonsky preprint

================================================================================

                      APPENDIX: FOS contacts
                      -----------------------

Any questions about the scheduling of your observations should be addressed to
your Program coordinator. Post-Observation questions can be addressed to your
Contact Scientist. If you do not know who these persons are, you can find the
information in http://www.stsci.edu/public/propinfo.html.

Analysis, STSDAS or any other questions can also be addressed to help@stsci.edu
================================================================================
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================================================================================
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================================================================================



