Hubble Space Telescope on-line telemetry archive for monitoring scientific instruments

2002 ◽  
Author(s):  
Manfred P. Miebach
1986 ◽  
Vol 7 ◽  
pp. 833-843 ◽  
Author(s):  
J. Koornneef ◽  
R. Bohlin ◽  
R. Buser ◽  
K. Horne ◽  
D. Turnshek

AbstractThe combined Scientific Instruments (SIs) on the Hubble Space Telescope (HST) feature an extensive wavelength coverage in both photometric and spectrophotometric modes with an overall dynamic range of more than twenty-five magnitudes. We demonstrate how synthetic photometry techniques are to be used to establish and maintain their calibration. This approach makes efficient use of limited HST observing time by taking full advantage of pre-launch knowledge on the SI sensitivity functions and calibration targets.


2002 ◽  
Author(s):  
David E. Lychenheim ◽  
Joyce Pepe ◽  
Debra Knapp

1998 ◽  
Vol 162 ◽  
pp. 74-78
Author(s):  
C.A. Christian

The data, scientific results, and expertise from NASA's Hubble Space Telescope (HST) and other NASA Missions are being integrated into programs that support innovative and experimental methods to improve content in science and math education. Partnerships with science museums, teachers, other educators, community colleges, universities and other key organizations integrate unique and cutting edge science data and the associated satellite technology into resources which have the potential to enhance science, math and technical learning. The inspiring nature of astronomical data and the technology associated with the HST and other missions can be used by teachers to engage students in many inventive activities. The resources created through collaborative teaming will be discussed, as well as the process for creating partnerships to benefit the education community. Many NASA supported programs encourage electronic access and distribution of multi-media interactive activities and curriculum support materials distributed across the Internet.


1994 ◽  
Vol 05 (05) ◽  
pp. 811-816
Author(s):  
CHRISTOPHER P. O’DEA

The Space Telescope Science Institute (STScI) makes available a wide variety of information concerning the Hubble Space Telescope (HST) via the Space Telescope Electronic Information Service (STEIS). STEIS is accessible via anonymous ftp, gopher, WAIS, and WWW. The information on STEIS includes how to propose for time on the HST, the current status of HST, reports on the scientific instruments, the observing schedule, data reduction software, calibration files, and a set of publicly available images in JPEG, GIF and TIFF format. STEIS serves both the astronomical community as well as the larger Internet community. WWW is currently the most widely used interface to STEIS. Future developments on STEIS are expected to include larger amounts of hypertext, especially HST images and educational material of interest to students, educators, and the general public, and the ability to query proposal status.


1985 ◽  
Vol 112 ◽  
pp. 75-84
Author(s):  
J. L. Russell

The Hubble Space Telescope (ST) will be launched with five dedicated scientific instruments and a capability to do astrometric measurements with the fine guidance sensors. Four of these – the Faint Object Camera, the Wide Field Camera, the Fine Guidance Sensors and the High Speed Photometer – can be used in the search for extrasolar planetary systems. The Faint Object Camera will be able to directly detect planets around a few of the nearby bright stars. The Wide Field Camera and the Fine Guidance Sensors can be used astrometrically, both with an accuracy of about 2 mas per observation. The High Speed Photometer possibly can detect planets during occultation of stars by the moon and minor planets. The ST is expected to be launched in mid-1986 and these observations are the among the first planned with the instruments.


1991 ◽  
Author(s):  
JEFFREY SPONSLER ◽  
MARK JOHNSTON ◽  
GLENN MILLER ◽  
ANTHONY KRUEGER ◽  
MICHAEL LUCKS ◽  
...  

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