HEASARC Staff Scientist Position - Applications are now being accepted for a Staff Scientist with significant experience and interest in the technical aspects of astrophysics research, to work in the High Energy Astrophysics Science Archive Research Center (HEASARC) at NASA Goddard Space Flight Center (GSFC) in Greenbelt, MD. Refer to the AAS Job register for full details.

Search:

[Advanced Search]



ACTIVE MISSIONS
   AstroSat    BurstCube
   CALET    Chandra
   Fermi    HXMT-Insight
   INTEGRAL    IXPE
   MAXI    NICER
   NuSTAR    SRG  eROSITA
   /ART-XC
   Swift    XMM-Newton
   XRISM    
PAST MISSIONS
   AGILE    ANS
   ARIEL V    ASCA
   BBXRT    BeppoSAX
   CGRO    COPERNICUS
   COS-B    DXS
   EINSTEIN    EUVE
   EXOSAT    GINGA
   GRANAT    HaloSat
   HAKUCHO    HEAO-1
   HEAO-3    HETE-2
   Hitomi    OSO-7
   OSO-8    ROSAT
   Rossi XTE    SAS-2
   SAS-3    Suzaku
   TENMA    UHURU
   VELA 5B     WASS
   XQC    

The EUVE Observatory

artist concept of EUVE satellite The Extreme Ultraviolet Explorer (EUVE), a NASA explorer class satellite mission, was launched on June 7 1992 and it operated till January 31 2001. EUVE is entirely dedicated to observations in the wavelength range from 70 to 760 Å. The first phase of the mission (six months) was dedicated to an all-sky survey using the imaging instruments. The second phase instead is dedicated to pointed observations with mainly the spectroscopic instruments.

Mission Characteristics

* Lifetime : June 7, 1992 - January 31, 2001
* Energy Range : 70-760 Å
* Special Features : First dedicated extreme ultraviolet mission
* Payload :
  • 2 Wolter-Schwarzschild Type I grazing incidence mirror,
    each with an imaging microchannel plate (MCP detector)
    (Scanner A & B) FOV ~5° diameter; two passbands 44-220 Å 140-360 Å
  • 1 Wolter-Schwarzschild Type II grazing incidence mirror,
    with an imaging microchannel plate (MCP detector)
    FOV ~4° diameter; two passbands 520-750 Å 400-600 Å
  • 1 Wolter-Schwarzschild Type II grazing incidence mirror Deep Survey/Spectrometer Telescope. The light is split, with half of the light fed to:
    • An imaging Deep Survey MCP detector
    • Three Spectrometers which are each combinations of a grating and MCP detector:
      SW (70-190 Å) MW (140-380 Å) LW (280-760 Å).
* Science Highlights:
  • All-sky survey catalog (801 objects)
  • EUV first detection of extragalactic objects (e.g. PKS 2155-304)
  • Detection of the photospheric emission from stars (e.g. epsilon CMa)
  • Quasi Periodic Oscillation detection in the Dwarf Nova SS Cygni
* Archive : HEASARC hosts catalogs, images, raw data and selected spectra
[EUVE Home]
[All Missions] [by Time] [by Energy]
Page authors: Lorella Angelini Jesse Allen
HEASARC Home | Observatories | Archive | Calibration | Software | Tools | Students/Teachers/Public
Last modified: Thursday, 24-Sep-2020 19:08:54 EDT

HEASARC Staff Scientist Position - Applications are now being accepted for a Staff Scientist with significant experience and interest in the technical aspects of astrophysics research, to work in the High Energy Astrophysics Science Archive Research Center (HEASARC) at NASA Goddard Space Flight Center (GSFC) in Greenbelt, MD. Refer to the AAS Job register for full details.