WFAU, Institute for Astronomy, University of Edinburgh
Description:
The Galaxy Evolution Explorer (GALEX) satellite is a NASA mission led by the California Institute of Technology to investigate how star formation in galaxies evolved from the early Universe up to the present. GALEX uses microchannel plate detectors to obtain direct images in the near-UV (NUV) and far-UV (FUV) and a grism to disperse light for low resolution spectroscopy
WFAU, Institute for Astronomy, University of Edinburgh
Description:
The Galaxy Evolution Explorer (GALEX) satellite is a NASA mission led by the California Institute of Technology to investigate how star formation in galaxies evolved from the early Universe up to the present. GALEX uses microchannel plate detectors to obtain direct images in the near-UV (NUV) and far-UV (FUV) and a grism to disperse light for low resolution spectroscopy
Spectra from the HST FOS instrument (processed by ESO and CADC)
in the 1,150 - 8,500 Å range, resolution ~ 250 and 1,300, V_max ~ 20, 1990 - 1997.
Links point to VO-compatible FITS files created by MAST staff.
Hubble Space Telescope Goddard High Resolution Spectrograph
Short Name:
HST.GHRS Spectra
Date:
22 Jul 2020 21:54:42
Publisher:
Space Telescope Science Institute Archive
Description:
Spectra from the HST GHRS instrument (processed by ESO and CADC)
in the 1,100 - 3,300 Å range, resolution ~ 2,000, 25,000, and 80,000 (echelle),
V_max ~ 18, 16, and 12 respectively, 1990 - 1997. Links point to VO-compatible FITS
files created by MAST staff.
Quick-look preview images produced and processed by CADC. Data from the following HST instruments are included: WFPC, WFPC2, STIS, NICMOS, FOC, and ACS.
Spectra from the following HST instruments are available: GHRS (processed by CADC), FOS (processed by ECF), and STIS (1st order). Separate SSAP services are registered for each instrument.
VO-compatible FITS files were created by MAST staff.
Spectra from the Univsity of Wisconsin Pine Bluff Observatory
in the 3,200 - 7,750 Å range, resolution ~ 80, V_max ~ 15, ~ 2800 observations
of ~ 400 targets, 1989-1998. Note spectropolarimetry data is also included.
Observations complement those obtained from the ASTRO WUPPE project.
