-
Wide Field Planetary Camera 1
The WF/PC-1 was used from April 1990 to November 1993, to obtain high resolution images of astronomical objects over a relatively wide field of view and a broad... -
Wide Field Planetary Camera 2
The WFPC2 is used to obtain high resolution images of astronomical objects over a relatively wide field of view and a broad range of wavelengths (1150 to 11,000 Å). -
Kepler Input Catalog
The KIC, or Kepler Input Catalog, is the primary source of information about objects observed as part of the ground-based Kepler Spectral Classification Program (SCP) in... -
Kepler Objects of Interest (KOI)
Launched in 2009, the Kepler Mission is surveying a region of our galaxy to determine what fraction of stars in our galaxy have planets and measure the size distribution of... -
Kepler K2 Ecliptic Plane Input Catalog
Launched in 2009, the Kepler Mission is surveying a region of our galaxy to determine what fraction of stars in our galaxy have planets and measure the size distribution of... -
VHS DR4 - VISTA Hemisphere Survey Data Release 4
The VHS will image the entire ~20 000 square degrees of the Southern Sky, with the exception of the areas already covered by the VIKING and VVV surveys, in J and Ks. The... -
VHS DR3 - VISTA Hemisphere Survey Data Release 3
The VHS will image the entire ~20 000 square degrees of the Southern Sky, with the exception of the areas already covered by the VIKING and VVV surveys, in J and Ks. The... -
VHS DR2 - VISTA Hemisphere Survey Data Release 2
The VHS will image the entire ~20 000 square degrees of the Southern Sky, with the exception of the areas already covered by the VIKING and VVV surveys, in J and Ks. The... -
VHS DR1 - VISTA Hemisphere Survey Data Release 1
The VHS will image the entire ~20 000 square degrees of the Southern Sky, with the exception of the areas already covered by the VIKING and VVV surveys, in J and Ks. The... -
Supporting Materials
This collection contains supporting materials for the article titled "Direct observations of a complex coronal web driving highly structured slow solar wind". The folder... -
Berkeley Extreme and Far-UV Spectrometer
The Berkeley Extreme and Far-UV Spectrometer (BEFS), flew on the Orbiting and Retrievable Far and Extreme Ultraviolet Spectrograph (ORFEUS)-SPAS I and II space... -
Space Telescope Imaging Spectrograph
The Space Telescope Imaging Spectrograph (STIS) was installed in HST on Feb. 14, 1997, replacing the GHRS spectrograph. STIS provides spectra and images at... -
Goddard High Resolution Spectrograph
GHRS was used to make finely detailed spectroscopic observations of ultraviolet sources, but was removed from HST in February 1997. -
Near Infrared Camera and Multi Object Spectrograph
The HST Near Infrared Camera and Multi-Object Spectrometer (NICMOS) provides imaging capabilities in broad, medium, and narrow band filters, broad-band imaging... -
Faint Object Camera
The Faint Object Camera (FOC) was one of the 4 original axial instruments on the Hubble Space Telescope (HST). FOC is used to make high-resolution observations... -
Faint Object Spectrograph
The Faint Object Spectrograph (FOS) was one of the 4 original axial instruments aboard the Hubble Space Telescope (HST). The FOS was designed to make... -
Advanced Camera for Surveys
HST Advanced Camera for Surveys (ACS) - Images: CCD images between 3,700 - 11 -
Hubble Space Telescope
Hubble Space Telescope (HST) is an orbiting astronomical observatory operating from the near-infrared into the ultraviolet. Launched in 1990 and scheduled to... -
HST Space Telescope Imaging Spectrograph
MAST-produced spectral container files for STIS spectra. STIS spectra range from 1150 to 10,300 at low to medium spectral resolution, high spatial resolution... -
Kepler Confirmed Planets
The list of currently confirmed exoplanets discovered by Kepler (from data compiled by http://nexsci.caltech.edu).
