The Large Magellanic Cloud was observed by the far ultraviolet camera spectrograph from the lunar surface during the Apollo 16 mission 22 April 1972. Images were obtained with about 3 arc min resolution, in the 1,050 to 1,600 and 1,250 to 1,600 A wavelength ranges, of nearly the entire LMC. Spectra were also obtained in the 1,050 to 1,600 and 900 to 1,600 A ranges along a strip 1/4 deg wide (determined by the instrument's grid collimator) passing across the LMC. The images and spectra have been scanned with a PDS microdensitometer, and isodensity contour plots have been prepared using the Univac 1108 computer
The Apollo 16 gnomon was photometrically calibrated at the Manned Spacecraft Center, Texas during De...
The region of the moon near the border between Mare Serenitatis and Mare Tranquillitatis is one of t...
This catalog contains 1273 proven or probable Large Magellanic Cloud (LMC) members, as found on deep...
Over 700 far UV photos were obtained with the S201 electrographic camera on Skylab 4 (27 Nov. 1973 -...
The Apollo 17 command service module in lunar orbit will carry a far ultraviolet scanning spectromet...
A detailed description of the machine-readable revised catalog as it is currently being distributed ...
The launch of sounding rocket 26.056 DG on 29 October 1976 is described and quick-look results from ...
The Galaxy Evolution Exporer (GALEX) has performed unprecedented imaging surveys of the Magellanic C...
A catalog which is a working document that shows the locations from which samples were collected dur...
Galactic (C II) 157 micron, fine-structure emission was estimated. At a Galactic longitude of 8 deg,...
A catalog of all pictures taken from the lunar module or the lunar surface during the Apollo 16 luna...
Preflight photographs of selected Apollo 17 equipment taken for use in determining the effects on va...
A catalog is presented of the documentation of Apollo 15 samples using photographs and verbal descri...
Observations obtained from Nimbus 3 and 4 satellites of solar long term variability and irradiance i...
An experiment using Earth based remote sensing radar, infrared eclipse, and color difference data to...
The Apollo 16 gnomon was photometrically calibrated at the Manned Spacecraft Center, Texas during De...
The region of the moon near the border between Mare Serenitatis and Mare Tranquillitatis is one of t...
This catalog contains 1273 proven or probable Large Magellanic Cloud (LMC) members, as found on deep...
Over 700 far UV photos were obtained with the S201 electrographic camera on Skylab 4 (27 Nov. 1973 -...
The Apollo 17 command service module in lunar orbit will carry a far ultraviolet scanning spectromet...
A detailed description of the machine-readable revised catalog as it is currently being distributed ...
The launch of sounding rocket 26.056 DG on 29 October 1976 is described and quick-look results from ...
The Galaxy Evolution Exporer (GALEX) has performed unprecedented imaging surveys of the Magellanic C...
A catalog which is a working document that shows the locations from which samples were collected dur...
Galactic (C II) 157 micron, fine-structure emission was estimated. At a Galactic longitude of 8 deg,...
A catalog of all pictures taken from the lunar module or the lunar surface during the Apollo 16 luna...
Preflight photographs of selected Apollo 17 equipment taken for use in determining the effects on va...
A catalog is presented of the documentation of Apollo 15 samples using photographs and verbal descri...
Observations obtained from Nimbus 3 and 4 satellites of solar long term variability and irradiance i...
An experiment using Earth based remote sensing radar, infrared eclipse, and color difference data to...
The Apollo 16 gnomon was photometrically calibrated at the Manned Spacecraft Center, Texas during De...
The region of the moon near the border between Mare Serenitatis and Mare Tranquillitatis is one of t...
This catalog contains 1273 proven or probable Large Magellanic Cloud (LMC) members, as found on deep...