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DPhot photometry method for the Spitzer Space Telescope
SPIE Proceedings, 2006DPhot is a "deep photometry" computer program for measuring faint point sources from an overlapping set of astronomical images without making a mosaic. A grid of points is written on the sky. The point response function is used to calculate influence coefficients between the grid points and the pixels.
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Planet Formation Studies with the Spitzer Space Telescope
Space 2005, 2005This paper will review the progress in planet formation science which Spitzer has enabled, and look forward to future contributions we can expect over the 5-year mission lifetime.
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The Spitzer Space Telescope: the first 30 months
SPIE Proceedings, 2006We provide an overview of the design of the Spitzer Space Telescope and review scientific highlights from the first 30 months of on-orbit operations.
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Observations of luminous infrared galaxies with the Spitzer Space Telescope
Nature Astronomy, 2020L. Armus +3 more
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On-Orbit Experience with the Spitzer Space Telescope Optical System
Frontiers in Optics, 2005The Spitzer Space Telescope operates at wavelengths between 3.6 and 160 microns. This paper describes the on-orbit performance of the beryllium optical system which was launched warm and radiatively cooled to cryogenic temperatures.
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Observing Exoplanets with the Spitzer Space Telescope
2017Drake Deming, Charles Beichman
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Asteroid (16) Psyche: Evidence for a silicate regolith from spitzer space telescope spectroscopy
, 2017Z. Landsman +5 more
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Spitzer Space Telescope: An Operational Learning Experience [PDF]
SpaceOps 2008 Conference, 2008 openaire +1 more source
The Spitzer Space Telescope: The Infrared Universe Revealed
2006 IEEE Aerospace Conference, 2006openaire +2 more sources