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data set:
KECK I LWS MID-IR IMAGES AND PHOTOMETRY OF 9P/TEMPEL 1
Mid-infrared images and photometry of comet 9P/Tempel 1 from August 21, 2000. Images were obtained by Y.Fernandez et al. with the LWS instrument at the Keck I telescope. This data set is a supplemental archive for Deep Impact.
DEEP IMPACTSUPPORT ARCHIVES - DI/EAR-C-KECK1LWS-3-9P-IMAGES-PHOT-V1.0 - starting 2000-08-21T10:51:19.92Z -
data set:
DELBO THERMAL INFRARED ASTEROID DIAMETERS AND ALBEDOS V1.0
Thermal infrared asteroid diameters and albedos by Delbo, observed 2000-2003.
SUPPORT ARCHIVES - EAR-A-KECK1LWS/ETAL-5-DELBO-V1.0 - starting 2000-03-16T00:00:00Z -
instrument:
KECK I LONG WAVELENGTH SPECTROGRAPH (IR) for KECK1
Information about the KECK I LONG WAVELENGTH SPECTROGRAPH (IR) for KECK1 instrument -
collection:
document collection for the "DELBO THERMAL INFRARED ASTEROID DIAMETERS AND ALBEDOS" bundle
This is the document collection for the ast.delbo.radiometric-diameters-albedos bundle. This data set contains radiometric albedos and diameters for Near Earth Asteroids (NEAs) derived by three different thermal models and reported in Delbo (2004) [DELBO2004]. The observed infrared fluxes on which the derivations were based are also included. -
instrument:
Keck I Long Wavelength Spectrograph (IR)
Information about the Keck I Long Wavelength Spectrograph (IR) instrument -
bundle:
DELBO THERMAL INFRARED ASTEROID DIAMETERS AND ALBEDOS
This data set contains radiometric albedos and diameters for Near Earth Asteroids (NEAs) derived by three different thermal models and reported in Delbo (2004) [DELBO2004]. The observed infrared fluxes on which the derivations were based are also included. -
collection:
data collection for the "DELBO THERMAL INFRARED ASTEROID DIAMETERS AND ALBEDOS" bundle
This is the data collection for the ast.delbo.radiometric-diameters-albedos bundle. This data set contains radiometric albedos and diameters for Near Earth Asteroids (NEAs) derived by three different thermal models and reported in Delbo (2004) [DELBO2004]. The observed infrared fluxes on which the derivations were based are also included.
Data Sets and Information