Found 9 datasets matching "multiple-comets".
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This data set is intended to include published broadband colors of centaurs and Transneptunian Objects (TNOs) published through March 2014. It includes some comets with Centaur...
Search relevance: 63.13 | Views last month: 1 -
The collections in this archive contain results that have been reported in the literature, or in some cases made available by private communication, for various comet properties. Individual...
Search relevance: 59.03 | Views last month: 0 -
This bundle collects data taken at McDonald Observatory.
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The Near-Earth Object Wide-field Infrared Survey Explorer Reactivation Mission (NEOWISE; Mainzer et al. 2014, ApJ, 792, 30) is a NASA Planetary Science Division space-based survey to detect, track...
Search relevance: 41.24 | Views last month: 1 -
The WISE 3-Band Cryo Single Exposure (L1b) Source Table contains positions and photometry in the 3.4, 4.6 and 12 μm bands for 3,703,319,374 sources extracted from observations made during the WISE...
Search relevance: 32.94 | Views last month: 1 -
The Near-Earth Object Wide-field Infrared Survey Explorer Reactivation Mission (NEOWISE; Mainzer et al. 2014, ApJ, 792, 30) is a NASA Planetary Science Division space-based survey to detect, track...
Search relevance: 31.79 | Views last month: 1 -
The NEOWISE Post-Cryo Data Release products were generated using data taken during the mission's Post-Cryo survey phase. This phase covers the time following the exhaustion of solid hydrogen in...
Search relevance: 30.87 | Views last month: 0 -
The Near-Earth Object Wide-field Infrared Survey Explorer Reactivation Mission (NEOWISE; Mainzer et al. 2014, ApJ, 792, 30) is a NASA Planetary Science Division space-based survey to detect, track...
Search relevance: 26.42 | Views last month: 0 -
NASA's Wide-field Infrared Survey Explorer (WISE; Wright et al. 2010) mapped the sky at 3.4, 4.6, 12, and 22 μm (W1, W2, W3, W4) in 2010 with an angular resolution of 6.1", 6.4", 6.5", & 12.0" in...
Search relevance: 23.77 | Views last month: 0