urn:nasa:pds:epoxi_mri:hartley2_photometry:epoxi_photometry_v5
1.0
EPOXI MRI-VIS 103P/Hartley 2 Encounter Photometry Description
1.9.0.0
Product_Document
Bodewits, D.; Farnham, T.; and A'Hearn, M.
2018
We perform photometric measurements of comet 103P/Hartley 2 using images taken through the CLEAR1 (broadband, 200-1100 nm), CN (387 nm), OH (309 nm), C2 (514 nm), and two continuum filters (Ultraviolet at 345 nm and Green at 526 nm) of the Medium Resolution Instrument (MRI) on board the Deep Impact flyby spacecraft from 1 October to 26 November 2010 during the EPOXI mission.
2017-07-25
1.0
Creation (Ben Hirsch)
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Bodewits, D.; Farnham, T.; and A'Hearn, M.
2018
1
We perform photometric measurements of comet 103P/Hartley 2 using images taken through the CLEAR1 (broadband, 200-1100 nm), CN (387 nm), OH (309 nm), C2 (514 nm), and two continuum filters (Ultraviolet at 345 nm and Green at 526 nm) of the Medium Resolution Instrument (MRI) on board the Deep Impact flyby spacecraft from 1 October to 26 November 2010 during the EPOXI mission. Our analysis includes over 30,000 MRI science images where the nucleus was not resolved. We apply two different methods for our analysis: simple aperture photometry using circular apertures and azimuthally-averaged photometry using concentric annuli to remove stars. The resulting photometry and computed errors from each method are provided as separate ASCII tables along with PDS labels describing the layouts and columns. A comparison with Version 1 of this dataset (Laughlin et al. 2012) is given in Sec. 6.
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English
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epoxi_photometry_v5.pdf
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