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EPOXI MARS OBS - HRII RAW SPECTRA V1.0
This data set contains raw, 1.05- to 4.8-micron spectra of Mars acquired by the High Resolution Infrared Spectrometer (HRII) for the EPOCh project during the second cruise phase of the EPOXI mission. One set of observations was acquired on 20-21 November 2009 to characterize Mars as an analog for extrasolar planets. The observing period lasted approximately 24 hours, and spectra were acquired twice per hour.
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EPOXI MARS OBS - HRII RAW SPECTRA V1.0
공공데이터포털
This data set contains raw, 1.05- to 4.8-micron spectra of Mars acquired by the High Resolution Infrared Spectrometer (HRII) for the EPOCh project during the second cruise phase of the EPOXI mission. One set of observations was acquired on 20-21 November 2009 to characterize Mars as an analog for extrasolar planets. The observing period lasted approximately 24 hours, and spectra were acquired twice per hour.
EPOXI MARS OBS - HRII CALIBRATED SPECTRA V1.0
공공데이터포털
This dataset contains calibrated, 1.05- to 4.8-micron spectra of Mars acquired by the High Resolution Infrared Spectrometer (HRII) for the EPOCh project during the second cruise phase of the EPOXI mission. One set of observations was acquired on 20-21 November 2009 to characterize Mars as an analog for extrasolar planets. The observing period lasted approximately 24 hours, and spectra were acquired twice every two hours.
EPOXI MARS OBS - HRII CALIBRATED SPECTRA V1.0
공공데이터포털
This dataset contains calibrated, 1.05- to 4.8-micron spectra of Mars acquired by the High Resolution Infrared Spectrometer (HRII) for the EPOCh project during the second cruise phase of the EPOXI mission. One set of observations was acquired on 20-21 November 2009 to characterize Mars as an analog for extrasolar planets. The observing period lasted approximately 24 hours, and spectra were acquired twice every two hours.
EPOXI MARS OBS - HRIV RAW IMAGES V1.0
공공데이터포털
This data set contains raw narrow band filter images (350-950 nm) images of Mars acquired by the Deep Impact High Resolution Visible CCD (HRIV) for the EPOCh project during the second cruise phase of the EPOXI mission. One set of observations was acquired on 20-21 November 2009 to characterize Mars as an analog for extrasolar planets. The observing period lasted approximately 24 hours. HRIV images were acquired once per hour with the filters centered on 350, 750 and 950 nm, whereas the 450-, 550-, 650-, and 850-nm data were taken every 15 minutes.
EPOXI MARS OBS - HRIV RAW IMAGES V1.0
공공데이터포털
This data set contains raw narrow band filter images (350-950 nm) images of Mars acquired by the Deep Impact High Resolution Visible CCD (HRIV) for the EPOCh project during the second cruise phase of the EPOXI mission. One set of observations was acquired on 20-21 November 2009 to characterize Mars as an analog for extrasolar planets. The observing period lasted approximately 24 hours. HRIV images were acquired once per hour with the filters centered on 350, 750 and 950 nm, whereas the 450-, 550-, 650-, and 850-nm data were taken every 15 minutes.
EPOXI MARS OBS - HRIV CALIBRATED IMAGES V1.0
공공데이터포털
This data set contains calibrated narrow band filter images (350-950 nm) images of Mars acquired by the Deep Impact High Resolution Visible CCD (HRIV) for the EPOCh project during the second cruise phase of the EPOXI mission. One set of observations was acquired on 20-21 November 2009 to characterize Mars as an analog for extrasolar planets. The observing period lasted approximately 24 hours. HRIV images were acquired once per hour with the filters centered on 350, 750 and 950 nm, whereas the 450-, 550-, 650-, and 850-nm data were taken every 15 minutes.
EPOXI MARS OBS - HRIV CALIBRATED IMAGES V1.0
공공데이터포털
This data set contains calibrated narrow band filter images (350-950 nm) images of Mars acquired by the Deep Impact High Resolution Visible CCD (HRIV) for the EPOCh project during the second cruise phase of the EPOXI mission. One set of observations was acquired on 20-21 November 2009 to characterize Mars as an analog for extrasolar planets. The observing period lasted approximately 24 hours. HRIV images were acquired once per hour with the filters centered on 350, 750 and 950 nm, whereas the 450-, 550-, 650-, and 850-nm data were taken every 15 minutes.
EPOXI MARS OBS - HRIV CALIBRATED IMAGES V2.0
공공데이터포털
This data set contains calibrated narrow band filter images (350-950 nm) images of Mars acquired by the Deep Impact High Resolution Visible CCD (HRIV) for the EPOCh project during the second cruise phase of the EPOXI mission. One set of observations was acquired on 20-21 November 2009 to characterize Mars as an analog for extrasolar planets. The observing period lasted approximately 24 hours. HRIV images were acquired once per hour with the filters centered on 350, 750 and 950 nm, whereas the 450-, 550-, 650-, and 850-nm data were taken every 15 minutes. Version 2.0 includes the application of a horizontal destriping process and revised electronic crosstalk calibration files.
EPOXI MARS OBS - HRIV CALIBRATED IMAGES V2.0
공공데이터포털
This data set contains calibrated narrow band filter images (350-950 nm) images of Mars acquired by the Deep Impact High Resolution Visible CCD (HRIV) for the EPOCh project during the second cruise phase of the EPOXI mission. One set of observations was acquired on 20-21 November 2009 to characterize Mars as an analog for extrasolar planets. The observing period lasted approximately 24 hours. HRIV images were acquired once per hour with the filters centered on 350, 750 and 950 nm, whereas the 450-, 550-, 650-, and 850-nm data were taken every 15 minutes. Version 2.0 includes the application of a horizontal destriping process and revised electronic crosstalk calibration files.
EPOXI MARS OBS - MRI RAW IMAGES V1.0
공공데이터포털
This data set contains raw 750-nm filter images of Mars acquired by the Deep Impact Medium Resolution Visible CCD (MRI) for the EPOCh project during the second cruise phase of the EPOXI mission. One set of observations was acquired on 20-21 November 2009 to characterize Mars as an analog for extrasolar planets. The observing period lasted approximately 24 hours, and one MRI image was taken simultaneously with the first north/south scan of the HRI IR spectrometer at half-hour intervals to provide context for the spectral scans.