Astronomy Image Explorer

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Map of the (left) spectral slope computed from ...

Map of the (left) spectral slope computed from 2.1 and 2.5 μm in μm−1; (right) reflectan...

Antonin Wargnier et al, The Planetary Science Journal 7 9

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Map of the (top) phase ratio I(5°)/I(15°) at 2....

Map of the (top) phase ratio I(5°)/I(15°) at 2.0 μm and (bottom) phase reddening (with s...

Antonin Wargnier et al, The Planetary Science Journal 7 9

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(Left) Ryugu phase curve from NIRS3 data acquir...

(Left) Ryugu phase curve from NIRS3 data acquired during the proximity phase at 2 μm. (R...

Antonin Wargnier et al, The Planetary Science Journal 7 9

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(Top) ONC-T image acquired in the ul filter fro...

(Top) ONC-T image acquired in the ul filter from the home position (∼20 km) on 2018 July...

Antonin Wargnier et al, The Planetary Science Journal 7 9

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Map of the Moon from (a) SP data (Y. Yokota et ...

Map of the Moon from (a) SP data (Y. Yokota et al. 2011, 2012) and (b) M3 data, with pro...

Antonin Wargnier et al, The Planetary Science Journal 7 9

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Spectral evolution of the Hapke parameters for ...

Spectral evolution of the Hapke parameters for Ryugu, in the near-infrared (1.8–3.1 μm).

Antonin Wargnier et al, The Planetary Science Journal 7 9

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(Top) ONC-T image of the Moon acquired in the u...

(Top) ONC-T image of the Moon acquired in the ul filter on 2015 December 05T11:50:43.00 ...

Antonin Wargnier et al, The Planetary Science Journal 7 9

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Ryugu phase curves from NIRS3 data before TD1, ...

Ryugu phase curves from NIRS3 data before TD1, between TD1 and TD2, and after TD2, at 2 ...

Antonin Wargnier et al, The Planetary Science Journal 7 9

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Ratio of the irradiance from the ROLO model and...

Ratio of the irradiance from the ROLO model and the SP model. The dashed line represents...

Antonin Wargnier et al, The Planetary Science Journal 7 9

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Relative correction factor as a function of the...

Relative correction factor as a function of the wavelength between 1.8 μm and 3.2 μm. Th...

Antonin Wargnier et al, The Planetary Science Journal 7 9

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Comparison between ONC-T and NIRS3 reflectance ...

Comparison between ONC-T and NIRS3 reflectance levels for an image/spectrum acquired at ...

Antonin Wargnier et al, The Planetary Science Journal 7 9

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Comparison between ONC-T and NIRS3 reflectance ...

Comparison between ONC-T and NIRS3 reflectance spectra (after applying the updated calib...

Antonin Wargnier et al, The Planetary Science Journal 7 9

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Example of three comparisons of spectra from M3...

Example of three comparisons of spectra from M3 data (black solid line) and NIRS3. M3 is...

Antonin Wargnier et al, The Planetary Science Journal 7 9

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Example of three comparisons of spectra from SP...

Example of three comparisons of spectra from SP data (black solid line) and NIRS3. SP is...

Antonin Wargnier et al, The Planetary Science Journal 7 9

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Average ratio of raw and interpolated radiance ...

Average ratio of raw and interpolated radiance factor from M3 data [in %]. The average i...

Antonin Wargnier et al, The Planetary Science Journal 7 9

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Average of the scale factors used to match M3 m...

Average of the scale factors used to match M3 model spectra with the 45 NIRS3 spectra fo...

Antonin Wargnier et al, The Planetary Science Journal 7 9

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Ryugu phase curves from NIRS3 data before TD1 (...

Ryugu phase curves from NIRS3 data before TD1 (purple circles), between TD1 and TD2 (blu...

Antonin Wargnier et al, The Planetary Science Journal 7 9

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Distribution of the illumination angles (incide...

Distribution of the illumination angles (incidence, emission, and phase) for the entire ...

Antonin Wargnier et al, The Planetary Science Journal 7 9

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Maps of the number of observations per 10° × 10...

Maps of the number of observations per 10° × 10° grid element.

Antonin Wargnier et al, The Planetary Science Journal 7 9

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Maps of the (left) minimum and (right) maximum ...

Maps of the (left) minimum and (right) maximum phase angle per 10° × 10° grid element.

Antonin Wargnier et al, The Planetary Science Journal 7 9

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Rms normalized to Hapke rms values as a functio...

Rms normalized to Hapke rms values as a function of wavelength.

Antonin Wargnier et al, The Planetary Science Journal 7 9

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Rms normalized to Hapke rms values as a functio...

Rms normalized to Hapke rms values as a function of wavelength.

Antonin Wargnier et al, The Planetary Science Journal 7 9

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Spectral slope (2.1–2.5 μm) distribution as a f...

Spectral slope (2.1–2.5 μm) distribution as a function of the NIRS3 spatial resolution [...

Antonin Wargnier et al, The Planetary Science Journal 7 9

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Spectral slope (2.1–2.5 μm) distribution as a f...

Spectral slope (2.1–2.5 μm) distribution as a function of the solar phase angle [degrees...

Antonin Wargnier et al, The Planetary Science Journal 7 9

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Hapke parameter maps at 2.0 μm using a 10° × 10...

Hapke parameter maps at 2.0 μm using a 10° × 10° grid at the Ryugu surface.

Antonin Wargnier et al, The Planetary Science Journal 7 9

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ANNOUNCEMENTS

Updated Search and Sort

We have updated the search and sort algorithm to return records in reverse chronological order based on the date/time that the images were uploaded to the Astronomy Image Explorer. This is potentially but rarely different from the publication date. Thank you!