A precise accounting for interstellar dust is required to interpret the energy output of galaxies. However comma our current understanding for how fundamental properties of dust grains vary between i
The proposed observation of seven obscured AGN are necessary to obtain acomplete and uniform coverage of the Xray emission for the sample of Seyfert2galaxies from the 12micron galaxy sample (12MGS). C
We propose a deep EPIC observation of the highly asymmetric young (< 600 yearsold) corecollapse (CC) supernova remnant G350.10.3, whose spectrum isdominated by ironrich ejecta expanding at up to 6,
GCOM-C/SGLI L3 Map Atmospheric corrected reflectance (SLZV) (1-Month,1/24 deg) is obtained from the SGLI sensor onboard GCOM-C and produced by the Japan Aerospace Exploration Agency (JAXA). GCOM-C is
Data Set Overview The Mars Express (MEX) Radio Science (MaRS) Data Archive is a timeordered collection of raw and partially processed data collected during the MEX Mission to Mars. For more informatio
