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Correction might be necessary for the interstellar absorption of starlight.
Moreover, interstellar absorption makes EUV observations challenging.
Distances can be determined by many methods geometric, photometric, and spectroscopic with corrections for interstellar absorption.
The "unabsorbed flux" or "flux" is a calculation of the flux without interstellar absorption.
The nebula is substantially reddened by interstellar absorption (the V-band absorption is about 1.5 magnitudes).
The fluxes FX given in Table 2 are not corrected for the interstellar absorption and refer to the 0.2 10.0 keV energy range.
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Fortunately, nearly all observations of nearby stars contain useful local interstellar medium absorption lines.
He developed what became known as the Whitford reddening curve, which gauged interstellar light absorption and was a vital tool in mapping the distribution of stars in the Milky Way.
IN a recent article1 describing results obtained with the coudé spectrograph of the Mount Wilson Observatory, W. S. Adams gives some details of the identification of a number of interstellar lines with absorption ; lines of various molecules in their lowest possible energy states.
We obtain ΔCext 9.7μm) by integrating the 9.7μm model extinction profile (with the continuum subtracted) over wavelength (see Fig. 2 for illustration) and then dividing the integrated value with the width of the interstellar 9.7μm silicate absorption feature.
By combining high-resolution hydrodynamical simulations of the hierarchical formation of a redshift z~6 quasar, stellar population synthesis models, prescriptions for interstellar and intergalactic absorption, and the photometric response of modern telescopes, we calculate the observable properties of quasar progenitors at high-redshifts.
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