The COS Legacy Archive Spectroscopy Survey (CLASSY) Treasury Atlas* ^∗ Based on observations made with the NASA/ESA Hubble Space Telescope, obtained from the Data Archive at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555.

Article

Abstract: Far-ultraviolet (FUV; ∼1200-2000 Å) spectra are fundamental to our understanding of star-forming gal

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Autores:

Aloisi A., Amorín R.O., Arellano-Córdova K.Z., Bayliss M., Berg D.A., Bordoloi R., Brinchmann J., Charlot S., Chen Z., Chevallard J., Chisholm J., Clark I., Erb D.K., Feltre A., Gronke M., Hayes M., Heckman T., Henry A., Hernandez S., James B.L., Jaskot A., Jones T., Kewley L.J., King T., Kumari N., Leitherer C., Mario Llerena, Martin C.L., Maseda M., McDonald M., Mingozzi M., Nanayakkara T., Ouchi M., Plat A., Pogge R.W., Ravindranath S., Rigby J.R., Sanders R., Scarlata C., Senchyna P., Skillman E.D., Stark D.P., Steidel C.C., Strom A.L., Sugahara Y., Wilkins S.M., Wofford A., Xu X.

Fuentes:

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