Rest-UV absorption lines as metallicity estimator: the metal content of 
star-forming galaxies at z similar to 5

Faisst, A. L.; Capak, P. L.; Davidzon, I.; Salvato, M.; Laigle, C.; Ilbert, O.; Onodera, M.; Hasinger, G.; Kakazu, Y.; Masters, D.; McCracken, H. J.; Mobasher, B.; Sanders, D.; Silverman, J. D.; Yan, L.; Scoville, N. Z.

doi:10.3847/0004-637X/822/1/29

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Rest-UV absorption lines as metallicity estimator: the metal content of star-forming galaxies at z similar to 5

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Salvato, M.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Faisst, A. L., Capak, P. L., Davidzon, I., Salvato, M., Laigle, C., Ilbert, O., Onodera, M., Hasinger, G., Kakazu, Y., Masters, D., McCracken, H. J., Mobasher, B., Sanders, D., Silverman, J. D., Yan, L., & Scoville, N. Z. (2016). Rest-UV absorption lines as metallicity estimator: the metal content of star-forming galaxies at z similar to 5. The Astrophysical Journal, 822(1):, pp. 1-18. doi:10.3847/0004-637X/822/1/29.

引用: https://hdl.handle.net/11858/00-001M-0000-002A-F334-E

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