In this work we evaluate the SFR from different star formation indicators in order to determine the best correction for dust extinction on a sample of star forming galaxies at tt [0,7-1,5]. The sample is composed by 87 sources detected at far-IR wavelenghts by the Herschel Space telescope (from the PEP survey), with a strong Hd emission in the near-IR 3D-UST stifless spectre.
Star formation properties of galaxies in a deep HST spectral imaging survey
Puglisi, Annagrazia
2014/2015
Abstract
In this work we evaluate the SFR from different star formation indicators in order to determine the best correction for dust extinction on a sample of star forming galaxies at tt [0,7-1,5]. The sample is composed by 87 sources detected at far-IR wavelenghts by the Herschel Space telescope (from the PEP survey), with a strong Hd emission in the near-IR 3D-UST stifless spectre.File in questo prodotto:
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Utilizza questo identificativo per citare o creare un link a questo documento:
https://hdl.handle.net/20.500.12608/18101