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1887
49137
On the importance of using appropriate spectral models to derive physical properties of galaxies at 0.7< z < 2.8
Author(s):
Pacifici, C.; Cunha, E. da; Charlot, S.; Rix, H.W.; Fumagalli, M.; Wel, A.; Franx, M. (
0000-0002-8871-3026
); Maseda, M.V.; Dokkum, P.G. van; Brammer, G.B.; Momcheva, I.; Skelton, R.E.; Whitaker, K.; Leja, J.; Lundgren, B.; Kassin, S.A.; Yi, S.K.
Published
2015
Publication type
Article / Letter to editor
Date issued
2015
Language
English
Is part of
Monthly Notices of the Royal Astronomical Society (2015), Vol. 447, no. 1, p. 786-805
hdl
1887/49137
doi
10.1093/mnras/stu2447
URL
http://adsabs.harvard.edu/abs/2015MNRAS.447..786P
Persistent identifier url
https://hdl.handle.net/1887/49137
Documents
01 - Monthly_Notices_of_the_Royal_Astronomical_Society_447oe2015oe786
version: Not Applicable (or Unknown)
Full text at Publisher's site
Open Access