D. F. Neidig < D. Fadda < D. Fappani

Facettes : Author.f AffOrg.f AffPays.f AffRegion.f AffVille.f Teeft.f

List of bibliographic references indexed by D. Fadda

Number of relevant bibliographic references: 6.

Ident.	Authors (with country if any)	Title
000215 (2007)	M. Magliocchetti [Italie] ; L. Silva [Italie] ; A. Lapi [Italie] ; G. De Zotti [Italie] ; G. L. Granato [Italie] ; D. Fadda [États-Unis] ; L. Danese [Italie]	A highly obscured and strongly clustered galaxy population discovered with the Spitzer Space Telescope
000234 (2007)	M. Magliocchetti [Italie] ; L. Silva [Italie] ; A. Lapi [Italie] ; G. De Zotti [Italie] ; G. L. Granato [Italie] ; D. Fadda [États-Unis] ; L. Danese [Italie]	A highly obscured and strongly clustered galaxy population discovered with the Spitzer Space Telescope
000284 (2005)	G. Rodighiero [Italie] ; D. Fadda [États-Unis] ; A. Franceschini [Italie] ; C. Lari [Italie]	A far-infrared view of the Lockman hole from ISO 95-µm observations – II. Optical identifications and insights into the nature of the far-infrared sources
000311 (2005)	G. Rodighiero [Italie] ; D. Fadda [États-Unis] ; A. Franceschini [Italie] ; C. Lari [Italie]	A far‐infrared view of the Lockman hole from ISO 95‐μm observations – II. Optical identifications and insights into the nature of the far‐infrared sources
000361 (2003)	G. Rodighiero [Italie] ; C. Lari [Italie] ; A. Franceschini [Italie] ; A. Gregnanin [Italie] ; D. Fadda [États-Unis, Espagne]	A far-infrared view of the Lockman Hole from ISO 95-μm observations – I. A new data reduction method
000390 (2003)	G. Rodighiero [Italie] ; C. Lari [Italie] ; A. Franceschini [Italie] ; A. Gregnanin [Italie] ; D. Fadda [États-Unis, Espagne]	A far‐infrared view of the Lockman Hole from ISO 95‐μm observations – I. A new data reduction method

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List of associated KwdEn.i

Nombre de documents	Descripteur
5	galaxies: evolution
5	infrared: galaxies
3	cosmology: observations
2	galaxies: fundamental parameters
2	methods: observational
1	cosmology: theory
1	galaxies: statistics
1	large‐scale structure of Universe

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