Abstract
Local luminosity functions are fundamental benchmarks for high-redshift galaxy formation and evolution studies as well as for models describing these processes. Determining the local luminosity function in the submillimeter range can help to better constrain in particular the bolometric luminosity density in the local Universe, and Herschel offers the first opportunity to do so in an unbiased way by imaging large sky areas at several submillimeter wavelengths. We present the first Herschel measurement of the submillimeter 0 \ensuremath
| Original language | English (Ireland) |
|---|---|
| Journal | Astronomy and Astrophysics |
| Volume | 518 |
| Publication status | Published - 1 Jan 2010 |
Authors (Note for portal: view the doc link for the full list of authors)
- Authors
- M. Vaccari and L. Marchetti and A. Franceschini and B. Altieri and A. Amblard and V. Arumugam and Robbie Richard Auld and H. Aussel and T. Babbedge and A. Blain and J. Bock and A. Boselli and V. Buat and D. Burgarella and N. Castro-Rodr\'iguez and A. Cava and P. Chanial and D. L. Clements and A. Conley and L. Conversi and A. Cooray and C. D. Dowell and E. Dwek and S. Dye and Stephen Anthony Eales and D. Elbaz and D. Farrah and M. Fox and Walter Kieran Gear and J. Glenn and E. A. Gonz\'alez Solares and Matthew Joseph Griffin and M. Halpern and E. Hatziminaoglou and J. Huang and E. Ibar and Kate Gudrun Isaak and R. J. Ivison and G. Lagache and L. Levenson and N. Lu and S. Madden and B. Maffei and G. Mainetti and A. M. J. Mortier and H. T. Nguyen and B. O'Halloran and S. J. Oliver and A. Omon