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Your search keyword '"Pearson, C. P."' showing total 26 results

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26 results on '"Pearson, C. P."'

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1. The HerMES SPIRE submillimeter local luminosity function

2. HerMES: Far infrared properties of known AGN in the HerMES fields

3. The far-infrared/radio correlation as probed byHerschel

4. HerMES: SPIRE galaxy number counts at 250, 350, and 500 μm

5. Herschelunveils a puzzling uniformity of distant dusty galaxies

6. HerMES: The SPIRE confusion limit

7. HerMES: The submillimeter spectral energy distributions ofHerschel/SPIRE-detected galaxies

8. Herscheland SCUBA-2 imaging and spectroscopy of a bright, lensed submillimetre galaxy atz= 2.3

9. First results from HerMES on the evolution of the submillimetre luminosity function

10. HerMES: Halo occupation number and bias properties of dusty galaxies from angular clustering measurements

11. Source counts at 15 microns from the AKARI NEP survey

13. Polycyclic aromatic hydrocarbon (PAH) luminous galaxies atz ~ 1

14. Dissecting the cosmic infrared background with 3D instruments

15. A deep survey of the AKARI north ecliptic pole field

16. HerMES: The submillimeter spectral energy distributions of Herschel/SPIRE-detected galaxies*

17. In-flight calibration of the Herschel-SPIRE instrument*

18. Herschel-ATLAS: Dust temperature and redshift distribution of SPIRE and PACS detected sources using submillimetre colours*

19. Herschel-ATLAS: Extragalactic number counts from 250 to 500 microns*

20. The Herschel-SPIRE instrument and its in-flight performance*

21. HerschelATLAS: The cosmic star formation history of quasar host galaxies*

22. Herscheland SCUBA-2 imaging and spectroscopy of a bright, lensed submillimetre galaxy at z= 2.3*

23. The AGN fraction of submm-selected galaxies and contributions to the submm/mm-wave extragalactic background light

24. Environmental dependence of 8  μm luminosity functions of galaxies at z~ 0.8***

25. Polycyclic aromatic hydrocarbon (PAH) luminous galaxies at z~ 1

26. Evolution of infrared luminosity functions of galaxies in the AKARI NEP-deep field***

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