scispace - formally typeset
N

N. Castro-Rodríguez

Researcher at University of La Laguna

Publications -  46
Citations -  4329

N. Castro-Rodríguez is an academic researcher from University of La Laguna. The author has contributed to research in topics: Galaxy & Redshift. The author has an hindex of 24, co-authored 46 publications receiving 4090 citations. Previous affiliations of N. Castro-Rodríguez include Spanish National Research Council.

Papers
More filters
Journal ArticleDOI

The Herschel Multi-tiered Extragalactic Survey: HerMES

Seb Oliver, +120 more
TL;DR: The Herschel Multi-tiered Extragalactic Survey (HerMES) is a legacy program designed to map a set of nested fields totalling ∼380deg^2 as mentioned in this paper.
Journal ArticleDOI

The Herschel Multi-tiered Extragalactic Survey: HerMES

Seb Oliver, +118 more
TL;DR: The Herschel Multi-tiered Extragalactic Survey (HerMES) is a legacy program designed to map a set of nested fields totalling ~380 deg^2 as mentioned in this paper.
Journal ArticleDOI

The Herschel* PEP/HerMES luminosity function - I. Probing the evolution of PACS selected Galaxies to z ≃ 4

Carlotta Gruppioni, +118 more
TL;DR: In this article, the authors exploit the deep and extended far-IR data sets (at 70, 100 and 160 μm) of the GPS PACS Evolutionary Probe (PEP) Survey, in combination with the Herschel Multi-tiered Extragalactic Survey data at 250, 350 and 500 μm, to derive the evolution of the rest-frame 35-, 60-, 90- and total infrared luminosity functions (LFs) up to z ∼ 4.
Journal ArticleDOI

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

Seb Oliver, +90 more
TL;DR: In this paper, the authors used the SPIRE instrument on the Herschel Multi-tiered Extra-Galactic Survey (HerMES) to directly resolve ~15% of the infrared extra-galactic background at the wavelength near where it peaks.
Journal ArticleDOI

HerMES: deep number counts at 250 μm, 350 μm and 500 μm in the COSMOS and GOODS-N fields and the build-up of the cosmic infrared background

Matthieu Béthermin, +75 more
TL;DR: In this paper, the authors derived the number counts and redshift distributions of the bright SPIRE sources in the COSMOS field with a method using the positions, the flux densities, and the redshifts of the 24 μm sources as a prior.