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NOEMA redshift measurements of bright Herschel galaxies
R. Neri, P. Cox, A. Omont +31
Using the IRAM NOrthern Extended Millimeter Array (NOEMA), we conducted a program to measure redshifts for 13 bright galaxies detected in the Herschel Astrophysical Large Area Surv…
HELP: A catalogue of 170 million objects, selected at 0.36-4.5 m, from 1270 deg. of prime extragalactic fields
Raphael Shirley, Yannick Roehlly, Peter D Hurley +15
We present an optical to near-infrared selected astronomical catalogue covering 1270 deg.. This is the first attempt to systematically combine data from 23 of the premier extra…
Properties of LBGs with [OIII] detection at z 3.5: The importance of including nebular emission data in SED fitting
Fang-Ting Yuan, Denis Burgarella, David Corre +3
Nebular emission lines are critical to measure physical properties in the ionized gas (e.g., metallicity, the SFR, or dust attenuation). They also account for a significant fractio…
Rest-frame FUV-to-FIR view of Lyman break galaxies at : Templates and dust attenuation
J. Álvarez-Márquez, D. Burgarella, V. Buat +2
This work explores from a statistical point of view the rest-frame Far-ultraviolet (FUV) to Far-infrared (FIR) emission of a population of Lyman break galaxies (LBGs) at t…
HELP project - a dreamed-of multiwavelength dataset for SED fitting: the influence of used models for the main physical properties of galaxies
Katarzyna Malek, Veronique Buat, Denis Burgarella +3
The Herschel Extragalactic Legacy Project (HELP) focuses to publish an astronomical multiwavelength catalogue of millions of objects over 1300~deg of the Herschel Space Observa…
Which attenuation curves for star-forming galaxies?
Buat, V., Corre +5
Dust attenuation shapes the spectral energy distributions of galaxies and any modelling and fitting procedure of their spectral energy distributions must account for this process.…