Selecting sources with rising flux densities towards longer wavelengths from Herschel/Spectral and Photometric Imaging Receiver (SPIRE) maps is an efficient way to produce a catalogue rich in high-redshift (z > 4) dusty star-forming galaxies. The effectiveness of this approach has already been confirmed by spectroscopic follow-up observations, but the previously available catalogues made this way are limited by small survey areas. Here we apply a map-based search method to 274 deg^2 of the Herschel Multi-tiered Extragalactic Survey (HerMES) Large Mode Survey and create a catalogue of 477 objects with SPIRE flux densities S_(500) > S_(350) > S_(250) and a 5σ cut-off S_(500) > 52 mJy. From this catalogue we determine that the total number of ...
The Herschel Multi-tiered Extragalactic Survey (HerMES) has identified large numbers of dusty star-f...
Observations suggest that almost half of the total light emitted by stars in the Universe is absorbe...
The wide-area imaging surveys with the Herschel Space Observatory at submillimeter (sub-mm) waveleng...
Selecting sources with rising flux densities towards longer wavelengths from Herschel/Spectral and P...
Selecting sources with rising flux densities towards longer wavelengths from Herschel/Spectral and P...
Selecting sources with rising flux densities towards longer wavelengths from Herschel/Spectral and P...
Selecting sources with rising flux densities towards longer wavelengths from Herschel/Spectral and P...
We present a method for selecting z > 4 dusty, star-forming galaxies (DSFGs) using Herschel/Spectral...
We present a method for selecting z > 4 dusty, star-forming galaxies (DSFGs) using Herschel/Spect...
We present a method for selecting z > 4 dusty, star-forming galaxies (DSFGs) using Herschel/Spectral...
We present a method for selecting z > 4 dusty, star-forming galaxies (DSFGs) using Herschel/Spectral...
We present colours of sources detected with the Herschel/SPIRE instrument in deep extragalactic surv...
High-redshift, luminous, dusty star-forming galaxies (DSFGs) constrain the extremity of galaxy forma...
High-redshift, luminous, dusty star-forming galaxies (DSFGs) constrain the extremity of galaxy forma...
The Herschel Multi-tiered Extragalactic Survey (HerMES) has identified large numbers of dusty star-f...
Observations suggest that almost half of the total light emitted by stars in the Universe is absorbe...
The wide-area imaging surveys with the Herschel Space Observatory at submillimeter (sub-mm) waveleng...
Selecting sources with rising flux densities towards longer wavelengths from Herschel/Spectral and P...
Selecting sources with rising flux densities towards longer wavelengths from Herschel/Spectral and P...
Selecting sources with rising flux densities towards longer wavelengths from Herschel/Spectral and P...
Selecting sources with rising flux densities towards longer wavelengths from Herschel/Spectral and P...
We present a method for selecting z > 4 dusty, star-forming galaxies (DSFGs) using Herschel/Spectral...
We present a method for selecting z > 4 dusty, star-forming galaxies (DSFGs) using Herschel/Spect...
We present a method for selecting z > 4 dusty, star-forming galaxies (DSFGs) using Herschel/Spectral...
We present a method for selecting z > 4 dusty, star-forming galaxies (DSFGs) using Herschel/Spectral...
We present colours of sources detected with the Herschel/SPIRE instrument in deep extragalactic surv...
High-redshift, luminous, dusty star-forming galaxies (DSFGs) constrain the extremity of galaxy forma...
High-redshift, luminous, dusty star-forming galaxies (DSFGs) constrain the extremity of galaxy forma...
The Herschel Multi-tiered Extragalactic Survey (HerMES) has identified large numbers of dusty star-f...
Observations suggest that almost half of the total light emitted by stars in the Universe is absorbe...
The wide-area imaging surveys with the Herschel Space Observatory at submillimeter (sub-mm) waveleng...