TY - JOUR

T1 - Dusty Galaxies at the Highest Redshifts

AU - Clements, David L.

AU - Greenslade, Josh

AU - Riechers, Dominik A.

AU - Wardlow, Julie

AU - Pérez-Fournon, Ismael

PY - 2015/8/1

Y1 - 2015/8/1

N2 - The use of red colour as the basis for selecting candidate high redshift dusty galaxies from surveys made with Herschel has proved highly successful. The highest redshift such object, HFLS3, lies at z = 6.34 and numerous other sources have been found. Spectroscopic followup confirms that most of these lie at z > 4. These sources are found in such numbers that they represent a challenge to current models of galaxy evolution. We also examine the prospects for finding dusty galaxies at still higher redshifts. These would not appear in the SPIRE surveys from Herschel but would be detected in longer wavelength, submm, surveys. Several such 'SPIRE-dropouts' have been found and are now subject to followup observations.

AB - The use of red colour as the basis for selecting candidate high redshift dusty galaxies from surveys made with Herschel has proved highly successful. The highest redshift such object, HFLS3, lies at z = 6.34 and numerous other sources have been found. Spectroscopic followup confirms that most of these lie at z > 4. These sources are found in such numbers that they represent a challenge to current models of galaxy evolution. We also examine the prospects for finding dusty galaxies at still higher redshifts. These would not appear in the SPIRE surveys from Herschel but would be detected in longer wavelength, submm, surveys. Several such 'SPIRE-dropouts' have been found and are now subject to followup observations.

KW - galaxies: starburst

KW - galaxies: submm

KW - galaxies:high redshift

U2 - 10.1017/S1743921315010078

DO - 10.1017/S1743921315010078

M3 - Journal article

AN - SCOPUS:84983372219

VL - 11

SP - 84

EP - 87

JO - Proceedings of the International Astronomical Union

JF - Proceedings of the International Astronomical Union

SN - 1743-9213

ER -