THE ALMA SPECTROSCOPIC SURVEY IN THE HUBBLE ULTRA DEEP FIELD : SEARCH FOR [ C II ] LINE AND DUST EMISSION IN 6 < z < 8 GALAXIES

@inproceedings{Aravena2016THEAS,
  title={THE ALMA SPECTROSCOPIC SURVEY IN THE HUBBLE ULTRA DEEP FIELD : SEARCH FOR [ C II ] LINE AND DUST EMISSION IN 6 < z < 8 GALAXIES},
  author={Manuel Aravena and Roberto Decarli and Fabian Walter and Rychard J. Bouwens and Pascal A. Oesch and Christopher L. Carilli and Franz Erik Bauer and Elisabete da Cunha and Emanuele Daddi and Jorge Gonzalez-Lopez and R J Ivison and Dominik Alexander Riechers and Ian R. Smail and A. Mark Swinbank and Axel Wei\ss and Timo Anguita and Roland Bacon and Eric Bell and F. de Bertoldi and Paulo C. Cort{\'e}s and Pierre Cox and Jacqueline Hodge and Eduardo Ibar and Hanae Inami and Leopoldo Infante and Alexander Karim and B. Magnelli and Kazuaki Ota and G. Popping and Paul P. van der Werf and Jeff Wagg and Yoshinobu Fudamoto},
  year={2016}
}
We present a search for [C II] line and dust continuum emission from optical dropout galaxies at z>6 using ASPECS, our Atacama Large Millimeter submillimeter Array Spectroscopic Survey in the Hubble Ultra-deep Field (UDF). Our observations, which cover the frequency range of 212–272 GHz, encompass approximately the range of 6<z<8 for [C II] line… CONTINUE READING