The dependence of star formation activity on environment and stellar mass at z∼ 1 from the HiZELS-Hα survey†

  1. David Sobral1,*,
  2. Philip N. Best1,
  3. Ian Smail2,
  4. James E. Geach2,
  5. Michele Cirasuolo1,3,
  6. Timothy Garn1,
  7. Gavin B. Dalton4,5

Article first published online: 25 OCT 2010

DOI: 10.1111/j.1365-2966.2010.17707.x

Issue

Monthly Notices of the Royal Astronomical Society

Monthly Notices of the Royal Astronomical Society

Volume 411, Issue 1, pages 675–692, February 2011

Additional Information

How to Cite

Sobral, D., Best, P. N., Smail, I., Geach, J. E., Cirasuolo, M., Garn, T. and Dalton, G. B. (2011), The dependence of star formation activity on environment and stellar mass at z∼ 1 from the HiZELS-Hα survey. Monthly Notices of the Royal Astronomical Society, 411: 675–692. doi: 10.1111/j.1365-2966.2010.17707.x

Author Information

  1. 1

    SUPA, Institute for Astronomy, Royal Observatory of Edinburgh, Blackford Hill, Edinburgh EH9 3HJ

  2. 2

    Institute for Computational Cosmology, Durham University, South Road, Durham DH1 3LE

  3. 3

    Astronomy Technology Centre, Royal Observatory of Edinburgh, Blackford Hill, Edinburgh EH9 3HJ

  4. 4

    Astrophysics, Department of Physics, Keble Road, Oxford OX1 3RH

  5. 5

    Space Science and Technology, Rutherford Appleton Laboratory, HSIC, Didcot OX11 0QX

* E-mail: drss@roe.ac.uk

  1. †

    Based on observations obtained using the Wide Field Camera on the 3.8-m United Kingdom Infrared Telescope, as part of the High-z Emission Line Survey (HiZELS).

Publication History

  1. Issue published online: 21 JAN 2011
  2. Article first published online: 25 OCT 2010
  3. Accepted 2010 September 14. Received 2010 August 25; in original form 2010 July 15

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