HiZELS:a high-redshift survey of Hα emitters - II. the nature of star-forming galaxies at z = 0.84

@article{Sobral2009HiZELSaHS,
  title={HiZELS:a high-redshift survey of H$\alpha$ emitters - II. the nature of star-forming galaxies at z = 0.84},
  author={David Sobral and Philip N. Best and James E. Geach and I. R. Smail and Jaron Daniel Kurk and Michele Cirasuolo and Mark M. Casali and R. J. Ivison and K. E. K. Coppin and G. B. Dalton IfA Edinburgh and Durham and Mpia and Eső and IfA University of Edinburgh and Oxford},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2009},
  volume={398},
  pages={75-90}
}
  • D. Sobral, P. Best, +12 authors Oxford
  • Published 26 January 2009
  • Physics
  • Monthly Notices of the Royal Astronomical Society
New results from a large survey of Hα emission-line galaxies at z = 0.84 using the Wide Field Camera on the United Kingdom Infrared Telescope and a custom narrow-band filter in the J band are presented as part of the High-z Emission Line Survey (HiZELS). The deep narrow-band images reach an effective flux limit of F Hα ∼ 10 -16 erg s -1 cm -2 in a comoving volume of 1.8 × 10 5 Mpc 3, resulting in the largest and deepest survey of its kind ever done at z ∼ 1. There are 1517 potential line… 
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References

SHOWING 1-10 OF 48 REFERENCES
HiZELS: a high-redshift survey of Hα emitters – I. The cosmic star formation rate and clustering at z= 2.23
We present results from a near-infrared narrow-band survey of emission-line galaxies at z = 2.23, using the Wide Field Camera on the United Kingdom Infrared Telescope. The H2S1 narrow-band filter (
The Hα Luminosity Function and Star Formation Rate at z ~ 0.24 Based on Subaru Deep Imaging Data
We have carried out a deep imaging survey for Hα-emitting galaxies at z ≈ 0.24 using a narrowband filter tuned with the redshifted line. The total sky area covered is 706 arcmin2 within a redshift
The Hα Luminosity Function and Star Formation Rate at z ≈ 0.24 in the COSMOS 2 Square Degree Field*
To derive a new Hα luminosity function and to understand the clustering properties of star-forming galaxies at z≈ 0.24, we have made a narrowband imaging survey for Hα-emitting galaxies in the Hubble
On near-infrared Hα searches for high-redshift galaxies⋆
The lack of success of Lyman-alpha searches for high-redshift (z>2) field galaxies may be due to extinction by dust, suggesting that surveys based on lines of longer wavelength, particularly H-alpha,
Star formation density and Hα luminosity function of an emission-line-selected galaxy sample at z∼ 0.24*
We use narrow-band imaging (full width at half-maximum = 70 A) to select a sample of emission-line galaxies between 0.20 ≤ z ≤ 1.22 in two fields covering 0.5 deg 2 . We use spectroscopic follow-up
The Luminosity Function and Star Formation Rate between Redshifts of 0.07 and 1.47 for Narrowband Emitters in the Subaru Deep Field
SDF line-emitting galaxies in four narrowband filters at low and intermediate redshifts are presented. Broadband colors, follow-up optical spectroscopy, and multiple NB filters are used to
zCOSMOS: A Large VLT/VIMOS Redshift Survey Covering 0 < z < 3 in the COSMOS Field*
zCOSMOS is a large-redshift survey that is being undertaken in the COSMOS field using 600 hr of observation with the VIMOS spectrograph on the 8 m VLT. The survey is designed to characterize the
The Hα luminosity function and star formation rate up to z ∼ 1 ⋆
We describe ISAAC/ESO-VLT observations of the Ha λ6563 Balmer line of 33 field galaxies from the Canada-France Redshift Survey (CFRS) with redshifts selected between 0.5 and 1.1. We detect Ha in
THE WYOMING SURVEY FOR Hα. I. INITIAL RESULTS AT z ∼ 0.16 AND 0.24
The Wyoming Survey for Hα, or WySH, is a large-area, ground-based, narrowband imaging survey for Hα-emitting galaxies over the latter half of the age of the universe. The survey spans several square
Star-Forming Galaxies at z ≈ 0.24 in the Subaru Deep Field and the Sloan Digital Sky Survey
We make a search for Halpha emitting galaxies at z=0.24 in the Subaru Deep Field (SDF) using the archival data set obtained with the Subaru Telescope. We carefully select Halpha emitters in the
...
1
2
3
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5
...