Description

New measurements of the Hα luminosity function (LF) and star formation rate

(SFR) volume density are presented for galaxies at z∼0.62 in the COSMOS field.

These results are part of the Dee

New measurements of the Hα luminosity function (LF) and star formation rate

(SFR) volume density are presented for galaxies at z∼0.62 in the COSMOS field.

These results are part of the Deep And Wide Narrowband Survey (DAWN), a unique

infrared imaging program with large areal coverage (∼1.1 deg 2 over 5 fields) and

sensitivity (9.9 × 10 −18 erg/cm 2 /s at 5σ).

The present sample, based on a single DAWN field, contains 116 Hα emission-

line candidates at z∼0.62, 25% of which have spectroscopic confirmations. These

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    Contributors
    Date Created
    • 2017
    Resource Type
  • Text
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    Note
    • Partial requirement for: M.S., Arizona State University, 2017
      Note type
      thesis
    • Includes bibliographical references (pages 34-35)
      Note type
      bibliography
    • Field of study: Astrophysics

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    by Alicia Gonzalez

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