Far-Ultraviolet Imaging of the Hubble Deep Field-North: Star Formation in Normal Galaxies atz < 1 | Zendy

Harry I. Teplitz | Zendy; Brian Siana | Zendy; T. M. Brown | Zendy; RangaRam Chary | Zendy; James Colbert | Zendy; Christopher J. Conselice | Zendy; D. F. de Mello | Zendy; Mark Dickinson | Zendy; Henry C. Ferguson | Zendy; Jonathan P. Gardner | Zendy; F. Menanteau | Zendy

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Far-Ultraviolet Imaging of the Hubble Deep Field-North: Star Formation in Normal Galaxies atz < 1

Author(s) -

Harry I. Teplitz,

Brian Siana,

T. M. Brown,

RangaRam Chary,

James Colbert,

Christopher J. Conselice,

D. F. de Mello,

Mark Dickinson,

Henry C. Ferguson,

Jonathan P. Gardner,

F. Menanteau

Publication year - 2006

Publication title -

the astronomical journal

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 2.61

H-Index - 271

eISSN - 1538-3881

pISSN - 0004-6256

DOI - 10.1086/505685

Subject(s) - physics , astrophysics , space telescope imaging spectrograph , galaxy , hubble deep field , advanced camera for surveys , redshift , cosmic variance , hubble ultra deep field , astronomy , star formation , extinction (optical mineralogy) , spiral galaxy , hubble deep field south , spectrograph , hubble space telescope , spectral line , optics

We present far-ultraviolet (FUV) imaging of the Hubble Deep Field North(HDF-N) taken with the Solar Blind Channel of the Advanced Camera for Surveys(ACS/SBC) and the FUV MAMA detector of the Space Telescope Imaging Spectrograph(STIS) onboard the Hubble Space Telescope. The full WFPC2 deep field has beenobserved at 1600 Angstroms. We detect 134 galaxies and one star down to a limitof FUV_{AB} ~ 29. All sources have counterparts in the WFPC2 image. Redshifts(spectroscopic or photometric) for the detected sources are in the range 0

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