Lyman Break Galaxy Candidates in the Sloan Digital Sky Survey First Data Release

نویسنده

  • David H. Weinberg
چکیده

We report the discovery of six compact, starburst galaxy candidates with redshifts 2.3 < z < 2.8 and r-band magnitudes 19.8−20.5 in the Quasar Catalog of the Sloan Digital Sky Survey First Data Release (SDSS DR1). The SDSS spectra of these objects resemble the composite spectrum of Lyman Break Galaxies (LBGs) at z ≈ 3 (albeit with some differences and broader spectral lines), but the systems are 4− 5 magnitudes brighter than an “L∗” LBG and 2 − 3 magnitudes brighter than the most luminous objects in typical LBG spectroscopic surveys. These objects could be extremely luminous LBGs, normal LBGs amplified by gravitational lensing (like MS 1512-cB58), or a rare class of unusual BAL quasars. Under the first hypothesis, star formation rates inferred from the UV continuum luminosities are ∼ 300−1000 M⊙ yr −1 with no correction for dust extinction. Such rates are similar to those inferred for ultraluminous infrared galaxies, but in these UV-bright objects the star formation is evidently not obscured by high dust column densities. The SDSS images show no evidence of multiple imaging or foreground lensing structures, but lensing amplification cannot be ruled out with the present data. The spectra have fairly broad absorption features and prominent high-ionization absorption, but they do not have high ionization emission lines, nor do they resemble spectra of known BAL quasars. Assuming that lensing and AGN contributions are unimportant, we estimate the high end of the z ≈ 2.5 galaxy luminosity function, making the crude but conservative assumption of unit detection efficiency over our observed redshift and magnitude range. The estimated comoving space density, Φ(M) = 2.5× 10h Mpc mag at absolute magnitude MUV ≈ −25 (UV rest wavelength λ ≈ 7600Å/[1 + z]), is above a Schechter function extrapolation of the LBG luminosity function from fainter magnitudes. Improved optical spectra and measurements at X-ray, IR, and sub-mm wavelengths could help determine the nature of these remarkable objects. Subject headings: galaxies: starburst — surveys

برای دانلود رایگان متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

Lyman Break Galaxies in the Sloan Digital Sky Survey First Data Release

We report the discovery of six compact, starburst galaxies with redshifts 2.3 < z < 2.8 and r-band magnitudes 19.8−20.5 in the Quasar Catalog of the Sloan Digital Sky Survey First Data Release (SDSS DR1). The SDSS spectra of these objects resemble the composite spectrum of Lyman Break Galaxies (LBGs) at z ≈ 3, but the galaxies are 4−5 magnitudes brighter than an “L∗” LBG and 2 − 3 magnitudes br...

متن کامل

Rest-frame Mid-infrared Detection of an Extremely Luminous Lyman Break Galaxy with the Spitzer Infrared Spectrograph (irs)

We present the first rest-frame 4 m detection of a Lyman break galaxy. The data were obtained using the 16 m imaging capability of the Spitzer Infrared Spectrograph. The target object, J134026.44+634433.2, is an extremely luminous Lyman break galaxy at z 1⁄4 2:79, first identified in Sloan Digital Sky Survey (SDSS) spectra (as reported by Bentz et al.). The source is strongly detected with a fl...

متن کامل

20 04 Bright Lyman Break Galaxy Candidates in the Sloan Digital Sky Survey First Data Release

We report the discovery of six compact, starburst galaxy candidates with redshifts 2.3 < z < 2.8 and r-band magnitudes 19.8−20.5 in the Quasar Catalog of the SDSS DR1. The SDSS spectra resemble the composite spectrum of Lyman Break Galaxies (LBGs) at z ≈ 3 (albeit with some differences and broader spectral lines), but the objects are 4−5 magnitudes brighter than an “L∗” LBG. These objects could...

متن کامل

ar X iv : a st ro - p h / 04 06 18 5 v 1 7 J un 2 00 4 Rest - Frame MIR Detection of an Extremely Luminous Lyman Break Galaxy with the Spitzer IRS 12

We present the first rest-frame ∼ 4µm detection of a Lyman break galaxy. The data were obtained using the 16µm imaging capability of the Spitzer Infrared Spectrograph. The target object, J134026.44+634433.2, is an extremely luminous Lyman break galaxy at z=2.79 first identified in Sloan Digital Sky Survey spectra (Bentz, Osmer, & Weinberg 2004). The source is strongly detected with a flux of 0....

متن کامل

A Search for Radio Gravitational Lenses, Using the Sloan Digital Sky Survey and the Very Large Array

We report on a novel search for radio gravitational lenses. Using the Very Large Array, we imaged ten candidates with both dual redshifts in Sloan Digital Sky Survey spectra and 1.4 GHz radio flux ≥ 2 mJy in the FIRST survey. The VLA maps show that in each case the radio emission is associated with the foreground galaxy rather than being lensed emission from the background galaxy, although at l...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 2003