The Discovery of Two Lyman α Emitters beyond Redshift 6 in the Subaru Deep Field

@article{Kodaira2003TheDO,
  title={The Discovery of Two Lyman $\alpha$ Emitters beyond Redshift 6 in the Subaru Deep Field},
  author={Keiichi Kodaira and Yoshiaki Taniguchi and Nobunari Kashikawa and Norio Kaifu and Hiroyasu Ando and Hiroshi Karoji and et al.},
  journal={Publications of the Astronomical Society of Japan},
  year={2003},
  volume={55}
}
We performed a deep optical imaging survey using a narrow-band filter (NB921) centered at λ=9196 u A together 

Figures and Tables from this paper

The escape of ionizing photons from supernova-dominated primordial galaxies
In order to assess the contribution of Lyman break galaxies (LBGs) and Lyman α emitters (LAEs) at redshifts 3 6. That implies that additional ionization sources may be required at z > 6.
Probing the universe at redshift 10 and beyond
Abstract The signature of objects in the very early universe lies deep in the near infrared bands. The Primordial Explorer ( PRIME ) is a proposed NASA Explorer-class mission aimed at the z  > 10
THE LYMAN ALPHA MORPHOLOGY OF LOCAL STARBURST GALAXIES: RELEASE OF CALIBRATED IMAGES
We present reduced and calibrated high resolution Lyman-alpha (Lyα) images for a sample of six local star-forming galaxies. Targets were selected to represent a range in luminosity and metallicity ...
A Lyman α emitter at z = 6.5 found with slitless spectroscopy
We report the discovery of a Lyman α emitting galaxy at z = 6.518. The single line was found in the 43 arcmin 2 VLT/FORS field by slitless spectroscopy limited to the atmospheric window at λ ∼ 9100 A
Narrowband survey of the goods fields : Search for Lyα emitters at z = 5.7
We present results from optical narrowband (λc = 8150 A and Δλ = 120 A) observations of the Great Observatories Origins Deep Survey (GOODS) fields, using Suprime-Cam on the Subaru Telescope. Using
A Luminous Lyα-emitting Galaxy at Redshift z = 6.535: Discovery and Spectroscopic Confirmation*
We present a redshift z = 6.535 galaxy discovered by its Lyα emission in a 9180 A narrowband image from the Large Area Lyman Alpha survey. The Lyα line luminosity (1.1 × 1043 ergs s-1) is among the
Lyα Emission-Line Galaxies at z = 3.1 in the Extended Chandra Deep Field-South
We describe the results of an extremely deep, 0.28 deg^2 survey for z = 3.1 Ly-alpha emission-line galaxies in the Extended Chandra Deep Field South. By using a narrow-band 5000 Anstrom filter and
The Wide Field Imager Lyman-Alpha Search (WFILAS) for galaxies at redshift ~5.7: II. Survey design and sample analysis
Context. Wide-field narrowband surveys are an efficient way of searching large volumes of high-redshift space for distant galaxies. Aims. We describe the Wide Field Imager Lyman-Alpha Search (WFILAS)
A very large telescope FORS2 multislit search for Lyα-emitting galaxies at z ∼ 6.5
We present results from a deep spectroscopic search in the 9150 A atmospheric window for z ~ 6.5 Lyα-emitting galaxies using the VLT/FORS2. Our multislit+narrowband filter survey covers a total
A Strong Lyα Emitter at z = 6.33 in the Subaru Deep Field Selected as an i'-Dropout*
We report on the discovery of a star-forming galaxy at z = 6.33 in the Subaru Deep Field. This object is selected as a candidate of an i'-dropout high-redshift galaxy around z = 6 because of its red
...
1
2
3
4
5
...

References

SHOWING 1-10 OF 32 REFERENCES
Lyman Alpha Imaging of a Proto-Cluster Region at =3.09
We present very deep imaging observations, through a narrow-band filter tuned to Lyman alpha at , of a volume containing a significant over-density of galaxies at this redshift previously discovered
Discovery of 9 ly alpha emitters at redshift Z 3.1 using narrow-band imaging and vlt spectroscopy
Narrowband imaging surveys aimed at detecting the faint emission from the 5007 A [O III] line of intracluster planetary nebulae in Virgo also probe high-redshift z ~ 3.1 Lyα emitters. Here we report
The discovery of a very narrow line star-forming object at a redshift of 5.66
We report on the discovery of a very narrow line star-forming object beyond a redshift of 5. Using the prime-focus camera, Suprime-Cam, on the 8.2 m Subaru Telescope together with a narrow-passband
High-z Lyα Emitters. I. A Blank-Field Search for Objects near Redshift z = 3.4 in and around the Hubble Deep Field and the Hawaii Deep Field SSA 22*
We present deep narrowband (λ = 5390 A, Δλ = 77 A) and multicolor observations of the Hubble Deep Field and the Hawaii Deep Field SSA 22 obtained with the LRIS instrument at the 10 m Keck II
Subaru Deep Survey. II. Luminosity Functions and Clustering Properties of Lyα Emitters at z = 4.86 in the Subaru Deep Field*
We report on early results from very deep and wide-field narrowband imaging on a 543 arcmin2 area of the Subaru Deep Field. We find 87 Lyα emitters (LAEs) at z = 4.86 ± 0.03 that are photometrically
HIGH-z Lya EMITTERS. I. A BLANK-FIELD SEARCH FOR OBJECTS NEAR REDSHIFT z \ 3.4 IN AND AROUND THE HUBBLE DEEP FIELD AND THE HAWAII DEEP FIELD SSA 221
We present deep narrowband (j \ 5390 *j \ 77 and multicolor observations of the Hubble Ae ,A e ) Deep Field and the Hawaii Deep Field SSA 22 obtained with the LRIS instrument at the 10 m Keck II
Approaching Reionization: The Evolution of the Lyα Forest from z = 4 to z = 6
We analyze the Lyα forest properties of a sample of 15 high-redshift quasars lying between z = 4.42 and z = 5.75, using high signal-to-noise spectra obtained with the Echellette Spectrograph and
One-Line Redshifts and Searches for High-Redshift Lyα Emission*
We report the serendipitous discovery of two objects close in projection with fairly strong emission lines at long wavelength (? ~ 9190 ?). One (A) seems not to be hosted by any galaxy brighter than
Detection of Lyman-α-emitting galaxies at redshift 4.55
STUDIESof the formation and early history of galaxies have been hampered by the difficulties inherent in detecting faint galaxy populations at high redshift. As a consequence, observations at the
The Evolution of the Global Star Formation History as Measured from the Hubble Deep Field
The Hubble Deep Field (HDF) is the deepest set of multicolor optical photometric observations ever undertaken, and it offers a valuable data set with which to study galaxy evolution. Combining the
...
1
2
3
4
...