(Q58908717)

P. Santini

10

0 references

Emanuele Giallongo

E. Giallongo

8

0 references

Vincenzo Testa

V. Testa

6

0 references

Mauro Giavalisco

9

M. Giavalisco

0 references

Anton Koekemoer

3

A. M. Koekemoer

0 references

Adriano Fontana

4

A. Fontana

0 references

author name string

A. Grazian

1

0 references

L. Pentericci

5

0 references

K. Boutsia

Astronomy and Astrophysics

7

0 references

language of work or name

English

0 references

publication date

18 July 2011

0 references

published in

1 reference

SIMBAD

volume

532

1 reference

SIMBAD

page(s)

33–33

1 reference

The Hubble Ultra Deep Field

SIMBAD

cites work

1 reference

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Galaxy Size Evolution at High Redshift and Surface Brightness Selection Effects: Constraints from the Hubble Ultra Deep Field

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DISCOVERY OFz∼ 8 GALAXIES IN THE HUBBLE ULTRA DEEP FIELD FROM ULTRA-DEEP WFC3/IR OBSERVATIONS

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z ∼ 7 galaxy candidates from NICMOS observations over the HDF-South and the CDF-South and HDF-North GOODS fields

21 January 2018

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A spectroscopic search for leaking Lyman continuum at z ~ 0.7

21 January 2018

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Spectroscopy of luminous z > 7 galaxy candidates and sources of contamination in z > 7 galaxy searches

21 January 2018

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Evidence of a fast evolution of the UV luminosity function beyond redshift 6 from a deep HAWK-I survey of the GOODS-S field

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The bright end of the z ~ 7 UV luminosity function from a wide and deep HAWK-I survey

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Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Likelihoods and Parameters from the WMAP data

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The Size Evolution of High-Redshift Galaxies

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On the Stellar Populations and Evolution of Star-forming Galaxies at 6.3 < z ⩽ 8.6

21 January 2018

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The lack of intense Ly{alpha} in ultradeep spectra of z = 7 candidates in GOODS-s: imprint of reionization?

21 January 2018

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The Rest-Frame Ultraviolet Luminosity Density of Star-forming Galaxies at Redshifts z > 3.5

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Seven-year Wilkinson Microwave Anisotropy Probe (WMAP) observations: cosmological interpretation

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The Star Formation History of Field Galaxies

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Evidence for strong evolution of the cosmic star formation density at high redshifts

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Galaxies at z = 6-9 from the WFC3/IR imaging of the Hubble Ultra Deep Field

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The UDF05 Follow‐up of the Hubble Ultra Deep Field. I. The Faint‐End Slope of the Lyman Break Galaxy Population atz∼ 5

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The UDF05 follow-up of the Hubble Ultra Deep Field. II. Constraints on reionization from z-dropout galaxies

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z∼ 7 GALAXIES IN THE HUDF: FIRST EPOCH WFC3/IR RESULTS

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A deep Hubble Space Telescope search for escaping Lyman continuum flux at z ~ 1.3: evidence for an evolving ionizing emissivity

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Cosmic Variance in the Great Observatories Origins Deep Survey

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Spectroscopic observations of Lyman break galaxies at redshifts ~4, 5, and 6 in the GOODS-South Field

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The great observatories origins deep survey: constraints on the Lyman continuum escape fraction distribution of lyman-break galaxies at 3.4 < z < 4.5

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Spectroscopic confirmation of two Lyman break galaxies at redshift beyond 7

21 January 2018

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Evolving Spectra of Population III Stars: Consequences for Cosmological Reionization

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The Hubble Space Telescope Wide Field Camera 3 Early Release Science data: panchromatic faint object counts for 0.2-2 {mu}m wavelength

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Probing very bright end of galaxy luminosity function at z >~ 7 using Hubble space telescope pure parallel observations

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