The Hubble Space Telescope and the high redshift universe

@inproceedings{Tanvir1997TheHS,
  title={The Hubble Space Telescope and the high redshift universe},
  author={Nial R. Tanvir and Alfonso Arag{\'o}n-Salamanca and Jasper V. Wall},
  year={1997}
}
Galaxy Population in a Cluster of Galaxies around the Radio Galaxy 3C 324 at z = 1.2
We discuss the properties of galaxies around the radio galaxy 3C 324 at z =1 .2 based on BV RI Kmulti-band imaging data. We have applied a photometric-redshift technique to objects in the 3C 324
New Constraints on the Molecular Gas in the Prototypical HyLIRGs BRI1202-0725 & BRI1335-0417
We present Karl G Jansky Very Large Array (VLA) observations of CO(2-1) line emission and rest-frame 250GHz continuum emission of the Hyper-Luminous IR Galaxies (HyLIRGs) BRI1202-0725 (z=4.69) and
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    Astronomical Telescopes + Instrumentation
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The James Webb Space Telescope (JWST) is the scientific successor to the Hubble Space Telescope. It is a cryogenic infrared space observatory with a 25 m2 aperture (6 m class) telescope that will
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One of the fundamental goals of modern Astronomy is to estimate the physical parameters of galaxies from images in different spectral bands. We present a hierarchical Bayesian model for obtaining age
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We present the burst ages for young stellar populations in a sample of six nearby (<10 Mpc) spiral galaxies using a differential pixel-based analysis of the ionized gas emission. We explore this as
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The Hubble Space Telescope (HST) finds galaxies whose Tolman dimming exceeds 10 mag. Could evolution alone explain these as our ancestor galaxies or could they be representatives of quite a different
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We present results from the multi-wavelength study of XMMU J1230.3+1339 at z�1. We analyze deep multi-band wide-field images from the Large Bin ocular Telescope, multi-object spectroscopy
The Massive Galaxy Cluster XMMU J1230.3+1339 at z ~ 1: Colour-magnitude relation, Butcher-Oemler e
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THE SPATIAL DISTRIBUTION FUNCTION OF GALAXIES AT HIGH REDSHIFT
This is the first exploration of the galaxy distribution function at redshifts greater than about 0.1. Redshifts are based on the North and South GOODS Catalogs. In each catalog we examine clustering
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