Hubble Space Telescope Imaging Polarimetry of the Gravitational Lens FSC 10214+4724

  title={Hubble Space Telescope Imaging Polarimetry of the Gravitational Lens FSC 10214+4724},
  author={Hien Nguyen and Peter R. Eisenhardt and Michael W. Werner and Robert W. Goodrich and David W. Hogg and Lee Armus and Baruch T. Soifer and Gerry X. Neugebauer},
  journal={The Astronomical Journal},
  pages={671 - 676}
We present imaging polarimetry of the extremely luminous, redshift 2.3 IRAS source FSC 10214+4724. The observations were obtained with HST's Faint Object Camera in the F437M filter, which is free of strong emission lines. The 0.″7 long arc is unresolved to 0.″04 FWHM in the transverse direction and has an integrated polarization of 28% ± 3%, in good agreement with ground-based observations. The polarization position angle varies along the arc by up to 35°. The overall position angle is 62° ± 3… 

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Ultraviolet Spectropolarimetry of Narrow-Line Radio Galaxies

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The preferentially magnified active nucleus in IRAS F10214+4724 – I. Lens model and spatially resolved radio emission

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We present a ≈20 ks Chandra ACIS-S observation of the strongly lensed z = 2.285 ultraluminous infrared galaxy FSC 10214 + 4724. Although this observation achieves the equivalent sensitivity of an up

Hubble Space Telescope NICMOS Observations of Rest-Frame Optical Continuum and Hα + [N I] Emission in FSC 10214+4724

High-resolution 1.10, 2.05, 2.12, and 2.15 μm imaging of the gravitationally lensed system FSC 10214+4724 are presented. These data extend Hubble Space Telescope (HST) observations of the lens system



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We present polarimetric evidence that the extraordinarily luminous galaxy FSC 10214+4724 harbors a hidden QSO. In polarized flux we see broad emission lines of C III] λ1909, C IV λ1550, and Lyα/N V

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Optical and near-IR images of the extremely luminous high-redshift IRAS source F10214+4724 both show a compact core surrounded by diffuse emission. The diffuse emission contains ∼12 per cent of the

The relationship between infrared, optical, and ultraviolet extinction

The parameterized extinction data of Fitzpatrick and Massa (1986, 1988) for the ultraviolet and various sources for the optical and near-infrared are used to derive a meaningful average extinction

HST Imaging Polarimetry of NGC 1068

The ultraviolet-to-radio continuum of the ultraluminous galaxy IRAS F10214+4724.

We present new observations and theoretical models for the continuous ultraviolet-to-radio spectrum of the ultraluminous protogalaxy candidate IRAS F 10214 + 4724. The radio spectrum at 1.49-8.44 GHz

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The conditions that prevail in the regions immediately surrounding the active nuclei in a sample of 20 nearby Seyfert galaxies are reported. Three of the nine Seyfert 1s show extended ionized gas

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