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

@article{Nguyen1998HubbleST,
  title={Hubble Space Telescope Imaging Polarimetry of the Gravitational Lens FSC 10214+4724},
  author={Hien Trong 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},
  year={1998},
  volume={117},
  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… 
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
The preferentially magnified active nucleus in IRAS F10214+4724 – I. Lens model and spatially resolved radio emission
This is the first paper in a series that presents a multiwavelength analysis of the archetype ultraluminous infrared galaxy IRAS F10214+4724, a gravitationally lensed, starburst/active galactic
The preferentially magnified active nucleus in IRAS F10214+4724 - III. VLBI observations of the radio core
We report 1.7 GHz very long baseline interferometry (VLBI) observations of IRAS F10214+4724, a lensed z = 2.3 obscured quasar with prodigious star formation. We detect what we argue to be the
A Chandra observation of the z= 2.285 galaxy FSC 10214+4724: evidence for a Compton-thick quasar?
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
Ultraviolet Spectropolarimetry of Narrow-Line Radio Galaxies
We present the results of UV spectropolarimetry (λrest ≃ 2000-3000 Å) and far-UV spectroscopy (λrest ≃ 1500-2000 Å) of two low-redshift narrow-line radio galaxies (NLRGs) taken with the Faint Object

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With a redshift of 2.3, the IRAS source FSC 10214+4724 is apparently one of the most luminous objects known in the universe. We present an image of FSC 10214+4724 at 0.8 μm obtained with the Hubble
High-Resolution Infrared Imaging of FSC 10214+4724: Evidence for Gravitational Lensing
We present near-infrared observations of the ultraluminous high-redshift (z = 2.286) IRAS source FSC 10214+4724 obtained in 0.″4 seeing at the W. M. Keck telescope. These observations show that FSC
Near-infrared imaging of FSC 10214+4724 with the W. M. Keck Telescope
Near-infrared observations of the z = 2.286 IRAS source FSC 10214+4724, made with the near-infrared camera on the W. M. Keck Telescope, are reported. Deep broad-band images at 2.15 and 1.27
IRAS F10214+4724: the inner 100 pc
We use new high-resolution near-infrared spectroscopy and our previously published optical spectroscopy of the gravitationally lensed Seyfert 2 galaxy F10214+4724 to study both the links between the
Extended Molecular Gas in FSC 10214+4724
We report high resolution imaging of the CO (3-2) emission in the luminous infrared source FSC 10214+4724 at z = 2.2853. Maps at resolutions of 2.″3 × 3.″0 and 45-90 km s-1 show the CO emission peak
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New observations with the IRAM interferometer of CO(3-2) from the highly luminous galaxy IRAS F10214+4724 show the source is 1.″5 × ≤0.″9; they display no evidence of any velocity gradient. This
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Near-infrared images of MG 1131+0456 with the W. M. Keck telescope: Another dusty gravitational lens?
Images of the gravitational lens system MG 1131+0456 taken with the near-infrared camera on the W. M. Keck telescope in the J and Ks bands show that the infrared counterparts of the compact radio
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FSC 10214+4724: A Gravitationally Lensed, Hidden QSO
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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