Hubble Space Telescope imaging of the large-redshift gravitational lens candidate 1208+1011

John N. Bahcall, Dan Maoz, Donald P. Schneider, Brian Yanny, Rodger Doxsey

Research output: Contribution to journalArticle

18 Citations (Scopus)

Abstract

Four-color photometry obtained with the Hubble Space Telescope is consistent with the hypothesis that the light from the quasar 1208+1011 (z = 3.8) is gravitationally lensed. Guided exposures taken with the HST Planetary Camera resolve the quasar image into two point-source components separated by 0″.476 ± 0″.004. The intensity ratio of the components is approximately 4:1 in each of four broad-band HST filters with mean wavelengths of 4352, 5416, 6898, and 8922 Å. The HST photometry, when combined with high-resolution ground-based spectroscopy, rules out the possibility that the secondary component is a Galactic star. The limit on additional point sources is 3% of the brighter image for separations greater than 0″.5 from the primary component and 5% of the brighter component for separations between 0″.1 and 0″.5. If the gravitational lens is an ordinary galaxy, it would not have been detected on the HST images.

Original languageEnglish (US)
JournalAstrophysical Journal
Volume392
Issue number1 PART 2
StatePublished - Jun 10 1992

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gravitational lenses
Hubble Space Telescope
point source
quasars
point sources
photometry
spectroscopy
filter
wavelength
cameras
galaxies
broadband
color
filters
stars
high resolution
wavelengths

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Bahcall, John N. ; Maoz, Dan ; Schneider, Donald P. ; Yanny, Brian ; Doxsey, Rodger. / Hubble Space Telescope imaging of the large-redshift gravitational lens candidate 1208+1011. In: Astrophysical Journal. 1992 ; Vol. 392, No. 1 PART 2.
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abstract = "Four-color photometry obtained with the Hubble Space Telescope is consistent with the hypothesis that the light from the quasar 1208+1011 (z = 3.8) is gravitationally lensed. Guided exposures taken with the HST Planetary Camera resolve the quasar image into two point-source components separated by 0″.476 ± 0″.004. The intensity ratio of the components is approximately 4:1 in each of four broad-band HST filters with mean wavelengths of 4352, 5416, 6898, and 8922 {\AA}. The HST photometry, when combined with high-resolution ground-based spectroscopy, rules out the possibility that the secondary component is a Galactic star. The limit on additional point sources is 3{\%} of the brighter image for separations greater than 0″.5 from the primary component and 5{\%} of the brighter component for separations between 0″.1 and 0″.5. If the gravitational lens is an ordinary galaxy, it would not have been detected on the HST images.",
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Hubble Space Telescope imaging of the large-redshift gravitational lens candidate 1208+1011. / Bahcall, John N.; Maoz, Dan; Schneider, Donald P.; Yanny, Brian; Doxsey, Rodger.

In: Astrophysical Journal, Vol. 392, No. 1 PART 2, 10.06.1992.

Research output: Contribution to journalArticle

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T1 - Hubble Space Telescope imaging of the large-redshift gravitational lens candidate 1208+1011

AU - Bahcall, John N.

AU - Maoz, Dan

AU - Schneider, Donald P.

AU - Yanny, Brian

AU - Doxsey, Rodger

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N2 - Four-color photometry obtained with the Hubble Space Telescope is consistent with the hypothesis that the light from the quasar 1208+1011 (z = 3.8) is gravitationally lensed. Guided exposures taken with the HST Planetary Camera resolve the quasar image into two point-source components separated by 0″.476 ± 0″.004. The intensity ratio of the components is approximately 4:1 in each of four broad-band HST filters with mean wavelengths of 4352, 5416, 6898, and 8922 Å. The HST photometry, when combined with high-resolution ground-based spectroscopy, rules out the possibility that the secondary component is a Galactic star. The limit on additional point sources is 3% of the brighter image for separations greater than 0″.5 from the primary component and 5% of the brighter component for separations between 0″.1 and 0″.5. If the gravitational lens is an ordinary galaxy, it would not have been detected on the HST images.

AB - Four-color photometry obtained with the Hubble Space Telescope is consistent with the hypothesis that the light from the quasar 1208+1011 (z = 3.8) is gravitationally lensed. Guided exposures taken with the HST Planetary Camera resolve the quasar image into two point-source components separated by 0″.476 ± 0″.004. The intensity ratio of the components is approximately 4:1 in each of four broad-band HST filters with mean wavelengths of 4352, 5416, 6898, and 8922 Å. The HST photometry, when combined with high-resolution ground-based spectroscopy, rules out the possibility that the secondary component is a Galactic star. The limit on additional point sources is 3% of the brighter image for separations greater than 0″.5 from the primary component and 5% of the brighter component for separations between 0″.1 and 0″.5. If the gravitational lens is an ordinary galaxy, it would not have been detected on the HST images.

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