The infrared surface brightness fluctuation hubble constant

Joseph B. Jensen, John L. Tonry, Rodger I Thompson, Edward A. Ajhar, Tod R. Lauer, Marcia J Rieke, Marc Postman, Michael C. Liu

Research output: Contribution to journalArticle

32 Citations (Scopus)

Abstract

We measured infrared surface brightness fluctuation (SBF) distances to an isotropically distributed sample of 16 distant galaxies with redshifts reaching 10,000 km s-1 using the near-IR camera and multi-object spectrometer (NICMOS) on the Hubble Space Telescope (HST). The excellent spatial resolution, very low background, and brightness of the IR fluctuations yielded the most distant SBF measurements to date. Twelve nearby galaxies were also observed and used to calibrate the F160W (1.6 μm) SBF distance scale. Of these, three have Cepheid variable star distances measured with HST and eleven have optical I-band SBF distance measurements. A distance modulus of 18.5 mag to the Large Magellanic Cloud was adopted for this calibration. We present the F160W SBF Hubble diagram and find a Hubble constant H0 = 76 ± 1.3 (1 σ statistical) ±6 (systematic) km s-1 Mpc-1. This result is insensitive to the velocity model used to correct for local bulk motions. Restricting the fit to the six most distant galaxies yields the smallest value of H0 = 72 ± 2.3 km s-1 Mpc-1 that is consistent with the data. This 6% decrease in the Hubble constant is consistent with the hypothesis that the Local Group inhabits an underdense region of the universe, but is also consistent with the best-fit value of H0 = 76 km s-1 Mpc-1 at the 1.5 σ level.

Original languageEnglish (US)
Pages (from-to)503-521
Number of pages19
JournalAstrophysical Journal
Volume550
Issue number2 PART 1
StatePublished - Apr 1 2001

Fingerprint

Hubble constant
brightness
galaxies
Hubble Space Telescope
cepheid variables
Hubble diagram
variable stars
Magellanic clouds
spatial resolution
spectrometer
diagram
calibration
universe
cameras
spectrometers

Keywords

  • Cosmological parameters
  • Distance scale
  • Galaxies: distances and redshifts
  • Large-scale structure of universe

ASJC Scopus subject areas

  • Space and Planetary Science

Cite this

Jensen, J. B., Tonry, J. L., Thompson, R. I., Ajhar, E. A., Lauer, T. R., Rieke, M. J., ... Liu, M. C. (2001). The infrared surface brightness fluctuation hubble constant. Astrophysical Journal, 550(2 PART 1), 503-521.

The infrared surface brightness fluctuation hubble constant. / Jensen, Joseph B.; Tonry, John L.; Thompson, Rodger I; Ajhar, Edward A.; Lauer, Tod R.; Rieke, Marcia J; Postman, Marc; Liu, Michael C.

In: Astrophysical Journal, Vol. 550, No. 2 PART 1, 01.04.2001, p. 503-521.

Research output: Contribution to journalArticle

Jensen, JB, Tonry, JL, Thompson, RI, Ajhar, EA, Lauer, TR, Rieke, MJ, Postman, M & Liu, MC 2001, 'The infrared surface brightness fluctuation hubble constant', Astrophysical Journal, vol. 550, no. 2 PART 1, pp. 503-521.
Jensen JB, Tonry JL, Thompson RI, Ajhar EA, Lauer TR, Rieke MJ et al. The infrared surface brightness fluctuation hubble constant. Astrophysical Journal. 2001 Apr 1;550(2 PART 1):503-521.
Jensen, Joseph B. ; Tonry, John L. ; Thompson, Rodger I ; Ajhar, Edward A. ; Lauer, Tod R. ; Rieke, Marcia J ; Postman, Marc ; Liu, Michael C. / The infrared surface brightness fluctuation hubble constant. In: Astrophysical Journal. 2001 ; Vol. 550, No. 2 PART 1. pp. 503-521.
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