The SBF Survey of Galaxy Distances. IV. SBF Magnitudes, Colors, and Distances

@article{Tonry2001TheSS,
  title={The SBF Survey of Galaxy Distances. IV. SBF Magnitudes, Colors, and Distances},
  author={J. Tonry and A. Dressler and J. Blakeslee and E. Ajhar and A. Fletcher and G. Luppino and M. Metzger and C. B. Moore},
  journal={The Astrophysical Journal},
  year={2001},
  volume={546},
  pages={681-693}
}
We report data for I-band surface brightness fluctuation (SBF) magnitudes, (V-I) colors, and distance moduli for 300 galaxies. The survey contains E, S0, and early-type spiral galaxies in the proportions of 49 : 42 : 9 and is essentially complete for E galaxies to Hubble velocities of 2000 km s-1, with a substantial sampling of E galaxies out to 4000 km s-1. The median error in distance modulus is 0.22 mag. We also present two new results from the survey. (1) We compare the mean peculiar flow… Expand

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Cosmic distances from surface brightness fluctuations
  • J. Blakeslee
  • Physics
  • Proceedings of the International Astronomical Union
  • 2012
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References

SHOWING 1-10 OF 31 REFERENCES
The Surface Brightness Fluctuation Survey of Galaxy Distances. II. Local and Large-Scale Flows* **
We present results from the Surface Brightness Fluctuation (SBF) Survey for the distances to 300 early-type galaxies, of which approximately half are ellipticals. A modest change in the zero point ofExpand
The sbf survey of galaxy distances. I. sample selection, photometric calibration, and the hubble constant
We describe a program of surface brightness fluctuation (SBF) measurements for determining galaxy distances. This paper presents the photometric calibration of our sample and of SBF in general.Expand
Theoretical predictions for surface brightness fluctuations and implications for stellar populations of elliptical galaxies
We compute theoretical predictions for surface brightness fluctuations (SBFs) of single-burst stellar populations (SSPs) using models optimized for this purpose. We present results over a wide rangeExpand
Detection of Surface Brightness Fluctuations in NGC 4373 Using the Hubble Space Telescope
Surface brightness fluctuations (SBF) have been detected for three elliptical galaxies-NGC 3379 in the Leo group, NGC 4406 in the Virgo cluster, and NGC 4373 in the Hydra-Centaurus supercluster-usingExpand
A Large-scale Bulk Flow of Galaxy Clusters
We report first results from the Streaming Motions of Abell Clusters (SMAC) project, an all-sky Fundamental Plane survey of 699 early-type galaxies in 56 clusters between ~3000 and ~14,000 km s-1.Expand
The far field hubble constant
We used the Hubble Space Telescope to obtain surface brightness fluctuation (SBF) observations of four nearby brightest cluster galaxies (BCGs) to calibrate the BCG Hubble diagram of Lauer & Postman.Expand
The Infrared Surface Brightness Fluctuation Distances to the Hydra and Coma Clusters
We present IR surface brightness fluctuation (SBF) distance measurements to NGC 4889 in the Coma Cluster and to NGC 3309 and NGC 3311 in the Hydra Cluster. We explicitly corrected for theExpand
The dependence of the brightness fluctuation distance indicator on stellar population age and metallicity
We describe how the extragalactic distance indicator L depends on stellar population age, metallicity, and IMF, assuming single-burst ages between 5 and 17 Gyr and metallicities between −0.5 and +0.5Expand
The Hubble Space Telescope Key Project on the Extragalactic Distance Scale. XXVI. The Calibration of Population II Secondary Distance Indicators and the Value of the Hubble Constant
A Cepheid-based calibration is derived for four distance indicators that utilize stars in old stellar populations: the tip of the red giant branch (TRGB), the planetary nebula luminosity functionExpand
The Hubble Space Telescope Key Project on the Extragalactic Distance Scale. XXVII. A Derivation of the Hubble Constant Using the Fundamental Plane and Dn-sigma; Relations in Leo I, Virgo and Fornax
Using published photometry and spectroscopy, we construct the fundamental plane and Dn-? relations in Leo I, Virgo, and Fornax. The published Cepheid period-luminosity (PL) relations to spirals inExpand
...
1
2
3
4
...