The Extragalactic Distance Scale Key Project. XVIII. The Discovery of Cepheids and a New Distance to NGC 4535 Using theHubble Space Telescope

1999 ◽  
Vol 521 (1) ◽  
pp. 155-178 ◽  
Author(s):  
L. M. Macri ◽  
J. P. Huchra ◽  
P. B. Stetson ◽  
N. A. Silbermann ◽  
W. L. Freedman ◽  
...  
1994 ◽  
Vol 428 ◽  
pp. 143 ◽  
Author(s):  
Shaun M. G. Hughes ◽  
Peter B. Stetson ◽  
Anne Turner ◽  
Robert C., Jr. Kennicutt ◽  
Robert Hill ◽  
...  

1996 ◽  
Vol 463 ◽  
pp. 26 ◽  
Author(s):  
Daniel D. Kelson ◽  
Garth D. Illingworth ◽  
Wendy F. Freedman ◽  
John A. Graham ◽  
Robert Hill ◽  
...  

1997 ◽  
Vol 478 (1) ◽  
pp. 430-430 ◽  
Author(s):  
Daniel D. Kelson ◽  
Garth D. Illingworth ◽  
Wendy F. Freedman ◽  
John A. Graham ◽  
Robert Hill ◽  
...  

1999 ◽  
Vol 183 ◽  
pp. 17-30 ◽  
Author(s):  
Wendy L. Freedman ◽  
Jeremy R. Mould ◽  
Robert C. Kennicutt ◽  
Barry F. Madore

A Joint Discussion on the extragalactic distance scale and the Hubble constant took place fifteen years ago, at the 1982 XVIIIth General Assembly of the IAU, held in Patras, Greece. At that time, the newest applications of infrared photometers to Tully-Fisher measurements (Aaronson 1983) and Cepheid distances (Madore 1983) were reported. CCDs were just coming into use and had not yet been applied to extragalactic distance determinations; all of the extragalactic Cepheid distances were based on photographic Argelander (eye-estimated) photometry (Tammann and Sandage 1983 and references therein). No Cepheid distances to type Ia supernova-host galaxies were available.


1995 ◽  
Vol 155 ◽  
pp. 258-259
Author(s):  
S. M. G. Hughes

AbstractAs part of the Extragalactic Distance Scale Key Project, the Hubble Space Telescope has been used to identify Cepheids in M100, M101 and NGC925, and to measure distances derived from the Cepheid PL relation. For M100, the distance of 17.1 ± 1.8 Mpc has been used to infer a preliminary value for H0 of ~ 80 km/s/Mpc, which brings the age of the Universe derived from the standard model of the Big Bang into conflict with the ages of the oldest stars.


1989 ◽  
Vol 111 ◽  
pp. 169-176
Author(s):  
Jeremy Mould

For three quarters of a century pulsating variable stars have lain at the foundation of the extragalactic distance scale. The construction of larger telescopes, advances in detector technology, hard work by observers, and our understanding of stellar structure have all contributed to the expansion of the realm of the Cepheids to the distance of M101. Now, with the advent of Hubble Space Telescope (HST), we can look forward to the detection of Cepheids in the Virgo cluster and the removal of much of the remaining uncertainty in the Hubble constant.


1996 ◽  
Vol 470 ◽  
pp. 1 ◽  
Author(s):  
N. A. Silbermann ◽  
Paul Harding ◽  
Barry F. Madore ◽  
Robert C., Jr. Kennicutt ◽  
Abhijit Saha ◽  
...  

2009 ◽  
Vol 5 (H15) ◽  
pp. 1-16 ◽  
Author(s):  
W. L. Freedman ◽  
R. C. Kennicutt ◽  
J. R. Mould

AbstractTen years ago our team completed the Hubble Space Telescope Key Project on the extragalactic distance scale. Cepheids were detected in some 25 galaxies and used to calibrate four secondary distance indicators that reach out into the expansion field beyond the noise of galaxy peculiar velocities. The result was H0 = 72 ± 8 km s−1 Mpc−1 and put an end to galaxy distances uncertain by a factor of two. This work has been awarded the Gruber Prize in Cosmology for 2009.


1994 ◽  
Vol 427 ◽  
pp. 628 ◽  
Author(s):  
Wendy L. Freedman ◽  
Shaun M. Hughes ◽  
Barry F. Madore ◽  
Jeremy R. Mould ◽  
Myung Gyoon Lee ◽  
...  

1996 ◽  
Vol 464 ◽  
pp. 568 ◽  
Author(s):  
Laura Ferrarese ◽  
Wendy L. Freedman ◽  
Robert J. Hill ◽  
Abhijit Saha ◽  
Barry F. Madore ◽  
...  

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