Allan Rex Sandage
Affiliations: | Mount Wilson-Palomar |
Area:
CosmologyWebsite:
https://baas.aas.org/pub/allan-r-sandage-1926-2010Google:
"Allan Rex Sandage"Bio:
(1926 - 2010)
https://en.wikipedia.org/wiki/Allan_Sandage
Sandage, Allan A study of the globular cluster M3. Dissertation (Ph.D.), California Institute of Technology (1953).
Mean distance: (not calculated yet)
Parents
Sign in to add mentor| Walter Baade | grad student | 1953 | Caltech | |
| (A study of the globular cluster M3.) | ||||
| Edwin Powell Hubble | grad student | 1950-1953 | Mount Wilson and Palomar Observatories (Astronomy Tree) | |
| Martin Schwarzschild | grad student | 1951-1953 | Princeton | |
Children
Sign in to add trainee| R. Michael Rich | research assistant | UCLA | |
| Howard H. Lanning | research assistant | 1971 | Carnegie Institution of Washington (Astronomy Tree) |
| Robert LeRoy Wildey | grad student | 1962 | Caltech (Astronomy Tree) |
| Philippe Véron | post-doc | ||
| Donald Lynden-Bell | post-doc | 1962 | Mount Wilson-Palomar |
| Nicholas B. Suntzeff | post-doc | 1982-1986 | Carnegie Institution of Science |
| Clarence Roger Lynds | research scientist | 1961-1963 | Kitt Peak National Observatory (Astronomy Tree) |
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Publications
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| Sandage A, Beaton RL, Majewski SR. (2016) Comparison of Hipparcos Trigonometric and Mount Wilson Spectroscopic Parallaxes for 90 Subgiants that Defined the Class in 1935 Publications of the Astronomical Society of the Pacific. 128: 64202 |
| Tammann GA, Reindl B, Sandage A. (2011) New period-luminosity and period-color relations of classical Cepheids - IV. The low-metallicity galaxies IC 1613, WLM, Pegasus, Sextans A and B, and Leo A in comparison to SMC Astronomy and Astrophysics. 531 |
| Sandage A. (2010) Amplitude Fine Structure In The Cepheid P-L Relation. I. Amplitude Distribution Across The Rr Lyrae Instability Strip Mapped Using The Accessibility Restriction Imposed By The Horizontal Branch The Astrophysical Journal. 722: 79-87 |
| Sandage A, Reindl B, Tammann GA. (2010) THE LINEARITY OF THE COSMIC EXPANSION FIELD FROM 300 TO 30,000 km s–1 AND THE BULK MOTION OF THE LOCAL SUPERCLUSTER WITH RESPECT TO THE COSMIC MICROWAVE BACKGROUND The Astrophysical Journal. 714: 1441-1459 |
| Sandage A. (2010) The Tolman Surface Brightness Test for the Reality of the Expansion. V. Provenance of the Test and a New Representation of the Data for Three Remote Hubble Space Telescope Galaxy Clusters The Astronomical Journal. 139: 728-742 |
| Sandage A, Tammann GA. (2008) Temperature Differences in the Cepheid Instability Strip Require Differences in the Period-Luminosity Relation in Slope and Zero Point The Astrophysical Journal. 686: 779-784 |
| Tammann GA, Sandage A, Reindl B. (2008) Comparison of Distances from RR Lyrae Stars, the Tip of the Red Giant Branch, and Classical Cepheids The Astrophysical Journal. 679: 52-70 |
| Tammann GA, Sandage A, Reindl B. (2008) The expansion field: the value of H 0 The Astronomy and Astrophysics Review. 15: 289-331 |
| Sandage A, Tammann GA. (2006) Absolute Magnitude Calibrations of Population I and II Cepheids and Other Pulsating Variables in the Instability Strip of the Hertzsprung-Russell Diagram Annual Review of Astronomy and Astrophysics. 44: 93-140 |
| Sandage A, Tammann GA, Saha A, et al. (2006) The Hubble Constant: A Summary of the Hubble Space Telescope Program for the Luminosity Calibration of Type Ia Supernovae by Means of Cepheids The Astrophysical Journal. 653: 843-860 |