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Stanford, S. A. |
Volume |
Paper Title |
Page Number |
Authors |
14 |
Longslit IR Spectroscopy of Interacting Galaxies |
56 |
Stanford, S. A. |
26 |
Dust Formation; Chromospheres in R Coronae Borealis Stars: How Where; Why? |
481 |
Clayton, G. C.; Whitney, B. A.; Stanford, S. A. |
146 |
An JR-Selected Galaxy Cluster at Z = 1.27 |
514 |
Stanford, S. A.; Elston, R.; Eisenhardt, P. R.; Spinrad, H.; Stern, D.; Dev, A. |
193 |
Ultra-Steep Spectrum Radio Galaxies at Hy Redshifts |
44 |
van Breugel, W.; De Breuck, C.; Stanford, S. A.; Röttgering, H.; Miley, G.; Stern, D.; Minniti, D.; Carilli, C. |
193 |
NICMOS Imaging of High-Redshift Radio Galaxies |
114 |
Zirm, A.; Dey, A.; Dickinson, M.; McCarthy, P. J.; Eisenhardt, P.; Djorgovski, S. G.; Spinrad, H.; Stanford, S. A.; van Breugel, W. |
193 |
Morphological Evolution in High Redshift Galaxy Clusters |
304 |
Stanford, S. A. |
268 |
X-Ray Temperature and Morphology of z>0.8 Clusters of Galaxies |
35 |
Holden, B.; Stanford, S. A.; Rosati, P.; Tozzi, P.; Squires, G.; Borgani, S.; Eisenhardt, P. |
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