Halos of Spiral Galaxies. II. Halo Metallicity-Luminosity Relation
Halos of Spiral Galaxies. III. Metallicity Distributions
Halos of Spiral Galaxies. I. The Tip of the Red Giant Branch as a Distance Indicator
Is NGC 300 a pure exponential disk galaxy?
Metallicity-corrected Tip of the Red Giant Branch Distance to NGC 4258
Stellar Disks and Halos of Edge-on Spiral Galaxies: NGC 891, NGC 4144, and NGC 4244
The Carnegie-Chicago Hubble Program. IX. Calibration of the Tip of the Red Giant Branch Method in the Megamaser Host Galaxy, NGC 4258 (M106)
The Extragalactic Distance Scale without Cepheids
The Globular Cluster Systems of Five Nearby Spiral Galaxies: New Insights from Hubble Space Telescope Imaging
The Outskirts of Spiral Galaxies: Evidence for Multiple Stellar Populations
The Stellar Content and Star Formation History of the Late-Type Spiral Galaxy NGC 300 from Hubble Space Telescope Observations
The structure and environment of young stellar clusters in spiral galaxies
Thick disks and halos of spiral galaxies M 81, NGC 55 and NGC 300
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
2001-06-11T06:28:14Z/2001-10-04T01:19:35Z
Version
1.0
Mission Description
Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited.
European Space Agency, Ferguson comma Harry C., 2002, 'Investigating the Formation History of Spiral Galaxy Halos', 1.0, European Space Agency, https://doi.org/10.5270/esa-mfejxmr