Constraints on the Field Star IMF from Resolved Stellar Populations Based Star Formation Histories
Faint dwarfs as a test of DM models: WDM versus CDM
Finding e Car Analogs in Nearby Galaxies Using Spitzer. II. Identification of An Emerging Class of Extragalactic Self-Obscured Stars
How Typical Are the Local Group Dwarf Galaxies?
MUSE crowded field 3D spectroscopy in NGC 300. I. First results from central fields
NGC 404: A Rejuvenated Lenticular Galaxy on a Merger-induced, Blueward Excursion Into the Green Valley
Reversal of Fortune: Increased Star Formation Efficiencies in the Early Histories of Dwarf Galaxies?
The ACS Nearby Galaxy Survey Treasury. VIII. The Global Star Formation Histories of 60 Dwarf Galaxies in the Local Volume
The Chandra Local Volume Survey. I. The X-Ray Point Source Populations of NGC 55, NGC 2403, and NGC 4214
Transient X-Ray Source Population in the Magellanic-type Galaxy NGC 55
Instrument
WFPC2, WFPC2/PC, WFPC2/WFC
Temporal Coverage
2007-07-28T12:49:16Z/2008-07-06T14:24:37Z
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, Dalcanton et al., 2008, 'Completing the ACS Nearby Galaxy Survey with WFPC2', 1.0, European Space Agency, https://doi.org/10.5270/esa-6duwnee