A spiral galaxys mass distribution uncovered through lensing and dynamics
Strong lensing constraints on modified gravity models
The first detection of neutral hydrogen in emission in a strong spiral lens
The SWELLS survey - I. A large spectroscopically selected sample of edge-on late-type lens galaxies
The SWELLS survey - II. Breaking the disc-halo degeneracy in the spiral galaxy gravitational lens SDSS J2141-0001
The SWELLS survey - IV. Precision measurements of the stellar and dark matter distributions in a spiral lens galaxy
The SWELLS survey - V. A Salpeter stellar initial mass function in the bulges of massive spiral galaxies
Instrument
WFPC2, WFPC2/PC, WFPC2/WFC
Temporal Coverage
2009-02-18T10:41:12Z/2009-04-25T22:48:52Z
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, Treu et al., 2010, 'Luminous and dark matter in disk galaxies from strong lensing and stellar kinematics', 1.0, European Space Agency, https://doi.org/10.5270/esa-vy1n72y