Dark and Baryonic Matter in Bright Spiral Galaxies. I. Near-Infrared and Optical Broadband Surface Photometry of 30 Galaxies
Gaps in the Cloud Cover? Comparing Extinction Measures in Spiral Disks
The Discovery of Cepheids and a New Distance to NGC 2841 Using the Hubble Space Telescope
The Opacity of Spiral Galaxy Disks. IV. Radial Extinction Profiles from Counts of Distant Galaxies Seen through Foreground Disks
The opacity of spiral galaxy disks. V. Dust opacity, HI distributions and sub-mm emission
The opacity of spiral galaxy disks. VI. Extinction, stellar light and color
The Opacity of Spiral Galaxy Disks. VIII. Structure of the Cold ISM
The opacity of spiral galaxy disks. VII. The accuracy of galaxy counts as an extinction probe
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
2000-02-29T08:27:14Z/2000-04-19T14:10:34Z
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, Bothun comma Gregory D., 2001, 'The Distance to NGC 2841: Improving the TF Calibration and Definitively Testing MOND', 1.0, European Space Agency, https://doi.org/10.5270/esa-dgt1dom