A comparison between the soft X-ray and O III morphologies of active galactic nuclei
A SITELLE view of M31s central region - I. Calibrations and radial velocity catalogue of nearly 800 emission-line point-like sources
High-resolution mapping of dust via extinction in the M31 bulge
Hubble Space Telescope Snapshot Search for Planetary Nebulae in Globular Clusters of the Local Group
Optical and UV Spectra of the Remnant of SN 1885 (S And) in M31
Photometric evidence of an intermediate-age stellar population in the inner bulge of M31
Planetary nebulae in the circumnuclear region of M31: a spectroscopic sample
The 2D Distribution of Iron-rich Ejecta in the Remnant of SN 1885 in M31
The impact of satellite trails on Hubble Space Telescope observations
The Panchromatic Hubble Andromeda Treasury. VII. The Steep Mid-ultraviolet to Near-infrared Extinction Curve in the Central 200 pc of the M31 Bulge
Instrument
ACS, ACS/WFC, WFC3, WFC3/UVIS
Temporal Coverage
2010-12-21T13:10:23Z/2011-01-02T20:52:22Z
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, Li comma Zhiyuan, 2012, 'An HST/WFC3 mapping of optical emission lines from the nuclear spiral in M31', 1.0, European Space Agency, https://doi.org/10.5270/esa-vckmdzx