A New Approach to Detailed Structural Decomposition from the SPLASH and PHAT Surveys: Kicked-up Disk Stars in the Andromeda Galaxy?
A Sub-2% Distance to M31 from Photometrically Homogeneous Near-infrared Cepheid Period-Luminosity Relations Measured with the Hubble Space Telescope
Cepheids in M31: The PAndromeda Cepheid Sample
Infrared Tip of the Red Giant Branch and Distances to the Maffei/IC 342 Group
On the Progenitors of Local Group Novae. II. The Red Giant Nova Rate of M31
On the Progenitors of Local Group Novae. I. The M31 Catalog
PHAT Stellar Cluster Survey. I. Year 1 Catalog and Integrated Photometry
Rebirth of X-Ray Emission from the Born-again Planetary Nebula A30
Supernova Remnant Progenitor Masses in M31
The impact of satellite trails on Hubble Space Telescope observations
The Panchromatic Hubble Andromeda Treasury
The Panchromatic Hubble Andromeda Treasury. II. Tracing the Inner M31 Halo with Blue Horizontal Branch Stars
The Panchromatic Hubble Andromeda Treasury. V. Ages and Masses of the Year 1 Stellar Clusters
Instrument
ACS, ACS/WFC, WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage
2010-07-12T16:38:43Z/2011-01-01T09:41:54Z
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., 2011, 'A Panchromatic Hubble Andromeda Treasury - I', 1.0, European Space Agency, https://doi.org/10.5270/esa-q7nr3da