A comprehensive catalogue of OB cluster candidates in M31 and their association with giant molecular clouds
A New Approach to Detailed Structural Decomposition from the SPLASH and PHAT Surveys: Kicked-up Disk Stars in the Andromeda Galaxy?
Cepheids in M31: The PAndromeda Cepheid Sample
Cosmic ray detection on resolved galaxies with deep learning
Discovery of Weak CN Stars in the Large Magellanic Cloud and Comparison to Stellar Models
Evidence for a Hot Galactic Halo around the Andromeda Galaxy Using Fast Radio Bursts along Two Sightlines
Hubble Space Telescope Imaging of the Outburst Site of M31 RV. II. No Blue Remnant in Quiescence
Infrared Tip of the Red Giant Branch and Distances to the Maffei/IC 342 Group
Large Magellanic Cloud Near-infrared Synoptic Survey. II. The Wesenheit Relations and Their Application to the Distance Scale
M31 Planetary nebulae as seen by the Panchromatic Hubble Andromeda Treasury
Mass-to-light Ratios of Spatially Resolved Stellar Populations in M31
Measuring Star Formation Histories, Distances, and Metallicities with Pixel Color-Magnitude Diagrams. II. Applications to Nearby Elliptical Galaxies
Measuring Star Formation Histories from Asymptotic Giant Branch Stars. I. A Demonstration in M31
MUSE integral-field spectroscopy towards the Frontier Fields cluster Abell S1063. I. Data products and redshift identifications
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
Optical Emission from Luminous and Very Soft X-Ray Sources in Nearby Galaxies: Testing the Scenario of Edge-on Supercritical Accretion Systems
PAndromeda--First Results from the High-cadence Monitoring of M31 with Pan-STARRS 1
PHAT Stellar Cluster Survey. I. Year 1 Catalog and Integrated Photometry
PHAT. XIX. The Ancient Star Formation History of the M31 Disk
Photometric evidence of an intermediate-age stellar population in the inner bulge of M31
Pixel Color Magnitude Diagrams for Semi-resolved Stellar Populations: The Star Formation History of Regions within the Disk and Bulge of M31
Ring or No Ring--Revisiting the Multiphase Nuclear Environment in M31
Spatially Resolved Metal Loss from M31
Star Clusters in M31. V. Internal Dynamical Trends: Some Troublesome, Some Reassuring
Supersoft X-rays reveal a classical nova in the M 31 globular cluster Bol 126
The 2D Distribution of Iron-rich Ejecta in the Remnant of SN 1885 in M31
The dust in M31
The impact of satellite trails on Hubble Space Telescope observations
The Panchromatic Hubble Andromeda Treasury
The Panchromatic Hubble Andromeda Treasury. I. Bright UV Stars in the Bulge of M31
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
The Progenitor Systems of Classical Novae in M31
The Red Supergiant Progenitor Luminosity Problem
The spectral energy distributions of very long-period Cepheids in the Milky Way, the Magellanic Clouds, M31, and M33
The survey of planetary nebulae in Andromeda (M 31). III. Constraints from deep planetary nebula luminosity functions on the origin of the inner halo substructures in M 31
Variable Stars in M31 Stellar Clusters from the Panchromatic Hubble Andromeda Treasury
Instrument
ACS, ACS/WFC, WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage
2010-07-21T19:30:53Z/2011-01-03T15:32:13Z
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-3h7byu3
