A New Sample of Transient Ultraluminous X-Ray Sources Serendipitously Discovered by Swift/XRT
An Ultraluminous Supersoft X-Ray Source in M81: An Intermediate-Mass Black Hole?
A Study of Cepheids in M81 with the Large Binocular Telescope (Efficiently Calibrated with Hubble Space Telescope)
Bulges of Nearby Galaxies with Spitzer: Scaling Relations in Pseudobulges and Classical Bulges
Calibrating X-Ray Binary Luminosity Functions via Optical Reconnaissance. II. The High-mass XLF and Globular Cluster Population of X-Ray Binaries in the Low Star-forming Spiral M81
Compact Optical Counterparts of Ultraluminous X-Ray Sources
Constraints for the Progenitor Masses of 17 Historic Core-collapse Supernovae
Cosmic-CoNN: A Cosmic-Ray Detection Deep-learning Framework, Data Set, and Toolkit
deepCR: Cosmic Ray Rejection with Deep Learning
Discovery of a radio transient in M81
Globular cluster systems in spiral galaxies
Hubble Space Telescope Photometry of Globular Clusters in M81
Luminous and Variable Stars in NGC 2403 and M81
On the nature of the brightest globular cluster in M81
Optical Counterparts of the Nearest Ultraluminous X-Ray Sources
Properties of the brightest globular cluster in M 81 based on multicolour observations
Quantitative Spectroscopy of Blue Supergiant Stars in the Disk of M81: Metallicity, Metallicity Gradient, and Distance
Roche-lobe Overflow Systems Powered by Black Holes in Young Star Clusters: The Importance of Dynamical Exchanges
Searching for Compact Star Clusters in M81 using HST/ACS images
Spectroscopic Studies of an Ultraluminous Supersoft X-Ray Source in M81
Structural Parameters of M81 Compact Star Clusters
Testing Density Wave Theory with Resolved Stellar Populations around Spiral Arms in M81
Testing Galaxy Formation Models with the GHOSTS Survey: The Color Profile of M81s Stellar Halo
The ACS Nearby Galaxy Survey Treasury
The GHOSTS survey - II. The diversity of halo colour and metallicity profiles of massive disc galaxies
The impact of satellite trails on Hubble Space Telescope observations
The Spitzer Local Volume Legacy: Survey Description and Infrared Photometry
The Tip of the Red Giant Branch Distances to Type Ia Supernova Host Galaxies. IV. Color Dependence and Zero-point Calibration
Uncloaking globular clusters in the inner galaxy
Wide-field HST/ACS images of M81: the population of compact star clusters
Wolf-Rayet stars in M81: detection and characterization using GTC/OSIRIS spectra and HST/ACS images
Wolf-Rayet stars in M 81 using GTC/OSIRIS: seven new detections, analysis, and classification of the full sample
Instrument
ACS, ACS/WFC, WFPC2, WFPC2/PC
Temporal Coverage
2005-12-05T06:26:16Z/2006-12-31T01:11:50Z
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, Zezas et al., 2007, 'The link between X-ray source and stellar populations in M81', 1.0, European Space Agency, https://doi.org/10.5270/esa-bgs9wu7