A 1.3% Distance to M33 from Hubble Space Telescope Cepheid Photometry
A First Look at Spatially Resolved Infrared Supernova Remnants in M33 with JWST
ALMA CO observations of a giant molecular cloud in M 33: Evidence for high-mass star formation triggered by cloud-cloud collisions
Classifying spectra of emission-line regions with neural networks: An application to integral field spectroscopic data of M33
Clusters, clouds, and correlations: relating young clusters to giant molecular clouds in M33 and M31
Deriving physical parameters of unresolved star clusters. VIII. Limits of aperture photometry for star cluster studies
Discovery of a Weak CN Spectral Absorption Feature in Red Supergiant Stars in the Andromeda (M31) and Triangulum (M33) Galaxies
Discovery of Weak CN Stars in the Large Magellanic Cloud and Comparison to Stellar Models
Hertzsprung gap stars in nearby galaxies and the quest for luminous red nova progenitors
JWST reveals star formation across a spiral arm in M33
Multiwavelength Characterization of the High-mass X-Ray Binary Population of M33
Optical Emission from Luminous and Very Soft X-Ray Sources in Nearby Galaxies: Testing the Scenario of Edge-on Supercritical Accretion Systems
Revealing Efficient Dust Formation at Low Metallicity in Extragalactic Carbon-rich Wolf-Rayet Binaries
Ring nebulae around Wolf-Rayet stars in M33 as seen by SITELLE
Searching for Balmer-dominated Type Ia Supernova Remnants in M33
The First Candidate Colliding-wind Binary in M33
The impact of satellite trails on Hubble Space Telescope observations
The Panchromatic Hubble Andromeda Treasury: Triangulum Extended Region (PHATTER). I. Ultraviolet to Infrared Photometry of 22 Million Stars in M33
The Panchromatic Hubble Andromeda Treasury: Triangulum Extended Region (PHATTER). IV. Star Cluster Catalog
The Panchromatic Hubble Andromeda Treasury: Triangulum Extended Region (PHATTER). VI. The High-mass Stellar Initial Mass Function of M33
The Panchromatic Hubble Andromeda Treasury: Triangulum Extended Region (PHATTER). V. The Structure of M33 in Resolved Stellar Populations
The Red Supergiant Binary Fraction as a Function of Metallicity in M31 and M33
The Samples and Binary Fractions of Red Supergiants in M31 and M33 by the HST Observations
The spatial correlation of high-mass X-ray binaries and young star clusters in nearby star-forming galaxies
The spectral energy distributions of very long-period Cepheids in the Milky Way, the Magellanic Clouds, M31, and M33
The TREX Survey: Kinematical Complexity Throughout M33s Stellar Disk and Evidence for a Stellar Halo
TREX: Kinematic Characterization of a High-dispersion Intermediate-age Stellar Component in M33
Instrument
ACS, ACS/WFC, WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage
2017-02-21T08:38:33Z/2018-02-25T12:27:20Z
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.
