A small and vigorous black hole in the early Universe
CLASSY. II. A Technical Overview of the COS Legacy Archive Spectroscopic Survey
CLASSY III. The Properties of Starburst-driven Warm Ionized Outflows
CLASSY IV. Exploring UV Diagnostics of the Interstellar Medium in Local High-z Analogs at the Dawn of the JWST Era
CLASSY. IX. The Chemical Evolution of the Ne, S, Cl, and Ar Elements
CLASSY. VIII. Exploring the Source of Ionization with UV Interstellar Medium Diagnostics in Local High-z Analogs
CLASSY VII Lya Profiles: The Structure and Kinematics of Neutral Gas and Implications for LyC Escape in Reionization-era Analogs
CLASSY. VI. The Density, Structure, and Size of Absorption-line Outflows in Starburst Galaxies
CLASSY V: The Impact of Aperture Effects on the Inferred Nebular Properties of Local Star-forming Galaxies
CLASSY. X. Highlighting Differences between Partial Covering and Semianalytic Modeling in the Estimation of Galactic Outflow Properties
CLASSY XII: nitrogen enrichment shaped by gas density and feedback
CLASSY. XI. Tracing Neutral Gas Properties Using UV Absorption Lines and 21 cm Observations
GN-z11 in Context: Possible Signatures of Globular Cluster Precursors at Redshift 10
Inferring the presence of very massive stars in local star-forming regions
Interpreting the Si II and C II Line Spectra from the COS Legacy Archive Spectroscopic SurveY Using a Virtual Galaxy from a High-resolution Radiation-hydrodynamic Simulation
New ionization models and the shocking nitrogen excess at z > 5
Only Nitrogen-enhanced Galaxies Have Detectable Ultraviolet Nitrogen Emission Lines at High Redshift
On the Average Ultraviolet Emission-line Spectra of High-redshift Galaxies: Hot and Cold, Carbon-poor, Nitrogen Modest, and Oozing Ionizing Photons
Physical Origins of Outflowing Cold Clouds in Local Star-forming Dwarf Galaxies
Shining a Light on the Connections between Galactic Outflows Seen in Absorption and Emission Lines
The COS Legacy Archive Spectroscopy Survey (CLASSY) Treasury Atlas
The Second Case of a Major Merger Triggering a Starburst in a Green Pea Galaxy
Under Pressure: Decoding the Effect of High Densities on Derived Nebular Properties
What Are the Radial Distributions of Density, Outflow Rates, and Cloud Structures in the M82 Wind?
Instrument
COS, COS/FUV, COS/NUV
Temporal Coverage
2019-12-16T23:54:37Z/2020-10-29T05:43:59Z
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, Berg, 2020, 'The COS Legacy Archive Spectroscopic SurveY (CLASSY): A UV Treasury of Star-Forming Galaxies', 1.0, European Space Agency, https://doi.org/10.5270/esa-zjzge4r