Chandra, EUVE, HST, and VLA Multiwavelength Campaign on HR 1099: Instrumental Capabilities, Data Reduction, and Initial Results
Chemical Consequences of the C/O Ratio on Hot Jupiters: Examples from WASP-12b, CoRoT-2b, XO-1b, and HD 189733b
Constraints on the Structure of the Heliospheric Interface Based on Ly a Absorption Spectra
CoolCAT
Coronal Emission Measures and Abundances for Moderately Active K Dwarfs Observed by Chandra
Correlating Intrinsic Stellar Parameters with Mg II Self-reversal Depths
Dependence of Heliospheric Lya Absorption on the Interstellar Magnetic Field
Detection of magnetic dipole lines of Fexii in the ultraviolet spectrum of the dwarf star e Eri
Disentangling Stellar and Airglow Emission Lines from Hubble Space Telescope (HST) Cosmic Origins Spectrograph (COS) Spectra
Evolution of the Solar Activity over Time and Effects on Planetary Atmospheres. I. High-Energy Irradiances (1-1700 A)
Evolution of the Solar Activity Over Time and Effects on Planetary Atmospheres. II. k1 Ceti, an Analog of the Sun when Life Arose on Earth
Inhomogeneity within Local Interstellar Clouds
In the Trenches of the Solar-Stellar Connection. VII. Wilson-Bappu 2022
In the Trenches of the Solar-Stellar Connection. VI. Total EclipSS
Lya Absorption from Heliosheath Neutrals
Mg II h + k Flux--Rotational Period Correlation for G-type Stars
New Mass-Loss Measurements from Astrospheric Lya Absorption
One Year in the Life of Young Suns: Data-constrained Corona-wind Model of k1 Ceti
Physical structure of the local interstellar medium
Reconstructing the XUV Spectra of Active Sun-like Stars Using Solar Scaling Relations with Magnetic Flux
Space Telescope Imaging Spectrograph Survey of Far-Ultraviolet Coronal Forbidden Lines in Late-Type Stars
Stellar Lya Emission Lines in the Hubble Space Telescope Archive: Intrinsic Line Fluxes and Absorption from the Heliosphere and Astrospheres
Suppressed Far-UV Stellar Activity and Low Planetary Mass Loss in the WASP-18 System
The Curious Case of the Alpha Persei Corona: A Dwarf in Supergiants Clothing?
The emission line near 1319 A in solar and stellar spectra
The Evolution of Solar Flux from 0.1 nm to 160 mm: Quantitative Estimates for Planetary Studies
The interstellar cloud surrounding the Sun: a new perspective
The SOHO-Stellar Connection
The Structure of the Local Interstellar Medium. I. High-Resolution Observations of Fe II, Mg II, and Ca II toward Stars within 100 Parsecs
The Structure of the Local Interstellar Medium. III. Temperature and Turbulence
The Structure of the Local Interstellar Medium. II. Observations of D I, C II, N I, O I, Al II, and Si II toward Stars within 100 Parsecs
The three-dimensional physical structure of the local interstellar medium
Ultraviolet Spectroscopy of Rapidly Rotating Solar-Mass Stars: Emission-line Redshifts as a Test of the Solar-Stellar Connection
UV and EUV observations of stellar coronal structure and activity
What Is the Total Deuterium Abundance in the Local Galactic Disk?
X-Ray and Ultraviolet Spectroscopy of Intermediate-Mass, First Crossing Giants
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA, STIS/NUV-MAMA
Temporal Coverage
1999-05-01T19:56:37Z/2000-10-03T06:31:47Z
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, Ayres comma Thomas R., 2000, 'Origins, Structure and Evolution of Magnetic Activity in the Cool Half of the H-R Diagram: A STIS Survey', 1.0, European Space Agency, https://doi.org/10.5270/esa-pbk16ix
