Characterizing the Circumgalactic Medium of Nearby Galaxies with HST/COS and HST/STIS Absorption-line Spectroscopy. II. Methods and Models
Chemical abundances along the quasar main sequence
Reporting a deficit of intrinsic N V absorbers in core-dominated radio-loud quasars
Signatures of gas flows - I. Connecting the kinematics of the H I circumgalactic medium to galaxy rotation
The Warm-Hot Disk-Halo Interface below the Perseus Spiral Arm
The XMM-Newton/HST View of the Obscuring Outflow in the Seyfert Galaxy Mrk 335 Observed at Extremely Low X-Ray Flux
Tracking the year-to-year variation in the spectral energy distribution of the narrow-line Seyfert 1 galaxy Mrk 335
Instrument
COS, COS/FUV
Temporal Coverage
2016-01-04T03:06:56Z/2016-01-07T06:05:41Z
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, Longinotti, 2017, 'The rise of an ionized outflow in the X-ray and UV spectra of the NLS1 Mrk 335', 1.0, European Space Agency, https://doi.org/10.5270/esa-303col1
Rights
Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.