A dataset provided by the European Space Agency

Name 12022
Title The chemical composition of AGN outflows
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=12022;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-93q70iw
Author Kaastra, Jelle
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=12022&mission=hst
Publication
  • A Generative Model for Quasar Spectra
  • AGN winds as probes of cosmic feedback: the case of Mrk 509
  • Bias in C IV-based quasar black hole mass scaling relationships from reverberation mapped samples
  • Calibrating C-IV-based Black Hole Mass Estimators
  • Characterizing the UV and X-ray Outflow in Mrk 509
  • C IV Line-width Anomalies: The Perils of Low Signal-to-noise Spectra
  • Extending the Calibration of C IV-based Single-epoch Black Hole Mass Estimators for Active Galactic Nuclei
  • Galactic-scale Absorption Outflow in the Low-luminosity Quasar IRAS F04250-5718: Hubble Space Telescope/Cosmic Origins Spectrograph Observations
  • Multiwavelength campaign on Mrk 509. II. Analysis of high-quality Reflection Grating Spectrometer spectra
  • Multiwavelength campaign on Mrk 509. I. Variability and spectral energy distribution
  • Multiwavelength campaign on Mrk 509. IV. Optical-UV-X-ray variability and the nature of the soft X-ray excess
  • Multiwavelength Campaign on Mrk 509 IX. Lower Limit on the Distance of the Absorber from HST COS and STIS Spectroscopy
  • Multiwavelength campaign on Mrk 509. IX. The Galactic foreground
  • Multiwavelength campaign on Mrk 509. V. Chandra-LETGS observation of the ionized absorber
  • Multiwavelength campaign on Mrk 509. VI. HST/COS observations of the far-ultraviolet spectrum
  • Multiwavelength campaign on Mrk 509. VIII. Location of the X-ray absorber
  • Multiwavelength campaign on Mrk 509. VII. Relative abundances of the warm absorber
  • Multiwavelength campaign on Mrk 509. XII. Broad band spectral analysis
  • Multiwavelength campaign on Mrk 509. XIV. Chandra HETGS spectra
  • Multiwavelength campaign on Mrk 509. X. Lower limit on the distance of the absorber from HST COS and STIS spectroscopy
  • Multiwavelength campaign on Mrk 509. XV. Global modeling of the broad emission lines in the optical, UV, and X-ray bands
  • Multiwavelength campaign on Mrk 509. XVI. Continued HST/COS monitoring of the far-ultraviolet spectrum
  • The Low-redshift Intergalactic Medium as Seen in Archival Legacy HST/STIS and FUSE Data
  • Winds in Mrk 509: A Common Origin for the X-ray and UV Ionized Gas?
Instrument COS, COS/FUV
Temporal Coverage 2009-12-10T02:35:28Z/2009-12-11T09:38:33Z
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.
Creator Contact https://support.cosmos.esa.int/esdc/index.php?/Tickets/Submit
Date Published 2010-12-11T16:35:13Z
Keywords Hubble, HST, HLA, HCV, ACS, COS, STIS, WFC3, FOC, FOS, HRS, NICMOS, WFPC, WFPC2
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Kaastra comma Jelle, 2010, 'The chemical composition of AGN outflows', 1.0, European Space Agency, https://doi.org/10.5270/esa-93q70iw