A dataset provided by the European Space Agency

Name 5182
Title UV SPECTROSCOPY OF LOW-REDSHIFT ACTIVE GALAXIES -- CYC 4
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=5182;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-ts4n49j
Author Boggess, Albert
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=5182&mission=hst
Publication
  • A deep X-ray view of the bare AGN Ark 120. V. Spin determination from disc-Comptonisation efficiency method
  • An XMM-Newton observation of Ark 120: the X-ray spectrum of a `bare Seyfert 1 nucleus
  • A Relation between Supermassive Black Hole Mass and Quasar Metallicity?
  • A Uniform Analysis of the Lya Forest at z = 0-5. III. Hubble Space Telescope Faint Object Spectrograph Spectral Atlas
  • A Uniform Analysis of the Lya Forest at z = 0-5. IV. The Clustering and Evolution of Clouds at z <= 1.7
  • A Uniform Analysis of the Lya Forest at z=0-5. V. The Extragalactic Ionizing Background at Low Redshift
  • Bias in C IV-based quasar black hole mass scaling relationships from reverberation mapped samples
  • Broad-line region physical conditions along the quasar eigenvector 1 sequence
  • Calibrating C-IV-based Black Hole Mass Estimators
  • Calibrating Mg II-based Black Hole Mass Estimators with Hb Reverberation Measurements
  • C IV Line-width Anomalies: The Perils of Low Signal-to-noise Spectra
  • Determining Central Black Hole Masses in Distant Active Galaxies and Quasars. II. Improved Optical and UV Scaling Relationships
  • Emission Line Properties of Active Galactic Nuclei from a Post-COSTAR Hubble Space Telescope Faint Object Spectrograph Spectral Atlas
  • Estimating black hole masses: Accretion disk fitting versus reverberation mapping and single epoch
  • Estimating Black Hole Masses in Active Galactic Nuclei Using the Mg II l2800 Emission Line
  • Extending the Calibration of C IV-based Single-epoch Black Hole Mass Estimators for Active Galactic Nuclei
  • Intrinsic Absorption Lines in Seyfert 1 Galaxies. I. Ultraviolet Spectra from the Hubble Space Telescope
  • Linking the power sources of emission-line galaxy nuclei from the highest to the lowest redshifts
  • Observational constraints on the structure and evolution of quasars
  • Strong Correlation between Fe II/Mg II Ratio and Eddington Ratio of Type 1 Active Galactic Nuclei
  • Supermassive Black Hole Mass Estimates Using Sloan Digital Sky Survey Quasar Spectra at 0.7 < z < 2
  • The Intermediate-ionization Lines as Virial Broadening Estimators for Population A Quasars
  • The Rise of an Ionized Wind in the Narrow-line Seyfert 1 Galaxy Mrk 335 Observed by XMM-Newton and HST
  • Ultraviolet and Optical Properties of Narrow-Line Seyfert 1 Galaxies
  • Virial Masses of Black Holes from Single Epoch Spectra of Active Galactic Nuclei
  • Weighing supermassive black holes
  • What controls the CIV line profile in active galactic nuclei?
Instrument FOS/BL
Temporal Coverage 1994-09-19T18:25:46Z/1995-07-29T20:48:17Z
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 1996-07-30T01:20:10Z
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, Boggess comma Albert, 1996, 'UV SPECTROSCOPY OF LOW-REDSHIFT ACTIVE GALAXIES -- CYC 4', 1.0, European Space Agency, https://doi.org/10.5270/esa-ts4n49j