A deep X-ray view of the bare AGN Ark 120. V. Spin determination from disc-Comptonisation efficiency method, Porquet, D.,Done, C.,Reeves, J. N., Astronomy and Astrophysics, 623, 2019-03-01 00:00:00, 2019A&A...623A..11P||An XMM-Newton observation of Ark 120: the X-ray spectrum of a `bare' Seyfert 1 nucleus, Vaughan, S.,Fabian, A. C.,Ballantyne, D. R., Monthly Notices of the Royal Astronomical Society, 351, 2004-06-01 00:00:00, 2004MNRAS.351..193V||A Relation between Supermassive Black Hole Mass and Quasar Metallicity?, Warner, Craig,Hamann, Fred,Dietrich, Matthias, The Astrophysical Journal, 596, 2003-10-01 00:00:00, 2003ApJ...596...72W||A Uniform Analysis of the Lyα Forest at z = 0-5. III. Hubble Space Telescope Faint Object Spectrograph Spectral Atlas, Bechtold, Jill,Dobrzycki, Adam,Wilden, Brenda, The Astrophysical Journal Supplement Series, 140, 2002-06-01 00:00:00, 2002ApJS..140..143B||A Uniform Analysis of the Lyα Forest at z = 0-5. IV. The Clustering and Evolution of Clouds at z <= 1.7, Dobrzycki, Adam,Bechtold, Jill,Scott, Jennifer, The Astrophysical Journal, 571, 2002-06-01 00:00:00, 2002ApJ...571..654D||A Uniform Analysis of the Lyα Forest at z=0-5. V. The Extragalactic Ionizing Background at Low Redshift, Scott, Jennifer,Bechtold, Jill,Morita, Miwa, The Astrophysical Journal, 571, 2002-06-01 00:00:00, 2002ApJ...571..665S||Bias in C IV-based quasar black hole mass scaling relationships from reverberation mapped samples, Brotherton, Michael S.,Runnoe, J. C.,Shang, Zhaohui, Monthly Notices of the Royal Astronomical Society, 451, 2015-08-01 00:00:00, 2015MNRAS.451.1290B||Broad-line region physical conditions along the quasar eigenvector 1 sequence, Marziani, P.,Sulentic, J. W.,Negrete, C. A., Monthly Notices of the Royal Astronomical Society, 409, 2010-12-01 00:00:00, 2010MNRAS.409.1033M||Calibrating C-IV-based Black Hole Mass Estimators, Park, Daeseong,Woo, Jong-Hak,Denney, Kelly D., The Astrophysical Journ...al, 770, 2013-06-01 00:00:00, 2013ApJ...770...87P||Calibrating Mg II-based Black Hole Mass Estimators with Hβ Reverberation Measurements, Bahk, Hyeonguk,Woo, Jong-Hak,Park, Daeseong, The Astrophysical Journal, 875, 2019-04-01 00:00:00, 2019ApJ...875...50B||C IV Line-width Anomalies: The Perils of Low Signal-to-noise Spectra, Denney, K. D.,Pogge, R. W.,Assef, R. J., The Astrophysical Journal, 775, 2013-09-01 00:00:00, 2013ApJ...775...60D||Determining Central Black Hole Masses in Distant Active Galaxies and Quasars. II. Improved Optical and UV Scaling Relationships, Vestergaard, Marianne,Peterson, Bradley M., The Astrophysical Journal, 641, 2006-04-01 00:00:00, 2006ApJ...641..689V||Emission Line Properties of Active Galactic Nuclei from a Post-COSTAR Hubble Space Telescope Faint Object Spectrograph Spectral Atlas, Kuraszkiewicz, Joanna K.,Green, Paul J.,Crenshaw, D. Michael, The Astrophysical Journal Supplement Series, 150, 2004-01-01 00:00:00, 2004ApJS..150..165K||Estimating black hole masses: Accretion disk fitting versus reverberation mapping and single epoch, Campitiello, Samuele,Celotti, Annalisa,Ghisellini, Gabriele, Astronomy and Astrophysics, 640, 2020-08-01 00:00:00, 2020A&A...640A..39C||Estimating Black Hole Masses in Active Galactic Nuclei Using the Mg II λ2800 Emission Line, Wang, Jian-Guo,Dong, Xiao-Bo,Wang, Ting-Gui, The Astrophysical Journal, 707, 2009-12-01 00:00:00, 2009ApJ...707.1334W||Extending the Calibration of C IV-based Single-epoch Black Hole Mass Estimators for Active Galactic Nuclei, Park, Daeseong,Barth, Aaron J.,Woo, Jong-Hak, The Astrophysical Journal, 839, 2017-04-01 00:00:00, 2017ApJ...839...93P||Intrinsic Absorption Lines in Seyfert 1 Galaxies. I. Ultraviolet Spectra from the Hubble Space Telescope, Crenshaw, D. Michael,Kraemer, Steven B.,Boggess, Albert, The Astrophysical Journal, 516, 1999-05-01 00:00:00, 1999ApJ...516..750C||Linking the power sources of emission-line galaxy nuclei from the highest to the lowest redshifts, Constantin, Anca, Ph.D. Thesis, 0, 2004-01-01 00:00:00, 2004PhDT........25C||Observational constraints on the structure and evolution of quasars, Kelly, Brandon C., Ph.D. Thesis, 0, 2008-01-01 00:00:00, 2008PhDT.........1K||Strong Correlation between Fe II/Mg II Ratio and Eddington Ratio of Type 1 Active Galactic Nuclei, Shin, Jaejin,Woo, Jong-Hak,Nagao, Tohru, The Astrophysical Journal, 917, 2021-08-01 00:00:00, 2021ApJ...917..107S||Supermassive Black Hole Mass Estimates Using Sloan Digital Sky Survey Quasar Spectra at 0.7 < z < 2, Rafiee, Alireza,Hall, Patrick B., The Astrophysical Journal Supplement Series, 194, 2011-06-01 00:00:00, 2011ApJS..194...42R||The Intermediate-ionization Lines as Virial Broadening Estimators for Population A Quasars, Marziani, Paola,Olmo, Ascensión del,Negrete, Castalia Alenka, The Astrophysical Journal Supplement Series, 261, 2022-08-01 00:00:00, 2022ApJS..261...30M||The Rise of an Ionized Wind in the Narrow-line Seyfert 1 Galaxy Mrk 335 Observed by XMM-Newton and HST, Longinotti, A. L.,Krongold, Y.,Kriss, G. A., The Astrophysical Journal, 766, 2013-04-01 00:00:00, 2013ApJ...766..104L||Ultraviolet and Optical Properties of Narrow-Line Seyfert 1 Galaxies, Constantin, Anca,Shields, Joseph C., Publications of the Astronomical Society of the Pacific, 115, 2003-05-01 00:00:00, 2003PASP..115..592C||Virial Masses of Black Holes from Single Epoch Spectra of Active Galactic Nuclei, Kelly, Brandon C.,Bechtold, Jill, The Astrophysical Journal Supplement Series, 168, 2007-01-01 00:00:00, 2007ApJS..168....1K||Weighing supermassive black holes, Rafiee, Alireza, Ph.D. Thesis, 0, 2010-01-01 00:00:00, 2010PhDT........56R||What controls the CIV line profile in active galactic nuclei?, Baskin, Alexei,Laor, Ari, Monthly Notices of the Royal Astronomical Society, 356, 2005-01-01 00:00:00, 2005MNRAS.356.1029B
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.
