Works matching Quasars
Results: 3066
The Quasar Saxophone Quartet: A Continuous Influence in Musical Creation for 25 Years!
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- Circuit: Musiques Contemporaines, 2019, v. 29, n. 3, p. 115
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Le quatuor de saxophones Quasar: un rayonnement continu de création musicale depuis 25 ans!
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- Circuit: Musiques Contemporaines, 2019, v. 29, n. 3, p. 55, doi. 10.7202/1066486ar
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Can Lorentz relativistic mass explain the lack of velocity time dilation in quasars?
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- Physics Essays, 2023, v. 36, n. 2, p. 123, doi. 10.4006/0836-1398-36.2.123
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Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). II. Discovery of 32 quasars and luminous galaxies at 5.7 < z ≤ 6.8.
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- Publications of the Astronomical Society of Japan, 2018, v. 70, n. Supp1, p. 1, doi. 10.1093/pasj/psx046
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Eddington ratios of dust-obscured quasars at z ≲ 1: Evidence supporting dust-obscured quasars as young quasars.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 690, p. 1, doi. 10.1051/0004-6361/202450290
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A quasar-galaxy merger at z ∼ 6.2: Black hole mass and quasar properties from the NIRSpec spectrum.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 685, p. 1, doi. 10.1051/0004-6361/202348535
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The WISSH quasars project VIII. Outflows and metals in the circum-galactic medium around the hyper-luminous z ~ 3.6 quasar J1538+08.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2020, v. 635, p. 1, doi. 10.1051/0004-6361/201936197
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Constraining the geometry and kinematics of the quasar broad emission line region using gravitational microlensing: II. Comparing models with observations in the lensed quasar HE0435−1223.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2019, v. 629, p. 1, doi. 10.1051/0004-6361/201731087
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Distribution of Doppler Redshifts of Associated Absorbers of SDSS Quasars.
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- Journal of Astrophysics & Astronomy, 2013, v. 34, n. 4, p. 357, doi. 10.1007/s12036-013-9189-1
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Quasar absorption lines: an overview.
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- Bulletin of the Astronomical Society of India, 2013, v. 41, n. 1, p. 41
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The discovery of quasars.
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- Bulletin of the Astronomical Society of India, 2013, v. 41, n. 1, p. 1
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Discovery of a hyperluminous quasar at z = 1.62 with Eddington ratio >3 in the eFEDS field confirmed by KOOLS-IFU on Seimei Telescope.
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- Publications of the Astronomical Society of Japan, 2024, v. 76, n. 6, p. 1173, doi. 10.1093/pasj/psae078
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Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). VIII. A less biased view of the early co-evolution of black holes and host galaxies.
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- Publications of the Astronomical Society of Japan, 2019, v. 71, n. 6, p. N.PAG, doi. 10.1093/pasj/psz096
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Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). III. Star formation properties of the host galaxies at z ≳ 6 studied with ALMA.
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- Publications of the Astronomical Society of Japan, 2018, v. 70, n. 3, p. 36-1, doi. 10.1093/pasj/psy026
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Optical variability properties of mini-BAL and NAL quasars.
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- Publications of the Astronomical Society of Japan, 2016, v. 68, n. 4, p. 48-1, doi. 10.1093/pasj/psw044
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The circum-galactic medium of quasars: transverse and line-of-sight absorptions.
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- Astrophysics & Space Science, 2020, v. 365, n. 11, p. 1, doi. 10.1007/s10509-020-03889-0
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Blue outliers among intermediate redshift quasars.
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- Astrophysics & Space Science, 2016, v. 361, n. 1, p. 1, doi. 10.1007/s10509-015-2590-2
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The fraction and mid-infrared properties of broad absorption line quasars from the Sloan Digital Sky Survey.
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- Astrophysics & Space Science, 2014, v. 349, n. 2, p. 947, doi. 10.1007/s10509-013-1669-x
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Properties of radio-detected broad absorption line quasars from the Sloan Digital Sky Survey.
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- Astrophysics & Space Science, 2013, v. 345, n. 2, p. 355, doi. 10.1007/s10509-013-1412-7
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The main sequence of quasars: The taming of the extremes.
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- Astronomische Nachrichten, 2022, v. 343, n. 1/2, p. 1, doi. 10.1002/asna.20210082
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Deep-Learning-Based Identification of Broad-Absorption Line Quasars.
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- Applied Sciences (2076-3417), 2025, v. 15, n. 3, p. 1024, doi. 10.3390/app15031024
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The VLBI structure of radio-loud Broad Absorption Line quasars.
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- Astronomische Nachrichten, 2016, v. 337, n. 1/2, p. 184, doi. 10.1002/asna.201512291
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The most distant quasar at z = 7.08: Probable retrograde rotation of an accreting supermassive black hole.
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- Astronomische Nachrichten, 2015, v. 336, n. 3, p. 312, doi. 10.1002/asna.201412161
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QSO MUSEUM: II. Search for extended Lyα emission around eight z ∼ 3 quasar pairs.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 691, p. 1, doi. 10.1051/0004-6361/202450959
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Exploring the links between quasar winds and radio emission along the main sequence at high redshift.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 691, p. 1, doi. 10.1051/0004-6361/202449976
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Ubiquitous radio emission in quasars: Predominant AGN origin and a connection to jets, dust, and winds.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 691, p. 1, doi. 10.1051/0004-6361/202348982
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Size and kinematics of the C IV broad emission line region from microlensing-induced line profile distortions in two gravitationally lensed quasars.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 687, p. 1, doi. 10.1051/0004-6361/202450258
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Quasars as standard candles: V. Accounting for the dispersion in the L<sub>X</sub>–L<sub>UV</sub> relation down to ≤ 0.06 dex.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 687, p. 1, doi. 10.1051/0004-6361/202348941
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Probing the broad line region geometry and size of the gravitationally lensed quasar Q2237+0305 with microlensing time series.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 687, p. 1, doi. 10.1051/0004-6361/202347953
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Tracing the rise of supermassive black holes: A panchromatic search for faint, unobscured quasars at z ≳ 6 with COSMOS-Web and other surveys.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 685, p. 1, doi. 10.1051/0004-6361/202349025
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Quasar 3C 47: Extreme Population B jetted source with double-peaked profiles.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 685, p. 1, doi. 10.1051/0004-6361/202348800
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The missing quasar image in the gravitationally lensed quasar HE0230−2130: Implications for the cored lens mass distribution and dark satellites.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 685, p. 1, doi. 10.1051/0004-6361/202347689
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Gaia Focused Product Release: A catalogue of sources around quasars to search for strongly lensed quasars.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 685, p. 1, doi. 10.1051/0004-6361/202347273
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Extreme FeLoBAL outflow in the VLT/UVES spectrum of quasar SDSS J1321−0041.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 684, p. 1, doi. 10.1051/0004-6361/202348215
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Nine lensed quasars and quasar pairs discovered through spatially extended variability in Pan-STARRS.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 682, p. 1, doi. 10.1051/0004-6361/202347598
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Probing the structure of the lensed quasar SDSS J1004+4112 through microlensing analysis of spectroscopic data.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 682, p. 1, doi. 10.1051/0004-6361/202347382
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HYPERION: Interacting companion and outflow in the most luminous z > 6 quasar.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 682, p. 1, doi. 10.1051/0004-6361/202347081
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The most luminous blue quasars at 3.0 < z < 3.3: III. LBT spectra and accretion parameters.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2023, v. 677, p. 1, doi. 10.1051/0004-6361/202346024
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The WISSH quasars project: XI. The mean spectral energy distribution and bolometric corrections of the most luminous quasars.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2023, v. 671, p. 1, doi. 10.1051/0004-6361/202244296
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Periodicity of quasar and galaxy redshift.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2020, v. 643, p. 1, doi. 10.1051/0004-6361/201630164
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Quasars as standard candles: III. Validation of a new sample for cosmological studies.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2020, v. 642, p. 1, doi. 10.1051/0004-6361/202038899
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The XXL Survey: XLIII. The quasar radio loudness dichotomy exposed via radio luminosity functions obtained by combining results from COSMOS and XXL-S X-ray selected quasars.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2020, v. 642, p. 1, doi. 10.1051/0004-6361/201936776
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The WISSH quasars project: VII. The impact of extreme radiative field in the accretion disc and X-ray corona interplay.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2020, v. 635, p. 1, doi. 10.1051/0004-6361/201937292
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Testing the paradigm: First spectroscopic evidence of a quasar–galaxy Mpc-scale association at cosmic dawn.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2019, v. 631, p. 1, doi. 10.1051/0004-6361/201936813
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Discovery of intergalactic bridges connecting two faint z ∼ 3 quasars.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2019, v. 631, p. 1, doi. 10.1051/0004-6361/201936211
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Radio loudness along the quasar main sequence.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2019, v. 630, p. 1, doi. 10.1051/0004-6361/201936270
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Proximate molecular quasar absorbers: Excess of damped H<sub>2</sub> systems at z<sub>abs</sub> ≈ z<sub>QSO</sub> in SDSS DR14.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2019, v. 627, p. 1, doi. 10.1051/0004-6361/201935371
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Black hole mass estimates in quasars: A comparative analysis of high- and low-ionization lines.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2019, v. 627, p. 1, doi. 10.1051/0004-6361/201935265
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GALEX colours of quasars and intergalactic medium opacity at low redshift.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2019, v. 623, p. N.PAG, doi. 10.1051/0004-6361/201832673
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AGN feedback on molecular gas reservoirs in quasars at z ~ 2.4.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2017, v. 605, p. 1, doi. 10.1051/0004-6361/201730672
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