K. Mcgill

Astronomy and Astrophysics · 2007–2015

A researcher in the Science corpus: 3 papers; trusts 7 researchers and is trusted by 2 researchers here, as inferred from the citation graph.

Subfields

Whom K. Mcgill trusts overall

Their strongest outbound trust, strongest first, inferred from their citations.

  1. M. Vestergaard
  2. B. Peterson
  3. H. Netzer
  4. J. Woo
  5. M. Bentz
  6. C. Onken
  7. S. Kaspi
  8. T. Treu
  9. S. Collin
  10. L. Ferrarese

Who trusts K. Mcgill overall

  1. J. Woo
  2. B. Trakhtenbrot
  3. Alister W. Graham
  4. T. Treu
  5. Yue Shen
  6. Chen Hu
  7. H. Netzer
  8. B. Peterson
  9. C. Onken
  10. A. Merloni

Papers from K. Mcgill's perspective

Ordered by how strongly the researchers K. Mcgill trusts endorse each paper. Same corpus, a different order for every researcher.

  1. Supermassive Black Holes in Active Galactic Nuclei. II. Calibration of the Black Hole Mass-Velocity Dispersion Relationship for Active Galactic Nuclei
  2. Central Masses and Broad-Line Region Sizes of Active Galactic Nuclei. II. A Homogeneous Analysis of a Large Reverberation-Mapping Database
  3. Black Hole Masses and Eddington Ratios at 0.3 < z < 4
  4. Energy input from quasars regulates the growth and activity of black holes and their host galaxies (Nature)
  5. THE RADIUS–LUMINOSITY RELATIONSHIP FOR ACTIVE GALACTIC NUCLEI: THE EFFECT OF HOST-GALAXY STARLIGHT ON LUMINOSITY MEASUREMENTS. II. THE FULL SAMPLE OF REVERBERATION-MAPPED AGNs
  6. The Relationship between Luminosity and Broad-Line Region Size in Active Galactic Nuclei
  7. Determining Central Black Hole Masses in Distant Active Galaxies and Quasars. II. Improved Optical and UV Scaling Relationships
  8. A Relationship between Nuclear Black Hole Mass and Galaxy Velocity Dispersion
  9. The Slope of the Black Hole Mass versus Velocity Dispersion Correlation
  10. Systematic effects in measurement of black hole masses by emission-line reverberation of active galactic nuclei: Eddington ratio and inclination

Their papers