F. Watson

Astronomy and Astrophysics · 2002–2018

A researcher in the Science corpus: 14 papers; trusts 9 researchers and is trusted by 9 researchers here, as inferred from the citation graph.

Subfields

Whom F. Watson trusts

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

  1. J. Binney (in Astronomy and Astrophysics)
  2. R. Scoccimarro (in Astronomy and Astrophysics)
  3. Volker Springel (in Astronomy and Astrophysics)
  4. Daniel J. Eisenstein (in Astronomy and Astrophysics)
  5. Simon D. M. White (in Astronomy and Astrophysics)
  6. Takahiko Matsubara (in Astronomy and Astrophysics)
  7. Carlos S. Frenk (in Astronomy and Astrophysics)
  8. M. White (in Astronomy and Astrophysics)
  9. J. Navarro (in Astronomy and Astrophysics)

Who trusts F. Watson

  1. Will J. Percival (in Astronomy and Astrophysics)
  2. Rafael C. Nunes (in Astronomy and Astrophysics)
  3. J. Tinker (in Astronomy and Astrophysics)
  4. A. Ross (in Astronomy and Astrophysics)
  5. Z. Xing (in Astronomy and Astrophysics)
  6. Daniel J. Eisenstein (in Astronomy and Astrophysics)
  7. M. White (in Astronomy and Astrophysics)
  8. Cameron McBride (in Astronomy and Astrophysics)
  9. P. McMillan (in Astronomy and Astrophysics)

Papers from F. Watson's perspective

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

  1. Maps of Dust Infrared Emission for Use in Estimation of Reddening and Cosmic Microwave Background Radiation Foregrounds
  2. The Two Micron All Sky Survey (2MASS)
  3. The 2dF Galaxy Redshift Survey: power-spectrum analysis of the final data set and cosmological implications
  4. The Sloan Digital Sky Survey: Technical Summary
  5. The 2dF Galaxy Redshift Survey: the power spectrum and the matter content of the Universe
  6. SEVEN-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE (WMAP) OBSERVATIONS: COSMOLOGICAL INTERPRETATION
  7. The Cosmological simulation code GADGET-2
  8. The 2dF Galaxy Redshift Survey: spectra and redshifts
  9. A 3% SOLUTION: DETERMINATION OF THE HUBBLE CONSTANT WITH THE HUBBLE SPACE TELESCOPE AND WIDE FIELD CAMERA 3
  10. Cosmological parameters from CMB and other data: A Monte Carlo approach

Their papers