M. Ishigaki

Astronomy and Astrophysics · 2014–2017

A researcher in the Science corpus: 3 papers; trusts 22 researchers and is trusted by 1 researcher here, as inferred from the citation graph.

Subfields

Whom M. Ishigaki trusts overall

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

  1. R. Bouwens
  2. M. Oguri
  3. P. Oesch
  4. M. Ouchi
  5. R. McLure
  6. G. Illingworth
  7. Richard S. Ellis
  8. J. Dunlop
  9. Brant Robertson
  10. M. Trenti

Who trusts M. Ishigaki overall

  1. P. Oesch
  2. R. Bouwens
  3. Girish Kulkarni
  4. D. McLeod
  5. R. Naidu
  6. A. Zitrin
  7. I. Labbé
  8. S. Tacchella
  9. M. Ouchi
  10. G. Illingworth

Papers from M. Ishigaki's perspective

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

  1. Stellar population synthesis at the resolution of 2003
  2. Constraining the Evolution of the Ionizing Background and the Epoch of Reionization with z ∼ 6 Quasars. II. A Sample of 19 Quasars
  3. The Hubble Ultra Deep Field
  4. First-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters
  5. ULTRAVIOLET LUMINOSITY FUNCTIONS FROM 132 z ∼ 7 AND z ∼ 8 LYMAN-BREAK GALAXIES IN THE ULTRA-DEEP HUDF09 AND WIDE-AREA EARLY RELEASE SCIENCE WFC3/IR OBSERVATIONS
  6. A STEEP FAINT-END SLOPE OF THE UV LUMINOSITY FUNCTION AT z ∼ 2–3: IMPLICATIONS FOR THE GLOBAL STELLAR MASS DENSITY AND STAR FORMATION IN LOW-MASS HALOS
  7. Galactic Stellar and Substellar Initial Mass Function
  8. The Direct Detection of Lyman Continuum Emission from Star-forming Galaxies at z~3
  9. THE UV LUMINOSITY FUNCTION OF STAR-FORMING GALAXIES VIA DROPOUT SELECTION AT REDSHIFTS z ∼ 7 AND 8 FROM THE 2012 ULTRA DEEP FIELD CAMPAIGN
  10. LARGE AREA SURVEY FOR z = 7 GALAXIES IN SDF AND GOODS-N: IMPLICATIONS FOR GALAXY FORMATION AND COSMIC REIONIZATION

Their papers