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M. Akiyama

Identifiers

  • name variant M. Akiyama 0.60 · backfill

Papers (34)

  1. An FMOS Survey of moderate-luminosity broad-line AGN in COSMOS, SXDS and E-CDF-S astro-ph.GA · 2018 · author #4
  2. Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). IV. Discovery of 41 Quasars and Luminous Galaxies at 5.7 < z < 6.9 astro-ph.GA · 2018 · author #9
  3. ALMA Twenty-six arcmin$^2$ Survey of GOODS-S at One-millimeter (ASAGAO): X-ray AGN Properties of Millimeter-Selected Galaxies astro-ph.HE · 2017 · author #7
  4. An Optically Faint Quasar Survey at z~5 in the CFHTLS Wide Field: Estimates of the Black Hole Masses and Eddington Ratios astro-ph.GA · 2017 · author #6
  5. Cluster Glimpses with Raven: AO Corrected Near and Mid-Infrared Images of Glimpse C01 and Glimpse C02 astro-ph.GA · 2016 · author #10
  6. Raven and the Center of Maffei 1: Multi-Object Adaptive Optics Observations of the Center of a Nearby Elliptical Galaxy and the Detection of an Intermediate Age Population astro-ph.GA · 2015 · author #7
  7. The Quasar-LBG Two-point Angular Cross-correlation Function at z ~ 4 in the COSMOS Field astro-ph.GA · 2015 · author #6
  8. Detailed Shape and Evolutionary Behavior of the X-ray Luminosity Function of Active Galactic Nuclei astro-ph.GA · 2015 · author #14
  9. A statistical relation between the X-ray spectral index and Eddington ratio of active galactic nuclei in deep surveys astro-ph.HE · 2013 · author #22
  10. Black hole mass and Eddington ratio distribution functions of X-ray selected broad-line AGNs at z~1.4 in the Subaru XMM-Newton Deep Field astro-ph.CO · 2012 · author #2
  11. FMOS near-IR spectroscopy of Herschel selected galaxies: star formation rates, metallicity and dust attenuation at z~1 astro-ph.CO · 2012 · author #6
  12. FIBRE-pac: FMOS image-based reduction package astro-ph.IM · 2011 · author #7
  13. The XMM-LSS survey: optical assessment and properties of different X-ray selected cluster classes astro-ph.CO · 2010 · author #21
  14. MOIRCS Deep Survey. VIII. Evolution of Star Formation Activity as a Function of Stellar Mass in Galaxies since z~3 astro-ph.CO · 2010 · author #6
  15. Unveiling the Nature of Submillimeter Galaxy SXDF850.6 astro-ph.CO · 2010 · author #4
  16. X-ray groups and clusters of galaxies in the Subaru-XMM Deep Field astro-ph.CO · 2009 · author #9
  17. MOIRCS Deep Survey IV: Evolution of Galaxy Stellar Mass Function Back to z ~ 3 astro-ph.CO · 2009 · author #6
  18. MOIRCS Deep Survey III: Active Galactic Nuclei in Massive Galaxies at z=2-4 astro-ph.CO · 2009 · author #3
  19. An extreme EXO: a type 2 QSO at z=1.87 astro-ph · 2008 · author #4
  20. Evolution of Star-forming Galaxies seen from Lyman Break Galaxies at $z\sim5$ astro-ph · 2008 · author #5
  21. Detections of Lyman Continuum from Star-forming Galaxies at z~3 Through Subaru/Suprime-Cam Narrow-band Imaging astro-ph · 2008 · author #7
  22. The Subaru/XMM-Newton Deep Survey (SXDS) - II. Optical Imaging and Photometric Catalogs astro-ph · 2008 · author #3
  23. Adaptive Optics Imaging of Lyman Break Galaxies as Progenitors of Spheroids in the Local Universe astro-ph · 2007 · author #1
  24. Balmer Absorption Lines in FeLoBALs astro-ph · 2006 · author #6
  25. Luminosity Dependent Evolution of Lyman Break Galaxies from redshift 5 to 3 astro-ph · 2006 · author #4
  26. An X-ray bright ERO hosting a type 2 QSO astro-ph · 2006 · author #6
  27. Deep Spectroscopic Survey of Lyman Break Galaxies at z~5 astro-ph · 2005 · author #4
  28. Evolution of Lyman Break Galaxies From z=5 to 3 astro-ph · 2005 · author #6
  29. Definitive Identification of the Transition between Small- to Large-Scale Clustering for Lyman Break Galaxies astro-ph · 2005 · author #5
  30. A Strong Lyman-alpha Emitter at z=6.33 in the Subaru Deep Field Selected as an i' Dropout astro-ph · 2004 · author #9
  31. XMM-Newton observations expose AGN in apparently normal galaxies astro-ph · 2003 · author #10
  32. Lyman Break Galaxies at z~5: Luminosity Function astro-ph · 2003 · author #7
  33. Log N - Log S Relations and Spectral Properties of Sources from the ASCA Large Sky Survey --- their Implications for the Origin of the Cosmic X-ray Background (CXB) astro-ph · 1999 · author #10
  34. Optical Identification of the Hardest X-ray Source in the ASCA Large Sky Survey astro-ph · 1998 · author #1

Mentions

  • 1305.3917 #22 · backfill · confidence 0.70 M. Akiyama
  • 1211.0069 #2 · backfill · confidence 0.70 M. Akiyama
  • 1207.5564 #6 · backfill · confidence 0.70 M. Akiyama
  • 1111.6746 #7 · backfill · confidence 0.70 M. Akiyama
  • 1010.6195 #21 · backfill · confidence 0.70 M. Akiyama
  • 1009.0002 #6 · backfill · confidence 0.70 M. Akiyama
  • 1001.3690 #4 · backfill · confidence 0.70 M. Akiyama
  • 0912.0039 #9 · backfill · confidence 0.70 M. Akiyama
  • 0907.0133 #6 · backfill · confidence 0.70 M. Akiyama
  • 0905.3320 #3 · backfill · confidence 0.70 M. Akiyama
  • 0810.0544 #4 · backfill · confidence 0.70 M. Akiyama
  • 0807.0138 #5 · backfill · confidence 0.70 M. Akiyama
  • 0805.4012 #7 · backfill · confidence 0.70 M. Akiyama
  • 0801.4017 #3 · backfill · confidence 0.70 M. Akiyama
  • 0709.3523 #1 · backfill · confidence 0.70 M. Akiyama

Frequent Coauthors