Evolution of star formation in the UKIDSS Ultra Deep Survey Field - I. Luminosity functions and cosmic star formation rate out to z = 1.6 (vol 433, pg 796, 2013)
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J. Dunlop | R. McLure | Daniel J. B. Smith | M. Jarvis | C. Collins | I. Baldry | G. Dalton | D. Bonfield | C. Simpson | P. Best | P. James | M. Ouchi | Y. Ono | A. Drake | Daniel J B Smith
[1] M. Sullivan,et al. The VISTA deep extragalactic observations (VIDEO) survey , 2012, 1206.4263.
[2] Michele Cirasuolo,et al. A large Hα survey at z = 2.23, 1.47, 0.84 and 0.40: the 11 Gyr evolution of star-forming galaxies from HiZELS , 2012, 1202.3436.
[3] T. Nagao,et al. THE STELLAR POPULATION AND STAR FORMATION RATES OF z ≈ 1.5–1.6 [O ii]-EMITTING GALAXIES SELECTED FROM NARROWBAND EMISSION-LINE SURVEYS , 2012, 1206.4303.
[4] J. Dunlop,et al. Radio imaging of the Subaru/XMM–NewtonDeep Field– III. Evolution of the radio luminosity function beyond z= 1 , 2012, 1201.3225.
[5] McGill,et al. Star formation at z=1.47 from HiZELS: an Hα+[O ii] double-blind study* , 2011, 1109.1830.
[6] Subaru Telescope,et al. Cosmic Star-Formation Activity at z = 2.2 Probed by H α Emission-Line Galaxies , 2010, 1012.4860.
[7] S. Roca-F brega,et al. Revista Mexicana de Astronomia y Astrofisica Conference Series , 2011 .
[8] C. Conselice,et al. Galaxy properties in different environments up to z∼ 3 in the GOODS NICMOS Survey , 2010, 1011.4846.
[9] I. Smail,et al. The dependence of star formation activity on environment and stellar mass at z∼ 1 from the HiZELS-Hα survey , 2010, 1007.2642.
[10] P. McCarthy,et al. The Redshift One LDSS-3 Emission line Survey (ROLES): survey method and z∼ 1 mass-dependent star formation rate density , 2010, 1002.3170.
[11] D. Schaerer,et al. The H-alpha luminosity function at redshift 2.2 - A new determination using VLT/HAWK-I , 2009, 0912.3267.
[12] R. Davies,et al. Astronomical Society of the Pacific Conference Series , 2010 .
[13] F. Lamareille. Spectral classification of emission-line galaxies from the Sloan Digital Sky Survey. I. An improved classification for high redshift galaxies , 2009, 0910.4814.
[14] S. M. Fall,et al. LARGE AREA SURVEY FOR z = 7 GALAXIES IN SDF AND GOODS-N: IMPLICATIONS FOR GALAXY FORMATION AND COSMIC REIONIZATION , 2009, 0908.3191.
[15] I. Baldry,et al. Evolution of the u-band luminosity function from redshift 1.2 to 0 , 2009, 0904.0349.
[16] Oxford,et al. HiZELS:a high-redshift survey of Hα emitters - II. the nature of star-forming galaxies at z = 0.84 , 2009, 0901.4114.
[17] Paolo Coppi,et al. EAZY: A Fast, Public Photometric Redshift Code , 2008, 0807.1533.
[18] R. J. Ivison,et al. HiZELS: a high-redshift survey of Hα emitters – I. The cosmic star formation rate and clustering at z= 2.23 , 2008, 0805.2861.
[19] S. Okamura,et al. The Subaru/XMM-Newton Deep Survey (SXDS). II. Optical Imaging and Photometric Catalogs , 2008, 0801.4017.
[20] S. Okamura,et al. The Subaru/XMM-Newton Deep Survey (SXDS). IV. Evolution of Lyα Emitters from z = 3.1 to 5.7 in the 1 deg2 Field: Luminosity Functions and AGN , 2007, 0707.3161.
[21] V. Villar,et al. The Hα-based Star Formation Rate Density of the Universe at z = 0.84 , 2007, 0712.4150.
[22] L. Guzzo,et al. The Hα Luminosity Function and Star Formation Rate at z ≈ 0.24 in the COSMOS 2 Square Degree Field , 2007, 0709.1009.
[23] E. Sadler,et al. Radio sources in the 6dFGS: local luminosity functions at 1.4 GHz for star-forming galaxies and radio-loud AGN , 2006, astro-ph/0612018.
[24] C. Conselice,et al. Number counts and clustering properties of bright distant red galaxies in the UKIDSS Ultra Deep Survey Early Data Release , 2006, astro-ph/0606386.
[25] M. Irwin,et al. The UKIRT Infrared Deep Sky Survey (UKIDSS) , 2006, astro-ph/0604426.
[26] Paul Clark,et al. The VISTA infrared camera , 2006, SPIE Astronomical Telescopes + Instrumentation.
[27] T. Nagao,et al. The Luminosity Function and Star Formation Rate between Redshifts of 0.07 and 1.47 for Narrowband Emitters in the Subaru Deep Field , 2006, astro-ph/0610846.
[28] A. Hopkins,et al. On the Normalization of the Cosmic Star Formation History , 2006, astro-ph/0601463.
[29] Tucson,et al. Infrared Luminosity Functions from the Chandra Deep Field-South: The Spitzer View on the History of Dusty Star Formation at 0 ≲ z ≲ 1* , 2005, astro-ph/0506462.
[30] Christopher D. Martin,et al. Spitzer View on the Evolution of Star-forming Galaxies from z = 0 to z ~ 3 , 2005, astro-ph/0505101.
[31] H. Spinrad,et al. The Hubble Space Telescope ACS Grism Parallel Survey. II. First Results and a Catalog of Faint Emission-Line Galaxies at z ≤ 1.6 , 2005, astro-ph/0503592.
[32] R. Nichol,et al. The Sloan Digital Sky Survey u‐band Galaxy Survey: luminosity functions and evolution , 2005, astro-ph/0501110.
[33] M. Langlois,et al. Society of Photo-Optical Instrumentation Engineers , 2005 .
[34] A. Cimatti,et al. A New Photometric Technique for the Joint Selection of Star-forming and Passive Galaxies at 1.4 ≲ z ≲ 2.5 , 2004, astro-ph/0409041.
[35] I. Smail,et al. A panoramic Hα imaging survey of the z= 0.4 cluster Cl 0024.0+1652 with Subaru , 2004, astro-ph/0408037.
[36] Cambridge,et al. The star formation rate of the Universe at z~ 6 from the Hubble Ultra-Deep Field , 2004, astro-ph/0403223.
[37] L. Moustakas,et al. Cosmic Variance in the Great Observatories Origins Deep Survey , 2003, astro-ph/0309071.
[38] S. Okamura,et al. The Hα Luminosity Function of the Galaxy Cluster A521 at z = 0.25 , 2003, astro-ph/0310212.
[39] S. Okamura,et al. Subaru Deep Survey. VI. A Census of Lyman Break Galaxies at z ≃ 4 and 5 in the Subaru Deep Fields: Clustering Properties , 2003, astro-ph/0309657.
[40] K. Glazebrook,et al. Constraints on a Universal Stellar Initial Mass Function from Ultraviolet to Near-Infrared Galaxy Luminosity Densities , 2003 .
[41] K. Glazebrook,et al. Constraints on a Universal IMF from UV to Near-IR Galaxy Luminosity Densities , 2003, astro-ph/0304423.
[42] J. Rhodes,et al. Emission-Line Galaxies in the Space Telescope Imaging Spectrograph Parallel Survey. I. Observations and Data Analysis , 2002, astro-ph/0212576.
[43] P. McCarthy,et al. Star Formation in Emission-Line Galaxies between Redshifts of 0.8 and 1.6 , 2002, astro-ph/0208551.
[44] D. Burke,et al. STAR FORMATION HISTORY SINCE z = 1.5 AS INFERRED FROM REST-FRAME ULTRAVIOLET LUMINOSITY DENSITY EVOLUTION , 2002, astro-ph/0203168.
[45] S. Maddox,et al. The Hα luminosity function and star formation rate up to z ∼ 1 ⋆ , 2001, astro-ph/0111390.
[46] Lennox L. Cowie,et al. Evidence for a Gradual Decline in the Universal Rest-Frame Ultraviolet Luminosity Density for z < 1 , 1999, astro-ph/9904345.
[47] Jr.,et al. STAR FORMATION IN GALAXIES ALONG THE HUBBLE SEQUENCE , 1998, astro-ph/9807187.
[48] D. Schlegel,et al. Maps of Dust Infrared Emission for Use in Estimation of Reddening and Cosmic Microwave Background Radiation Foregrounds , 1998 .
[49] D. Hogg,et al. The O II Luminosity Density of the Universe , 1998, astro-ph/9804129.
[50] D. Schlegel,et al. Maps of Dust IR Emission for Use in Estimation of Reddening and CMBR Foregrounds , 1997, astro-ph/9710327.
[51] E. Bertin,et al. SExtractor: Software for source extraction , 1996 .
[52] O. Fèvre,et al. The Canada-France Redshift Survey: The Luminosity Density and Star Formation History of the Universe to z ~ 1 , 1996, astro-ph/9601050.
[53] A. Aragón-Salamanca,et al. The Current Star Formation Rate of the Local Universe , 1995, astro-ph/9510061.
[54] P. Hewett,et al. On near-infrared Hα searches for high-redshift galaxies⋆ , 1995, astro-ph/9501026.
[55] Robert C. Kennicutt,et al. The Integrated spectra of nearby galaxies: General properties and emission line spectra , 1992 .
[56] J. Mathis,et al. The relationship between infrared, optical, and ultraviolet extinction , 1989 .
[57] D. Osterbrock,et al. Astrophysics of Gaseous Nebulae and Active Galactic Nuclei , 1989 .
[58] G. Zamorani,et al. Analysis of complete quasar samples to obtain parameters of luminosity and evolution functions , 1983 .
[59] P. Schechter. An analytic expression for the luminosity function for galaxies , 1976 .