The 0.1 <z < 1.65 evolution of the bright end of the [O ii] luminosity function

@article{Comparat2015The0,
  title={The 0.1 <z < 1.65 evolution of the bright end of the [O ii] luminosity function},
  author={Johan Comparat and Johan Richard and Jean-Paul Kneib and Olivier Ilbert and Violeta Gonzalez-Perez and Laurence Tresse and Julien Zoubian and S. Arnouts and Roland Bacon and Joel R. Brownstein and Carlton M. Baugh and Timoth'ee Delubac and Anne Ealet and St'ephanie Escoffier and Jian Ge and Eric Jullo and Cedric G Lacey and Nicholas P. Ross and David J. Schlegel and Donald P. Schneider and Oliver Steele and Lidia A. M. Tasca and Ch. Y{\'e}che and Michael P. Lesser and Zhao-ji Jiang and Yipeng Jing and Zhou Fan and Xiaohui Fan and Jun Ma and Jundan Nie and Jiali Wang and Zhen-Yu Wu and Tianmeng Zhang and Xu Zhou and Zhi-min Zhou and Hu Zou},
  journal={Astronomy and Astrophysics},
  year={2015},
  volume={575}
}
We present the [Oii] (λλ3729,3726) luminosity function measured in the redshift range 0.1 <z< 1.65 with unprecedented depth and accuracy. Our measurements are based on medium resolution flux-calibrated spectra of emission line galaxies with the visual and near UV FOcal Reducer and low dispersion Spectrograph (FORS2) for the Very Large Telescope (VLT) of the European Southern Observatory (ESO) and with the SDSS-III/BOSS spectrograph. The FORS2 spectra and the corresponding catalog containing… 

Herschel and ALMA Observations of Massive SZE-selected Clusters

We present new Herschel observations of four massive, Sunyaev–Zel’dovich effect–selected clusters at , two of which have also been observed with the Atacama Large Millimeter/submillimeter Array

GalPaK3D: A BAYESIAN PARAMETRIC TOOL FOR EXTRACTING MORPHOKINEMATICS OF GALAXIES FROM 3D DATA

We present a method to constrain galaxy parameters directly from three-dimensional data cubes. The algorithm compares directly the data with a parametric model mapped in x , y , λ ?> coordinates. It

COSMOS2020: A Panchromatic View of the Universe to z ∼ 10 from Two Complementary Catalogs

The Cosmic Evolution Survey (COSMOS) has become a cornerstone of extragalactic astronomy. Since the last public catalog in 2015, a wealth of new imaging and spectroscopic data have been collected in

The Mass–Metallicity Relation at z ∼ 0.8: Redshift Evolution and Parameter Dependency

The spectra of emission-line galaxies from the extended Baryon Oscillation Spectroscopic Survey of the Sloan Digit Sky Survey (SDSS) are used to study the mass–metallicity relation (MZR) at z ∼ 0.8.

Clustering properties of g-selected galaxies at z similar to 0.8

Current and future large redshift surveys, as the Sloan Digital Sky Survey IV extended Baryon Oscillation Spectroscopic Survey (SDSS-IV/eBOSS) or the Dark Energy Spectroscopic Instrument (DESI), will

Groups and Protocluster Candidates in the CLAUDS and HSC-SSP Joint Deep Surveys

Using the extended halo-based group finder developed by Yang et al., which is able to deal with galaxies via spectroscopic and photometric redshifts simultaneously, we construct galaxy group and

Lyman Continuum Galaxy Candidates in COSMOS

Star-forming galaxies are the sources likely to have reionized the universe. As we cannot observe them directly due to the opacity of the intergalactic medium at z ≳ 5, we study z ∼ 3–5 galaxies as

Morphological Evolution of the Hosts of Far-infrared/Submillimeter Galaxies

We present a host morphological study of 1266 far-infrared galaxies (FIRGs) and submillimeter galaxies (SMGs) in the Cosmic Evolution Survey field using the F160W and F814W images obtained by the

HELP: the Herschel Extragalactic Legacy Project

We present the Herschel Extragalactic Legacy Project (HELP). This project collates, curates, homogenizes, and creates derived data products for most of the premium multiwavelength extragalactic

Classifying stars, galaxies, and AGNs in CLAUDS + HSC-SSP using gradient boosted decision trees

Classifying catalog objects as stars, galaxies, or AGN is a crucial part of any statistical study of galaxies. We describe our pipeline for binary (star/galaxy) and multiclass (star/galaxy/Type I
...

References

SHOWING 1-10 OF 70 REFERENCES

THE [O ii] λ3727 LUMINOSITY FUNCTION AT z ∼ 1

We measure the evolution of the [O ii] λ3727 luminosity function (LF) at 0.75 < z < 1.45 using high-resolution spectroscopy of ∼14,000 galaxies observed by the Deep Extragalactic Evolutionary Probe 2

2007b, ApJS, 172, 1 Article number, page

  • 2007

Optical Star Formation Rate Indicators

Using integrated optical spectrophotometry for 412 star-forming galaxies at z ~ 0, and fiber-aperture spectrophotometry for 120,846 SDSS galaxies at z ~ 0.1, we investigate the Hα λ6563, Hβ λ4861, [O

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)

We present new results on the cosmic star formation history in the Subaru/XMM–Newton Deep Survey (SXDS)–Ultra Deep Survey (UDS) field out to z = 1.6. We compile narrowband data from the Subaru

Erratum: The local star formation rate density: assessing calibrations using [O ii], Hα and UV luminosities

We explore the use of simple star formation rate (SFR) indicators (such as may be used in high-redshift galaxy surveys) in the local Universe using [O II], Hα and u-band luminosities from the deeper

COSMOS: Hubble Space Telescope Observations

The Cosmic Evolution Survey (COSMOS) was initiated with an extensive allocation (590 orbits in Cycles 12-13) using the Hubble Space Telescope (HST) for high-resolution imaging. Here we review the

Accurate photometric redshifts for the CFHT legacy survey calibrated using the VIMOS VLT deep survey

We present photometric redshifts for an uniquely large and deep sample of 522286 objects with i'_{AB}<25 in the Canada-France Legacy Survey ``Deep Survey'' fields, which cover a total effective area

The Cosmic Evolution Survey (COSMOS): Overview

The Cosmic Evolution Survey (COSMOS) is designed to probe the correlated evolution of galaxies, star formation, active galactic nuclei (AGNs), and dark matter (DM) with large-scale structure (LSS)

Mass assembly in quiescent and star-forming galaxies since z ≃ 4 from UltraVISTA

We estimate the galaxy stellar mass function and stellar mass density for star-forming and quiescent galaxies with 0.2   1.5 consistent with the expected uncertainties. We also develop a new method
...