The ALPINE-ALMA [CII] survey: Data processing, catalogs, and statistical source properties

@article{Bthermin2020TheA,
  title={The ALPINE-ALMA [CII] survey: Data processing, catalogs, and statistical source properties},
  author={Matthieu B{\'e}thermin and Yoshinobu Fudamoto and Michele Ginolfi and Federica Loiacono and Yana Khusanova and Peter Capak and Paolo Cassata and Andreas L. Faisst and Olivier Le F{\`e}vre and Daniel Schaerer and John D. Silverman and L. Yan and Ricardo Amor{\'i}n and Sandro Bardelli and M{\'e}d{\'e}ric Boquien and Alessandro Cimatti and Iary Davidzon and Miroslava Dessauges-Zavadsky and Seiji Fujimoto and Carlotta Gruppioni and Nimish P. Hathi and Edo Ibar and G. C. Jones and Anton M. Koekemoer and Guilaine Lagache and Brian C. Lemaux and C. Moreau and Pascal A. Oesch and Francesca Pozzi and Dominik A. Riechers and Margherita Talia and Sune Toft and Livia Vallini and D. Vergani and Gianni Zamorani and Elena Zucca},
  journal={Astronomy \& Astrophysics},
  year={2020}
}
The Atacama Large Millimeter Array (ALMA) Large Program to INvestigate [CII] at Early times (ALPINE) targets the [CII] 158 μm line and the far-infrared continuum in 118 spectroscopically confirmed star-forming galaxies between z = 4.4 and z = 5.9. It represents the first large [CII] statistical sample built in this redshift range. We present details regarding the data processing and the construction of the catalogs. We detected 23 of our targets in the continuum. To derive accurate infrared… 
The ALPINE-ALMA [CII] survey
  • Astronomy & Astrophysics
  • 2020
The ALPINE-ALMA [CII] survey
Star formation rate (SFR) measurements at z > 4 have relied mostly on the rest-frame far-ultraviolet (FUV) observations. The corrections for dust attenuation based on the IRX-β relation are highly
The ALPINE-ALMA [CII] survey
  • Astronomy & Astrophysics
  • 2020
The ALPINE-ALMA [Cii] survey. Little to no evolution in the [C ii]-SFR relation over the last 13 Gyr
The [CII] 158 micron line is one of the strongest IR emission lines, which has been shown to trace the star-formation rate (SFR) of galaxies in the nearby Universe and up to $z \sim 2$. Whether this
The ALPINE-ALMA [CII] survey
  • Astronomy & Astrophysics
  • 2021
The ALPINE–ALMA [C ii] Survey: Size of Individual Star-forming Galaxies at z = 4–6 and Their Extended Halo Structure
We present the physical extent of [CII] 158um line-emitting gas from 46 star-forming galaxies at z=4-6 from the ALMA Large Program to INvestigate CII at Early Times (ALPINE). Using exponential
The ALPINE-ALMA [C II] survey: the luminosity function of serendipitous [C II] line emitters at $z\sim 5$
We present the first [CII] 158 $\mu$m luminosity function (LF) at $z\sim 5$ from a sample of serendipitous lines detected in the ALMA Large Program to INvestigate [CII] at Early times (ALPINE). A
The ALPINE-ALMA [CII] survey: Molecular gas budget in the Early Universe as traced by [CII]
The molecular gas content of normal galaxies at z>4 is poorly constrained, because the commonly used molecular gas tracers become hard to detect. We use the [CII]158um luminosity, recently proposed
The ALPINE-ALMA [CII] survey
  • Astronomy & Astrophysics
  • 2020
The ALPINE-ALMA [C II] Survey: [C II] 158 μm Emission Line Luminosity Functions at z ∼ 4–6
We present the [CII]158μm line luminosity functions (LFs) at z ∼ 4−6 using the ALMA observations of 118 sources, which are selected to have UV luminosity M_(1500A) 10⁹ L_⊙) compared to z∼0. This
...
...

References

SHOWING 1-10 OF 157 REFERENCES
The ALPINE-ALMA [CII] survey
  • Astronomy & Astrophysics
  • 2020
The ALPINE-ALMA [CII] survey
Star formation rate (SFR) measurements at z > 4 have relied mostly on the rest-frame far-ultraviolet (FUV) observations. The corrections for dust attenuation based on the IRX-β relation are highly
The ALPINE–ALMA [C ii] Survey: Multiwavelength Ancillary Data and Basic Physical Measurements
We present the ancillary data and basic physical measurements for the galaxies in the ALMA Large Program to Investigate C+ at Early Times (ALPINE) survey - the first large multi-wavelength survey
The ALPINE-ALMA [CII] survey
  • Astronomy & Astrophysics
  • 2020
The ALPINE−ALMA [C ii] Survey: on the nature of an extremely obscured serendipitous galaxy
We report the serendipitous discovery of a dust-obscured galaxy observed as part of the Atacama Large Millimeter Array (ALMA) Large Program to INvestigate [C ii] at Early times (ALPINE). While this
The ALPINE-ALMA [Cii] survey. Little to no evolution in the [C ii]-SFR relation over the last 13 Gyr
The [CII] 158 micron line is one of the strongest IR emission lines, which has been shown to trace the star-formation rate (SFR) of galaxies in the nearby Universe and up to $z \sim 2$. Whether this
The ALPINE–ALMA [C ii] Survey: Size of Individual Star-forming Galaxies at z = 4–6 and Their Extended Halo Structure
We present the physical extent of [CII] 158um line-emitting gas from 46 star-forming galaxies at z=4-6 from the ALMA Large Program to INvestigate CII at Early Times (ALPINE). Using exponential
The ALPINE-ALMA [CII] survey: Molecular gas budget in the Early Universe as traced by [CII]
The molecular gas content of normal galaxies at z>4 is poorly constrained, because the commonly used molecular gas tracers become hard to detect. We use the [CII]158um luminosity, recently proposed
The ALPINE-ALMA [CII] survey
  • Astronomy & Astrophysics
  • 2020
On the [CII]-SFR relation in high redshift galaxies
After two ALMA observing cycles, only a handful of [CII] $158\,\mu m$ emission line searches in z>6 galaxies have reported a positive detection, questioning the applicability of the local [CII]-SFR
...
...