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 L. 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
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. 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 [C ii] 158 μm line-emitting gas from 46 star-forming galaxies at z = 4–6 from the ALMA Large Program to INvestigate C ii 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
ALPINE: A Large Survey to Understand Teenage Galaxies
A multiwavelength study of galaxies is important to understand their formation and evolution. Only in the recent past, thanks to the Atacama Large (Sub) Millimeter Array (ALMA), were we able to study
Probing Cold Gas in a Massive, Compact Star-forming Galaxy at z = 6
Observations of low-order 12C16O transitions represent the most direct way to study galaxies’ cold molecular gas, the fuel of star formation. Here we present the first detection of CO(J = 2 → 1) in a
Significant Dust-obscured Star Formation in Luminous Lyman-break Galaxies at z ∼ 7–8
We make use of Atacama Large Millimeter/submillimeter Array continuum observations of 15 luminous Lyman-break galaxies at z ∼ 7–8 to probe their dust-obscured star formation. These observations are
ALMA Lensing Cluster Survey: Bright [C ii] 158 μm Lines from a Multiply Imaged Sub-L ⋆ Galaxy at z = 6.0719
We present bright [C ii] 158 μm line detections from a strongly magnified and multiply imaged (μ ∼ 20–160) sub–L * ( MUV=−19.75−0.44+0.55 ) Lyman-break galaxy (LBG) at z = 6.0719 ± 0.0004, drawn from
The ALPINE-ALMA [C II] Survey: [C II] 158 μm Emission Line Luminosity Functions at z ∼ 4–6
We present the [C II] 158 μm line luminosity functions (LFs) at z ∼ 4–6 using the ALMA observations of 118 sources, which are selected to have UV luminosity M1500Å < −20.2 and optical spectroscopic
...
...

References

SHOWING 1-10 OF 158 REFERENCES
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 multiwavelength survey that
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 [C ii] 158 μm line-emitting gas from 46 star-forming galaxies at z = 4–6 from the ALMA Large Program to INvestigate C ii 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
2017, A&A, to be sub
  • 2017
Astronomy and Astro
  • 2014
ALPINE targets are classified as merging systems (see the criteria in Le Fèvre et al.)
  • 2020
ON THE [C ii]–SFR RELATION IN HIGH REDSHIFT GALAXIES
After two Atacama Large Millimeter/submillimeter Array (ALMA) observing cycles, only a handful of [C ii] 158 μm emission line searches in z > 6 galaxies have reported a positive detection,
...
...