DOAJ Open Access 2024

ALMA Lensing Cluster Survey: Deep 1.2 mm Number Counts and Infrared Luminosity Functions at z ≃ 1–8

Seiji Fujimoto Kotaro Kohno Masami Ouchi Masamune Oguri Vasily Kokorev +38 lainnya

Abstrak

We present a statistical study of 180 dust continuum sources identified in 33 massive cluster fields by the Atacama Large Millimeter/submillimeter Array Lensing Cluster Survey (ALCS) over a total of 133 arcmin ^2 area, homogeneously observed at 1.2 mm. ALCS enables us to detect extremely faint millimeter sources by lensing magnification, including near-infrared (NIR) dark objects showing no counterparts in existing Hubble Space Telescope and Spitzer images. The dust continuum sources belong to a blind sample ( N = 141) with signal-to-noise ratio (S/N) ≳ 5.0 (a purity of >0.99) or a secondary sample ( N = 39) with S/N = 4.0–5.0 screened by priors. With the blind sample, we securely derive 1.2 mm number counts down to ∼7 μ Jy, and find that the total integrated 1.2 mm flux is ${20.7}_{-6.5}^{+8.5}$ Jy deg ^−2 , resolving ≃80% of the cosmic infrared background light. The resolved fraction varies by a factor of 0.6–1.1 due to the completeness correction depending on the spatial size of the millimeter emission. We also derive infrared (IR) luminosity functions (LFs) at z = 0.6–7.5 with the $1/{V}_{\max }$ method, finding the redshift evolution of IR LFs characterized by positive luminosity and negative density evolution. The total (= UV + IR) cosmic star formation rate density (SFRD) at z > 4 is estimated to be ${161}_{-21}^{+25}$ % of the Madau and Dickinson measurements mostly based on rest-frame UV surveys. Although our general understanding of the cosmic SFRD is unlikely to change beyond a factor of 2, these results add to the weight of evidence for an additional (≈60%) SFRD component contributed by the faint millimeter population, including NIR-dark objects.

Topik & Kata Kunci

Penulis (43)

S

Seiji Fujimoto

K

Kotaro Kohno

M

Masami Ouchi

M

Masamune Oguri

V

Vasily Kokorev

G

Gabriel Brammer

F

Fengwu Sun

J

Jorge González-López

F

Franz E. Bauer

G

Gabriel B. Caminha

B

Bunyo Hatsukade

J

Johan Richard

I

Ian Smail

A

Akiyoshi Tsujita

Y

Yoshihiro Ueda

R

Ryosuke Uematsu

A

Adi Zitrin

D

Dan Coe

J

Jean-Paul Kneib

M

Marc Postman

K

Keiichi Umetsu

C

Claudia del P. Lagos

G

Gergö Popping

Y

Yiping Ao

L

Larry Bradley

K

Karina Caputi

M

Miroslava Dessauges-Zavadsky

E

Eiichi Egami

D

Daniel Espada

R

R. J. Ivison

M

Mathilde Jauzac

K

Kirsten K. Knudsen

A

Anton M. Koekemoer

G

Georgios E. Magdis

G

Guillaume Mahler

A

A. M. Muñoz Arancibia

T

Timothy Rawle

K

Kazuhiro Shimasaku

S

Sune Toft

H

Hideki Umehata

F

Francesco Valentino

T

Tao Wang

W

Wei-Hao Wang

Format Sitasi

Fujimoto, S., Kohno, K., Ouchi, M., Oguri, M., Kokorev, V., Brammer, G. et al. (2024). ALMA Lensing Cluster Survey: Deep 1.2 mm Number Counts and Infrared Luminosity Functions at z ≃ 1–8. https://doi.org/10.3847/1538-4365/ad5ae2

Akses Cepat

PDF tidak tersedia langsung

Cek di sumber asli →
Lihat di Sumber doi.org/10.3847/1538-4365/ad5ae2
Informasi Jurnal
Tahun Terbit
2024
Sumber Database
DOAJ
DOI
10.3847/1538-4365/ad5ae2
Akses
Open Access ✓