Finding High-redshift Galaxies with JWST

Publikation: Bidrag til tidsskriftTidsskriftartikelForskningfagfællebedømt

Standard

Finding High-redshift Galaxies with JWST. / Steinhardt, Charles L.; Jespersen, Christian Kragh; Linzer, Nora B.

I: Astrophysical Journal, Bind 923, Nr. 1, 8, 07.12.2021.

Publikation: Bidrag til tidsskriftTidsskriftartikelForskningfagfællebedømt

Harvard

Steinhardt, CL, Jespersen, CK & Linzer, NB 2021, 'Finding High-redshift Galaxies with JWST', Astrophysical Journal, bind 923, nr. 1, 8. https://doi.org/10.3847/1538-4357/ac2a2f

APA

Steinhardt, C. L., Jespersen, C. K., & Linzer, N. B. (2021). Finding High-redshift Galaxies with JWST. Astrophysical Journal, 923(1), [8]. https://doi.org/10.3847/1538-4357/ac2a2f

Vancouver

Steinhardt CL, Jespersen CK, Linzer NB. Finding High-redshift Galaxies with JWST. Astrophysical Journal. 2021 dec. 7;923(1). 8. https://doi.org/10.3847/1538-4357/ac2a2f

Author

Steinhardt, Charles L. ; Jespersen, Christian Kragh ; Linzer, Nora B. / Finding High-redshift Galaxies with JWST. I: Astrophysical Journal. 2021 ; Bind 923, Nr. 1.

Bibtex

@article{3a036aa7aa9f4650b4cad23f39d19585,
title = "Finding High-redshift Galaxies with JWST",
abstract = "One of the primary goals for the upcoming James Webb Space Telescope is to observe the first galaxies. Predictions for planned and proposed surveys have typically focused on average galaxy counts, assuming a random distribution of galaxies across the observed field. The first and most-massive galaxies, however, are expected to be tightly clustered, an effect known as cosmic variance. We show that cosmic variance is likely to be the dominant contribution to uncertainty for high-redshift mass and luminosity functions, and that median high-redshift and high-mass galaxy counts for planned observations lie significantly below average counts. Several different strategies are considered for improving our understanding of the first galaxies, including adding depth, area, and independent pointings. Adding independent pointings is shown to be the most efficient both for discovering the single highest-redshift galaxy and also for constraining mass and luminosity functions.",
keywords = "COSMIC VARIANCE, MASSIVE GALAXIES, BILLION YEARS, LUMINOSITY, MODEL, PREDICTIONS, UNIVERSE",
author = "Steinhardt, {Charles L.} and Jespersen, {Christian Kragh} and Linzer, {Nora B.}",
year = "2021",
month = dec,
day = "7",
doi = "10.3847/1538-4357/ac2a2f",
language = "English",
volume = "923",
journal = "Astrophysical Journal",
issn = "0004-637X",
publisher = "Institute of Physics Publishing, Inc",
number = "1",

}

RIS

TY - JOUR

T1 - Finding High-redshift Galaxies with JWST

AU - Steinhardt, Charles L.

AU - Jespersen, Christian Kragh

AU - Linzer, Nora B.

PY - 2021/12/7

Y1 - 2021/12/7

N2 - One of the primary goals for the upcoming James Webb Space Telescope is to observe the first galaxies. Predictions for planned and proposed surveys have typically focused on average galaxy counts, assuming a random distribution of galaxies across the observed field. The first and most-massive galaxies, however, are expected to be tightly clustered, an effect known as cosmic variance. We show that cosmic variance is likely to be the dominant contribution to uncertainty for high-redshift mass and luminosity functions, and that median high-redshift and high-mass galaxy counts for planned observations lie significantly below average counts. Several different strategies are considered for improving our understanding of the first galaxies, including adding depth, area, and independent pointings. Adding independent pointings is shown to be the most efficient both for discovering the single highest-redshift galaxy and also for constraining mass and luminosity functions.

AB - One of the primary goals for the upcoming James Webb Space Telescope is to observe the first galaxies. Predictions for planned and proposed surveys have typically focused on average galaxy counts, assuming a random distribution of galaxies across the observed field. The first and most-massive galaxies, however, are expected to be tightly clustered, an effect known as cosmic variance. We show that cosmic variance is likely to be the dominant contribution to uncertainty for high-redshift mass and luminosity functions, and that median high-redshift and high-mass galaxy counts for planned observations lie significantly below average counts. Several different strategies are considered for improving our understanding of the first galaxies, including adding depth, area, and independent pointings. Adding independent pointings is shown to be the most efficient both for discovering the single highest-redshift galaxy and also for constraining mass and luminosity functions.

KW - COSMIC VARIANCE

KW - MASSIVE GALAXIES

KW - BILLION YEARS

KW - LUMINOSITY

KW - MODEL

KW - PREDICTIONS

KW - UNIVERSE

U2 - 10.3847/1538-4357/ac2a2f

DO - 10.3847/1538-4357/ac2a2f

M3 - Journal article

VL - 923

JO - Astrophysical Journal

JF - Astrophysical Journal

SN - 0004-637X

IS - 1

M1 - 8

ER -

ID: 286851442