Simulating JWST deep extragalactic imaging surveys and physical parameter recovery

Research output: Contribution to journal › Journal article › Research › peer-review

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Simulating JWST deep extragalactic imaging surveys and physical parameter recovery. / Kauffmann, O. B.; Le Fevre, O.; Ilbert, O.; Chevallard, J.; Williams, C. C.; Curtis-Lake, E.; Colina, L.; Perez-Gonzalez, P. G.; Pye, J. P.; Caputi, K.

In: Astronomy & Astrophysics, Vol. 640, A67, 13.08.2020.

Research output: Contribution to journal › Journal article › Research › peer-review

Harvard

Kauffmann, OB, Le Fevre, O, Ilbert, O, Chevallard, J, Williams, CC, Curtis-Lake, E, Colina, L, Perez-Gonzalez, PG, Pye, JP & Caputi, K 2020, 'Simulating JWST deep extragalactic imaging surveys and physical parameter recovery', Astronomy & Astrophysics, vol. 640, A67. https://doi.org/10.1051/0004-6361/202037450

APA

Kauffmann, O. B., Le Fevre, O., Ilbert, O., Chevallard, J., Williams, C. C., Curtis-Lake, E., Colina, L., Perez-Gonzalez, P. G., Pye, J. P., & Caputi, K. (2020). Simulating JWST deep extragalactic imaging surveys and physical parameter recovery. Astronomy & Astrophysics, 640, [A67]. https://doi.org/10.1051/0004-6361/202037450

Vancouver

Kauffmann OB, Le Fevre O, Ilbert O, Chevallard J, Williams CC, Curtis-Lake E et al. Simulating JWST deep extragalactic imaging surveys and physical parameter recovery. Astronomy & Astrophysics. 2020 Aug 13;640. A67. https://doi.org/10.1051/0004-6361/202037450

Author

Kauffmann, O. B. ; Le Fevre, O. ; Ilbert, O. ; Chevallard, J. ; Williams, C. C. ; Curtis-Lake, E. ; Colina, L. ; Perez-Gonzalez, P. G. ; Pye, J. P. ; Caputi, K. / Simulating JWST deep extragalactic imaging surveys and physical parameter recovery. In: Astronomy & Astrophysics. 2020 ; Vol. 640.

Bibtex

@article{caf0a58a5d2c45ea9d619bf2ef6d570b,
title = "Simulating JWST deep extragalactic imaging surveys and physical parameter recovery",
abstract = "We present a new prospective analysis of deep multi-band imaging with the James Webb Space Telescope (JWST). In this work, we investigate the recovery of high-redshift 5 6 and redshifts of 0 5 galaxy samples can be reduced to <0.01 arcmin(-2) with a limited impact on galaxy completeness. We investigate multiple high-redshift galaxy selection techniques and find that the best compromise between completeness and purity at 5",
keywords = "galaxies: high-redshift, galaxies: photometry, galaxies: distances and redshifts, galaxies: fundamental parameters, galaxies: evolution, SPECTRAL ENERGY-DISTRIBUTIONS, GALAXY LUMINOSITY FUNCTION, HUBBLE FRONTIER FIELDS, STAR-FORMING GALAXIES, PHOTOMETRIC REDSHIFTS, SPACE-TELESCOPE, STELLAR POPULATION, LEGACY SURVEY, EVOLUTION, COSMOS",
author = "Kauffmann, {O. B.} and {Le Fevre}, O. and O. Ilbert and J. Chevallard and Williams, {C. C.} and E. Curtis-Lake and L. Colina and Perez-Gonzalez, {P. G.} and Pye, {J. P.} and K. Caputi",
year = "2020",
month = aug,
day = "13",
doi = "10.1051/0004-6361/202037450",
language = "English",
volume = "640",
journal = "Astronomy & Astrophysics",
issn = "0004-6361",
publisher = "E D P Sciences",

}

RIS

TY - JOUR

T1 - Simulating JWST deep extragalactic imaging surveys and physical parameter recovery

AU - Kauffmann, O. B.

AU - Le Fevre, O.

AU - Ilbert, O.

AU - Chevallard, J.

AU - Williams, C. C.

AU - Curtis-Lake, E.

AU - Colina, L.

AU - Perez-Gonzalez, P. G.

AU - Pye, J. P.

AU - Caputi, K.

PY - 2020/8/13

Y1 - 2020/8/13

N2 - We present a new prospective analysis of deep multi-band imaging with the James Webb Space Telescope (JWST). In this work, we investigate the recovery of high-redshift 5 6 and redshifts of 0 5 galaxy samples can be reduced to <0.01 arcmin(-2) with a limited impact on galaxy completeness. We investigate multiple high-redshift galaxy selection techniques and find that the best compromise between completeness and purity at 5

AB - We present a new prospective analysis of deep multi-band imaging with the James Webb Space Telescope (JWST). In this work, we investigate the recovery of high-redshift 5 6 and redshifts of 0 5 galaxy samples can be reduced to <0.01 arcmin(-2) with a limited impact on galaxy completeness. We investigate multiple high-redshift galaxy selection techniques and find that the best compromise between completeness and purity at 5

KW - galaxies: high-redshift

KW - galaxies: photometry

KW - galaxies: distances and redshifts

KW - galaxies: fundamental parameters

KW - galaxies: evolution

KW - SPECTRAL ENERGY-DISTRIBUTIONS

KW - GALAXY LUMINOSITY FUNCTION

KW - HUBBLE FRONTIER FIELDS

KW - STAR-FORMING GALAXIES

KW - PHOTOMETRIC REDSHIFTS

KW - SPACE-TELESCOPE

KW - STELLAR POPULATION

KW - LEGACY SURVEY

KW - EVOLUTION

KW - COSMOS

U2 - 10.1051/0004-6361/202037450

DO - 10.1051/0004-6361/202037450

M3 - Journal article

VL - 640

JO - Astronomy & Astrophysics

JF - Astronomy & Astrophysics

SN - 0004-6361

M1 - A67

ER -

ID: 248233740