Constraints on Cosmology and Baryonic Feedback with the Deep Lens Survey Using Galaxy-Galaxy and Galaxy-Mass Power Spectra

Mijin Yoon; M. James Jee; J. Anthony Tyson; Samuel Schmidt; David Wittman; Ami Choi

doi:10.3847/1538-4357/aaf3a9

Constraints on Cosmology and Baryonic Feedback with the Deep Lens Survey Using Galaxy-Galaxy and Galaxy-Mass Power Spectra

Mijin Yoon, M. James Jee, J. Anthony Tyson, Samuel Schmidt, David Wittman, Ami Choi

Research output: Contribution to journal › Article › peer-review

4 Citations (Scopus)

Abstract

We present cosmological parameter measurements from the Deep Lens Survey (DLS) using galaxy-mass and galaxy-galaxy power spectra in the multipole range ℓ = 250-2000. We measure galaxy-galaxy power spectra from two lens bins centered at z ∼ 0.27 and 0.54 and galaxy-mass power spectra by cross-correlating the positions of galaxies in these two lens bins with galaxy shapes in two source bins centered at z ∼ 0.64 and 1.1. We marginalize over a baryonic feedback process using a single-parameter representation and a sum of neutrino masses, as well as photometric redshift and shear calibration systematic uncertainties. For a flat ΛCDM cosmology, we determine , in good agreement with our previous DLS cosmic shear and the Planck cosmic microwave background (CMB) measurements. Without the baryonic feedback marginalization, S ₈ decreases by because the dark-matter-only power spectrum lacks the suppression at the highest ℓ values owing to active galactic nucleus (AGN) feedback. Together with the Planck CMB measurements, we constrain the baryonic feedback parameter to , which suggests an interesting possibility that the actual AGN feedback might be stronger than the recipe used in the OverWhelmingly Large cosmological hydrodynamical Simulations. The interpretation is limited by the validity of the baryonic feedback simulation and the one-parameter representation of the effect.

Original language	English
Article number	111
Journal	Astrophysical Journal
Volume	870
Issue number	2
DOIs	https://doi.org/10.3847/1538-4357/aaf3a9
Publication status	Published - 2019 Jan 10

Bibliographical note

Funding Information:
We thank the anonymous referee for his/her constructive suggestions for improving the quality of the paper. We also thank Kyle Finner and Cris Sabiu for their careful reading of the manuscript and providing useful comments. M. J. Jee acknowledges support for the current research from the National Research Foundation of Korea under program nos. 2017R1A2B2004644 and 2017R1A4A1015178. M. Yoon acknowledges support from the Yonsei University Observatory–KASI Joint Research Program (2018). J. A. Tyson and S. Schmidt acknowledge partial support from DOE grant DE-SC0009999 and NSF/ AURA grant N56981C.

Publisher Copyright:
© 2019. The American Astronomical Society. All rights reserved..

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

Access to Document

10.3847/1538-4357/aaf3a9

Cite this

@article{18840ea1dc714c54835a4e66cd896840,

title = "Constraints on Cosmology and Baryonic Feedback with the Deep Lens Survey Using Galaxy-Galaxy and Galaxy-Mass Power Spectra",

abstract = "We present cosmological parameter measurements from the Deep Lens Survey (DLS) using galaxy-mass and galaxy-galaxy power spectra in the multipole range ℓ = 250-2000. We measure galaxy-galaxy power spectra from two lens bins centered at z ∼ 0.27 and 0.54 and galaxy-mass power spectra by cross-correlating the positions of galaxies in these two lens bins with galaxy shapes in two source bins centered at z ∼ 0.64 and 1.1. We marginalize over a baryonic feedback process using a single-parameter representation and a sum of neutrino masses, as well as photometric redshift and shear calibration systematic uncertainties. For a flat ΛCDM cosmology, we determine , in good agreement with our previous DLS cosmic shear and the Planck cosmic microwave background (CMB) measurements. Without the baryonic feedback marginalization, S 8 decreases by because the dark-matter-only power spectrum lacks the suppression at the highest ℓ values owing to active galactic nucleus (AGN) feedback. Together with the Planck CMB measurements, we constrain the baryonic feedback parameter to , which suggests an interesting possibility that the actual AGN feedback might be stronger than the recipe used in the OverWhelmingly Large cosmological hydrodynamical Simulations. The interpretation is limited by the validity of the baryonic feedback simulation and the one-parameter representation of the effect.",

author = "Mijin Yoon and {James Jee}, M. and {Anthony Tyson}, J. and Samuel Schmidt and David Wittman and Ami Choi",

note = "Funding Information: We thank the anonymous referee for his/her constructive suggestions for improving the quality of the paper. We also thank Kyle Finner and Cris Sabiu for their careful reading of the manuscript and providing useful comments. M. J. Jee acknowledges support for the current research from the National Research Foundation of Korea under program nos. 2017R1A2B2004644 and 2017R1A4A1015178. M. Yoon acknowledges support from the Yonsei University Observatory–KASI Joint Research Program (2018). J. A. Tyson and S. Schmidt acknowledge partial support from DOE grant DE-SC0009999 and NSF/ AURA grant N56981C. Publisher Copyright: {\textcopyright} 2019. The American Astronomical Society. All rights reserved..",

year = "2019",

month = jan,

day = "10",

doi = "10.3847/1538-4357/aaf3a9",

language = "English",

volume = "870",

journal = "Astrophysical Journal",

issn = "0004-637X",

publisher = "IOP Publishing Ltd.",

number = "2",

}

TY - JOUR

T1 - Constraints on Cosmology and Baryonic Feedback with the Deep Lens Survey Using Galaxy-Galaxy and Galaxy-Mass Power Spectra

AU - Yoon, Mijin

AU - James Jee, M.

AU - Anthony Tyson, J.

AU - Schmidt, Samuel

AU - Wittman, David

AU - Choi, Ami

N1 - Funding Information: We thank the anonymous referee for his/her constructive suggestions for improving the quality of the paper. We also thank Kyle Finner and Cris Sabiu for their careful reading of the manuscript and providing useful comments. M. J. Jee acknowledges support for the current research from the National Research Foundation of Korea under program nos. 2017R1A2B2004644 and 2017R1A4A1015178. M. Yoon acknowledges support from the Yonsei University Observatory–KASI Joint Research Program (2018). J. A. Tyson and S. Schmidt acknowledge partial support from DOE grant DE-SC0009999 and NSF/ AURA grant N56981C. Publisher Copyright: © 2019. The American Astronomical Society. All rights reserved..

PY - 2019/1/10

Y1 - 2019/1/10

N2 - We present cosmological parameter measurements from the Deep Lens Survey (DLS) using galaxy-mass and galaxy-galaxy power spectra in the multipole range ℓ = 250-2000. We measure galaxy-galaxy power spectra from two lens bins centered at z ∼ 0.27 and 0.54 and galaxy-mass power spectra by cross-correlating the positions of galaxies in these two lens bins with galaxy shapes in two source bins centered at z ∼ 0.64 and 1.1. We marginalize over a baryonic feedback process using a single-parameter representation and a sum of neutrino masses, as well as photometric redshift and shear calibration systematic uncertainties. For a flat ΛCDM cosmology, we determine , in good agreement with our previous DLS cosmic shear and the Planck cosmic microwave background (CMB) measurements. Without the baryonic feedback marginalization, S 8 decreases by because the dark-matter-only power spectrum lacks the suppression at the highest ℓ values owing to active galactic nucleus (AGN) feedback. Together with the Planck CMB measurements, we constrain the baryonic feedback parameter to , which suggests an interesting possibility that the actual AGN feedback might be stronger than the recipe used in the OverWhelmingly Large cosmological hydrodynamical Simulations. The interpretation is limited by the validity of the baryonic feedback simulation and the one-parameter representation of the effect.

AB - We present cosmological parameter measurements from the Deep Lens Survey (DLS) using galaxy-mass and galaxy-galaxy power spectra in the multipole range ℓ = 250-2000. We measure galaxy-galaxy power spectra from two lens bins centered at z ∼ 0.27 and 0.54 and galaxy-mass power spectra by cross-correlating the positions of galaxies in these two lens bins with galaxy shapes in two source bins centered at z ∼ 0.64 and 1.1. We marginalize over a baryonic feedback process using a single-parameter representation and a sum of neutrino masses, as well as photometric redshift and shear calibration systematic uncertainties. For a flat ΛCDM cosmology, we determine , in good agreement with our previous DLS cosmic shear and the Planck cosmic microwave background (CMB) measurements. Without the baryonic feedback marginalization, S 8 decreases by because the dark-matter-only power spectrum lacks the suppression at the highest ℓ values owing to active galactic nucleus (AGN) feedback. Together with the Planck CMB measurements, we constrain the baryonic feedback parameter to , which suggests an interesting possibility that the actual AGN feedback might be stronger than the recipe used in the OverWhelmingly Large cosmological hydrodynamical Simulations. The interpretation is limited by the validity of the baryonic feedback simulation and the one-parameter representation of the effect.

UR - http://www.scopus.com/inward/record.url?scp=85060228550&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=85060228550&partnerID=8YFLogxK

U2 - 10.3847/1538-4357/aaf3a9

DO - 10.3847/1538-4357/aaf3a9

M3 - Article

AN - SCOPUS:85060228550

SN - 0004-637X

VL - 870

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 2

M1 - 111

ER -

Constraints on Cosmology and Baryonic Feedback with the Deep Lens Survey Using Galaxy-Galaxy and Galaxy-Mass Power Spectra

Abstract

Bibliographical note

All Science Journal Classification (ASJC) codes

Access to Document

Other files and links

Fingerprint

Cite this