AEGIS: Galaxy spectral energy distributions from the X-ray to radio

N. P. Konidaris; P. Guhathakurta; K. Bundy; A. L. Coil; C. J. Conselice; M. C. Cooper; P. R.M. Eisenhardt; J. S. Huang; R. J. Ivison; S. A. Kassin; E. N. Kirby; J. M. Lotz; J. A. Newman; K. G. Noeske; R. M. Rich; T. A. Small; C. N.A. Willmer; S. P. Willner

doi:10.1086/517929

AEGIS: Galaxy spectral energy distributions from the X-ray to radio

N. P. Konidaris
, P. Guhathakurta
, K. Bundy
, A. L. Coil
, C. J. Conselice
, M. C. Cooper
, P. R.M. Eisenhardt
, J. S. Huang
, R. J. Ivison
, S. A. Kassin
, E. N. Kirby
, J. M. Lotz
, J. A. Newman
, K. G. Noeske
, R. M. Rich
, T. A. Small
, C. N.A. Willmer
, S. P. Willner

Steward Observatory

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

6 Scopus citations

Abstract

The All-Wavelength Extended Groth Strip International Survey (AEGIS) team presents broadband spectral energy distributions (SEDs), from X-ray to radio wavelengths, for 71 galaxies spanning the redshift range 0.55-1.16 (〈z〉 ∼ 0.7). Galaxies with secure redshifts are selected from a small (22 arcmin²) subsection of the Keck/ DEIMOS Galaxy Redshift Survey in the Extended Groth Strip field that has also been targeted for deep panchromatic imaging by ultraviolet (120-250 nm), optical (360-900 nm), optical/near-infrared (440-1600 nm), near-infrared (1200-2200 nm), mid/far-infrared (3.6-70 μm), and radio (6-20 cm). A typical galaxy in our sample is M_B = -19.82. The ultraviolet to mid-infrared portion of their SEDs are found to be bracketed by two stellaronly model SEDs: (1) an early burst followed by passive evolution and (2) a constant star formation rate since early times. This suggests that few of these galaxies are undergoing major starbursts. Approximately half the galaxies show a mid- to far-infrared excess relative to the model SEDs, consistent with thermal emission from interstellar dust. Two objects have power-law SEDs, indicating that they are dominated by active galactic nuclei; both are detected in X-rays. SEDs, from the ultraviolet to the infrared, follow expected trends: redder SEDs are associated with red U - B, early-type morphology, and low [O II] emission, and vice versa for blue SEDs.

Original language	English (US)
Pages (from-to)	L7-L10
Journal	Astrophysical Journal
Volume	660
Issue number	1 II
DOIs	https://doi.org/10.1086/517929
State	Published - May 1 2007

Keywords

Galaxies: evolution
Galaxies: general
Infrared: galaxies
Radio continuum: galaxies
Ultraviolet: galaxies
X-rays: galaxies

ASJC Scopus subject areas

Astronomy and Astrophysics
Space and Planetary Science

Access to Document

10.1086/517929

Cite this

Konidaris, N. P., Guhathakurta, P., Bundy, K., Coil, A. L., Conselice, C. J., Cooper, M. C., Eisenhardt, P. R. M., Huang, J. S., Ivison, R. J., Kassin, S. A., Kirby, E. N., Lotz, J. M., Newman, J. A., Noeske, K. G., Rich, R. M., Small, T. A., Willmer, C. N. A., & Willner, S. P. (2007). AEGIS: Galaxy spectral energy distributions from the X-ray to radio. Astrophysical Journal, 660(1 II), L7-L10. https://doi.org/10.1086/517929

Konidaris, NP, Guhathakurta, P, Bundy, K, Coil, AL, Conselice, CJ, Cooper, MC, Eisenhardt, PRM, Huang, JS, Ivison, RJ, Kassin, SA, Kirby, EN, Lotz, JM, Newman, JA, Noeske, KG, Rich, RM, Small, TA, Willmer, CNA & Willner, SP 2007, 'AEGIS: Galaxy spectral energy distributions from the X-ray to radio', Astrophysical Journal, vol. 660, no. 1 II, pp. L7-L10. https://doi.org/10.1086/517929

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title = "AEGIS: Galaxy spectral energy distributions from the X-ray to radio",

abstract = "The All-Wavelength Extended Groth Strip International Survey (AEGIS) team presents broadband spectral energy distributions (SEDs), from X-ray to radio wavelengths, for 71 galaxies spanning the redshift range 0.55-1.16 (〈z〉 ∼ 0.7). Galaxies with secure redshifts are selected from a small (22 arcmin2) subsection of the Keck/ DEIMOS Galaxy Redshift Survey in the Extended Groth Strip field that has also been targeted for deep panchromatic imaging by ultraviolet (120-250 nm), optical (360-900 nm), optical/near-infrared (440-1600 nm), near-infrared (1200-2200 nm), mid/far-infrared (3.6-70 μm), and radio (6-20 cm). A typical galaxy in our sample is MB = -19.82. The ultraviolet to mid-infrared portion of their SEDs are found to be bracketed by two stellaronly model SEDs: (1) an early burst followed by passive evolution and (2) a constant star formation rate since early times. This suggests that few of these galaxies are undergoing major starbursts. Approximately half the galaxies show a mid- to far-infrared excess relative to the model SEDs, consistent with thermal emission from interstellar dust. Two objects have power-law SEDs, indicating that they are dominated by active galactic nuclei; both are detected in X-rays. SEDs, from the ultraviolet to the infrared, follow expected trends: redder SEDs are associated with red U - B, early-type morphology, and low [O II] emission, and vice versa for blue SEDs.",

keywords = "Galaxies: evolution, Galaxies: general, Infrared: galaxies, Radio continuum: galaxies, Ultraviolet: galaxies, X-rays: galaxies",

author = "Konidaris, \{N. P.\} and P. Guhathakurta and K. Bundy and Coil, \{A. L.\} and Conselice, \{C. J.\} and Cooper, \{M. C.\} and Eisenhardt, \{P. R.M.\} and Huang, \{J. S.\} and Ivison, \{R. J.\} and Kassin, \{S. A.\} and Kirby, \{E. N.\} and Lotz, \{J. M.\} and Newman, \{J. A.\} and Noeske, \{K. G.\} and Rich, \{R. M.\} and Small, \{T. A.\} and Willmer, \{C. N.A.\} and Willner, \{S. P.\}",

year = "2007",

month = may,

day = "1",

doi = "10.1086/517929",

language = "English (US)",

volume = "660",

pages = "L7--L10",

journal = "Astrophysical Journal",

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publisher = "American Astronomical Society",

number = "1 II",

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TY - JOUR

T1 - AEGIS

T2 - Galaxy spectral energy distributions from the X-ray to radio

AU - Konidaris, N. P.

AU - Guhathakurta, P.

AU - Bundy, K.

AU - Coil, A. L.

AU - Conselice, C. J.

AU - Cooper, M. C.

AU - Eisenhardt, P. R.M.

AU - Huang, J. S.

AU - Ivison, R. J.

AU - Kassin, S. A.

AU - Kirby, E. N.

AU - Lotz, J. M.

AU - Newman, J. A.

AU - Noeske, K. G.

AU - Rich, R. M.

AU - Small, T. A.

AU - Willmer, C. N.A.

AU - Willner, S. P.

PY - 2007/5/1

Y1 - 2007/5/1

N2 - The All-Wavelength Extended Groth Strip International Survey (AEGIS) team presents broadband spectral energy distributions (SEDs), from X-ray to radio wavelengths, for 71 galaxies spanning the redshift range 0.55-1.16 (〈z〉 ∼ 0.7). Galaxies with secure redshifts are selected from a small (22 arcmin2) subsection of the Keck/ DEIMOS Galaxy Redshift Survey in the Extended Groth Strip field that has also been targeted for deep panchromatic imaging by ultraviolet (120-250 nm), optical (360-900 nm), optical/near-infrared (440-1600 nm), near-infrared (1200-2200 nm), mid/far-infrared (3.6-70 μm), and radio (6-20 cm). A typical galaxy in our sample is MB = -19.82. The ultraviolet to mid-infrared portion of their SEDs are found to be bracketed by two stellaronly model SEDs: (1) an early burst followed by passive evolution and (2) a constant star formation rate since early times. This suggests that few of these galaxies are undergoing major starbursts. Approximately half the galaxies show a mid- to far-infrared excess relative to the model SEDs, consistent with thermal emission from interstellar dust. Two objects have power-law SEDs, indicating that they are dominated by active galactic nuclei; both are detected in X-rays. SEDs, from the ultraviolet to the infrared, follow expected trends: redder SEDs are associated with red U - B, early-type morphology, and low [O II] emission, and vice versa for blue SEDs.

AB - The All-Wavelength Extended Groth Strip International Survey (AEGIS) team presents broadband spectral energy distributions (SEDs), from X-ray to radio wavelengths, for 71 galaxies spanning the redshift range 0.55-1.16 (〈z〉 ∼ 0.7). Galaxies with secure redshifts are selected from a small (22 arcmin2) subsection of the Keck/ DEIMOS Galaxy Redshift Survey in the Extended Groth Strip field that has also been targeted for deep panchromatic imaging by ultraviolet (120-250 nm), optical (360-900 nm), optical/near-infrared (440-1600 nm), near-infrared (1200-2200 nm), mid/far-infrared (3.6-70 μm), and radio (6-20 cm). A typical galaxy in our sample is MB = -19.82. The ultraviolet to mid-infrared portion of their SEDs are found to be bracketed by two stellaronly model SEDs: (1) an early burst followed by passive evolution and (2) a constant star formation rate since early times. This suggests that few of these galaxies are undergoing major starbursts. Approximately half the galaxies show a mid- to far-infrared excess relative to the model SEDs, consistent with thermal emission from interstellar dust. Two objects have power-law SEDs, indicating that they are dominated by active galactic nuclei; both are detected in X-rays. SEDs, from the ultraviolet to the infrared, follow expected trends: redder SEDs are associated with red U - B, early-type morphology, and low [O II] emission, and vice versa for blue SEDs.

KW - Galaxies: evolution

KW - Galaxies: general

KW - Infrared: galaxies

KW - Radio continuum: galaxies

KW - Ultraviolet: galaxies

KW - X-rays: galaxies

UR - https://www.scopus.com/pages/publications/34249096468

UR - https://www.scopus.com/pages/publications/34249096468#tab=citedBy

U2 - 10.1086/517929

DO - 10.1086/517929

M3 - Article

AN - SCOPUS:34249096468

SN - 0004-637X

VL - 660

SP - L7-L10

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 1 II

ER -

AEGIS: Galaxy spectral energy distributions from the X-ray to radio

Abstract

Keywords

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