The Chandra Deep Field-North survey. VIII. X-ray constraints on spiral galaxies from 0.4 < z < 1.5

A. E. Hornschemeier; W. N. Brandt; D. M. Alexander; F. E. Bauer; G. P. Garmire; D. P. Schneider; M. W. Bautz; G. Chartas

doi:10.1086/338802

The Chandra Deep Field-North survey. VIII. X-ray constraints on spiral galaxies from 0.4 < z < 1.5

A. E. Hornschemeier, W. N. Brandt, D. M. Alexander, F. E. Bauer, G. P. Garmire, D. P. Schneider, M. W. Bautz, G. Chartas

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Abstract

We present a statistical X-ray study of spiral galaxies in the Hubble Deep Field-North and its flanking fields using the Chandra Deep Field-North 1 Ms data set. We find that ≈L* galaxies with 0.4 ≲ z ≲ 1.5 have X-ray luminosity and ratios of X-ray to B-band luminosity similar to those in the local universe. The data, however, are consistent with an increase in both by a factor of ≈2-3. We have also determined that typical spiral galaxies at 0.4 ≲ z ≲ 1.5 should be detected in the 0.5-2 keV band in the flux range (3-6) × 10^-18 erg cm^-2 s^-1.

Original language	English (US)
Pages (from-to)	82-87
Number of pages	6
Journal	Astrophysical Journal
Volume	568
Issue number	1 I
DOIs	https://doi.org/10.1086/338802
State	Published - Mar 20 2002

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

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@article{ac8282d9988d4eff906b6b65e2a0eb29,

title = "The Chandra Deep Field-North survey. VIII. X-ray constraints on spiral galaxies from 0.4 < z < 1.5",

abstract = "We present a statistical X-ray study of spiral galaxies in the Hubble Deep Field-North and its flanking fields using the Chandra Deep Field-North 1 Ms data set. We find that ≈L* galaxies with 0.4 ≲ z ≲ 1.5 have X-ray luminosity and ratios of X-ray to B-band luminosity similar to those in the local universe. The data, however, are consistent with an increase in both by a factor of ≈2-3. We have also determined that typical spiral galaxies at 0.4 ≲ z ≲ 1.5 should be detected in the 0.5-2 keV band in the flux range (3-6) × 10-18 erg cm-2 s-1.",

author = "Hornschemeier, {A. E.} and Brandt, {W. N.} and Alexander, {D. M.} and Bauer, {F. E.} and Garmire, {G. P.} and Schneider, {D. P.} and Bautz, {M. W.} and G. Chartas",

year = "2002",

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doi = "10.1086/338802",

language = "English (US)",

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journal = "Astrophysical Journal",

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TY - JOUR

T1 - The Chandra Deep Field-North survey. VIII. X-ray constraints on spiral galaxies from 0.4 < z < 1.5

AU - Hornschemeier, A. E.

AU - Brandt, W. N.

AU - Alexander, D. M.

AU - Bauer, F. E.

AU - Garmire, G. P.

AU - Schneider, D. P.

AU - Bautz, M. W.

AU - Chartas, G.

PY - 2002/3/20

Y1 - 2002/3/20

N2 - We present a statistical X-ray study of spiral galaxies in the Hubble Deep Field-North and its flanking fields using the Chandra Deep Field-North 1 Ms data set. We find that ≈L* galaxies with 0.4 ≲ z ≲ 1.5 have X-ray luminosity and ratios of X-ray to B-band luminosity similar to those in the local universe. The data, however, are consistent with an increase in both by a factor of ≈2-3. We have also determined that typical spiral galaxies at 0.4 ≲ z ≲ 1.5 should be detected in the 0.5-2 keV band in the flux range (3-6) × 10-18 erg cm-2 s-1.

AB - We present a statistical X-ray study of spiral galaxies in the Hubble Deep Field-North and its flanking fields using the Chandra Deep Field-North 1 Ms data set. We find that ≈L* galaxies with 0.4 ≲ z ≲ 1.5 have X-ray luminosity and ratios of X-ray to B-band luminosity similar to those in the local universe. The data, however, are consistent with an increase in both by a factor of ≈2-3. We have also determined that typical spiral galaxies at 0.4 ≲ z ≲ 1.5 should be detected in the 0.5-2 keV band in the flux range (3-6) × 10-18 erg cm-2 s-1.

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U2 - 10.1086/338802

DO - 10.1086/338802

M3 - Review article

AN - SCOPUS:0000870040

SN - 0004-637X

VL - 568

SP - 82

EP - 87

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 1 I

ER -

The Chandra Deep Field-North survey. VIII. X-ray constraints on spiral galaxies from 0.4 < z < 1.5

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