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• W2000957087 endingPage "116" @default.
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• W2000957087 abstract "Phenomenological models for evolution of dusty and E/S0 galaxies, respectively, are developed to address two major questions concerning galaxy populations in deep infrared (IR) surveys: (1) Do normal late-type galaxies or starburst galaxies (including galaxies with obscured active galactic nuclei) dominate among sources in deep IR surveys? (2) How much do E/S0 galaxies contribute to the counts in deep mid-infrared (MIR: 3-20 μm) surveys? Among three new models for evolution of dusty galaxies, it is assumed in model S1 that starburst galaxies are the dominant population and in model S2 that normal galaxies dominate. Model S3 is an intermediate model. Comparing the model predictions with a wide range of observational data collected from the literature, we find that none of these models can be ruled out, given the uncertainties of the data. We show that the most direct method to distinguish these models is to compare the predicted color distributions of IR galaxies with observations, which will soon be available from the SIRTF Wide-Area Infrared Extragalactic (SWIRE) survey. The models for E/S0 galaxies follow a simple passive evolution approach. Among the three E/S0 models (E1, E2, and E3) investigated in this paper, model E2, which is specified by a peak formation redshift zpeak = 2 and an e-folding formation timescale ω = 2 Gyr, fits the data best. This suggests a synchronization between the evolution of E/S0 galaxies and that of starburst galaxies, in the sense that the peak of the formation function of E/S0 galaxies (zpeak = 2) is close to the peak of the evolution functions of starburst galaxies (zpeak = 1.4). We find that E/S0 galaxies contribute about 10%-30% of the counts in the MIR bands of less than 10 μm and up to 30%-50% of the optical/near-IR counts in the bright end. Their contributions to counts in the UV (2000 Å) and in the longer wavelength IR (≥12 μm) bands are negligible. Taking into account this contribution, new predictions for counts and confusion limits in the SIRTF bands are presented." @default.
• W2000957087 created "2016-06-24" @default.
• W2000957087 creator A5006293834 @default.
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• W2000957087 creator A5056373596 @default.
• W2000957087 creator A5081811248 @default.
• W2000957087 creator A5088456706 @default.
• W2000957087 date "2003-04-10" @default.
• W2000957087 modified "2023-10-03" @default.
• W2000957087 title "Models for Evolution of Dusty and E/S0 Galaxies Seen in Multiband Surveys" @default.
• W2000957087 cites W1484400061 @default.
• W2000957087 cites W1544224100 @default.
• W2000957087 cites W1573037074 @default.
• W2000957087 cites W1606766154 @default.
• W2000957087 cites W1607434071 @default.
• W2000957087 cites W1629401862 @default.
• W2000957087 cites W1681063222 @default.
• W2000957087 cites W1963799757 @default.
• W2000957087 cites W1965732366 @default.
• W2000957087 cites W1968297864 @default.
• W2000957087 cites W1971306567 @default.
• W2000957087 cites W1973808059 @default.
• W2000957087 cites W1977875822 @default.
• W2000957087 cites W1978480760 @default.
• W2000957087 cites W1980454973 @default.
• W2000957087 cites W1980514159 @default.
• W2000957087 cites W1981528645 @default.
• W2000957087 cites W1982555406 @default.
• W2000957087 cites W1986010423 @default.
• W2000957087 cites W1986407319 @default.
• W2000957087 cites W1988786669 @default.
• W2000957087 cites W1990726182 @default.
• W2000957087 cites W1991526001 @default.
• W2000957087 cites W1996419423 @default.
• W2000957087 cites W1996581037 @default.
• W2000957087 cites W1999264850 @default.
• W2000957087 cites W1999600037 @default.
• W2000957087 cites W2001441366 @default.
• W2000957087 cites W2002794632 @default.
• W2000957087 cites W2003050568 @default.
• W2000957087 cites W2004557233 @default.
• W2000957087 cites W2013536682 @default.
• W2000957087 cites W2020547167 @default.
• W2000957087 cites W2021460372 @default.
• W2000957087 cites W2023869431 @default.
• W2000957087 cites W2024000946 @default.
• W2000957087 cites W2025802512 @default.
• W2000957087 cites W2026074979 @default.
• W2000957087 cites W2027209393 @default.
• W2000957087 cites W2027825752 @default.
• W2000957087 cites W2029193721 @default.
• W2000957087 cites W2038384670 @default.
• W2000957087 cites W2043685494 @default.
• W2000957087 cites W2045213752 @default.
• W2000957087 cites W2046909799 @default.
• W2000957087 cites W2047890375 @default.
• W2000957087 cites W2052305773 @default.
• W2000957087 cites W2053591448 @default.
• W2000957087 cites W2055499986 @default.
• W2000957087 cites W2056003967 @default.
• W2000957087 cites W2061562981 @default.
• W2000957087 cites W2063116743 @default.
• W2000957087 cites W2070304421 @default.
• W2000957087 cites W2072682817 @default.
• W2000957087 cites W2074255988 @default.
• W2000957087 cites W2075988470 @default.
• W2000957087 cites W2078435760 @default.
• W2000957087 cites W2082012530 @default.
• W2000957087 cites W2083227489 @default.
• W2000957087 cites W2084061910 @default.
• W2000957087 cites W2084263945 @default.
• W2000957087 cites W2085110299 @default.
• W2000957087 cites W2085426743 @default.
• W2000957087 cites W2088864336 @default.
• W2000957087 cites W2095225003 @default.
• W2000957087 cites W2097999451 @default.
• W2000957087 cites W2117629212 @default.
• W2000957087 cites W2123310675 @default.
• W2000957087 cites W2132073473 @default.
• W2000957087 cites W2134407184 @default.
• W2000957087 cites W2137023092 @default.
• W2000957087 cites W2139632325 @default.
• W2000957087 cites W2140887005 @default.
• W2000957087 cites W2144286571 @default.
• W2000957087 cites W2146518005 @default.
• W2000957087 cites W2147847259 @default.
• W2000957087 cites W2160325371 @default.
• W2000957087 cites W2163832108 @default.
• W2000957087 cites W2164494399 @default.
• W2000957087 cites W2168126149 @default.
• W2000957087 cites W2168495929 @default.
• W2000957087 cites W2276876173 @default.
• W2000957087 cites W2326277288 @default.
• W2000957087 cites W2591733255 @default.
• W2000957087 cites W2951408172 @default.
• W2000957087 cites W2951581092 @default.
• W2000957087 cites W2951752678 @default.

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