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The dusty SF history of distant galaxies and modelling tools
Astrophysics · Submitted 28 Jun 2000
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim I emphasize the importance of dust reprocessing in the high--z universe, as demonstrated in particular by IR and sub-mm data.
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The abstract, sentence by sentence
I review recent advances in the determination of the cosmic history of star formation, and its relevance in our understanding of the formation of structures. I emphasize the importance of dust reprocessing in the high--z universe, as demonstrated in particular by IR and sub-mm data. This demand a panchromatic approach to observations and suitable modelling tools. I summarize the basic requirements for these models and to what extent they are satisfied by models published so far.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | I review recent advances in the determination of the cosmic history of star formation, and its relevance in our understanding of the formation of structures. | contribution 0.73 | 0.19 | 0.10 | unclear 0.56 |
| s1 | I emphasize the importance of dust reprocessing in the high--z universe, as demonstrated in particular by IR and sub-mm data. | background 0.62 | 0.11 | 0.21 | asserted 1.00 |
| s2 | This demand a panchromatic approach to observations and suitable modelling tools. | background 0.52 | 0.07 | 0.16 | asserted 0.98 |
| s3 | I summarize the basic requirements for these models and to what extent they are satisfied by models published so far. | contribution 0.82 | 0.52 | 0.13 | asserted 0.60 |
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The paper
Original abstract
I review recent advances in the determination of the cosmic history of star formation, and its relevance in our understanding of the formation of structures. I emphasize the importance of dust reprocessing in the high--z universe, as demonstrated in particular by IR and sub-mm data. This demand a panchromatic approach to observations and suitable modelling tools. I summarize the basic requirements for these models and to what extent they are satisfied by models published so far.
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Papers whose main result relates to this one's
States the same result 1 paper
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We emphasize the importance of dust reprocessing in the high--z universe, as demonstrated in particular by IR and sub-mm data.
The dusty SF history of high-z galaxies, modelling tools and future prospects · 1.00
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