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The ISO/NASA Key Project on AGN Spectral Energy Distributions (Characteristics of the ISO Data)

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Paper breakdownThe authors' claims, conditions and measurements, as JSON Signed receiptProof this review has not been altered
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Eric J. Hooper (1), Belinda J. Wilkes (1), Kim K. McLeod (2), Martin S. Elvis (1), Chris D. Impey (3), Carol J. Lonsdale (4), Matt A. Malkan (5), Jonathan C. McDowell (1) ((1) Harvard-Smithsonian CfA
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(2) Wellesley College, (3) Steward Observatory, (4) IPAC, (5) UCLA)

Astrophysics · Submitted 5 Feb 1999

abstract compiled · 2026-09-23 · no language-model review

The authors' main claim This paper presents an overview of the analysis and reduction techniques, as well as general trends within the data set (comparisons with IRAS fluxes, uncertainties as a function of background sky brightness, and an analysis of vignetting corrections in chopped observing mode).

how it is stated · asserted 0.99 read the record →

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arXiv IDastro-ph/9902099 (version 1)
Pith IDKPELY6MF, Pith's permanent record of this paper and its review
Citation(2) Wellesley College, (3) Steward Observatory, (4) IPAC, (5) UCLA), Belinda J. Wilkes (1), Carol J. Lonsdale (4), Chris D. Impey (3), Eric J. Hooper (1), Jonathan C. McDowell (1) ((1) Harvard-Smithsonian CfA, Kim K. McLeod (2), Martin S. Elvis (1), Matt A. Malkan (5). "The ISO/NASA Key Project on AGN Spectral Energy Distributions (Characteristics of the ISO Data)." arXiv:astro-ph/9902099 (1999). https://pith.science/paper/KPELY6MF
Claim paper

The compiled record

The paper's own sentences, arranged. Each label is drawn from a closed vocabulary; the number beside it is the probability the classifier gave that label. Numbers in the tables are the authors', checked by code. No sentence in this record was written by a model.

Open the compiled record

Compiled by classifier-1.13-20260917 via OpenRouter, question bank abstract-p1-20260923, 2026-09-23: 1 request, 4,912 input tokens, $0.0002 reported.

What the abstract itself states, as probabilities: claims first 0.03 · states limitation 0.41 · human participants 0.02 · controlled comparison 0.13 · randomized assignment 0.02 · states quantitative result 0.58 · compares with prior results 0.88 · mentions code or data availability 0.04.

The abstract, sentence by sentence

arXiv listing abstract v1. Results and the main claim are underlined; .

The U.S. ISO Key Project on quasar spectral energy distributions seeks to better understand the very broad-band emission features of quasars from radio to X-rays. A key element of this project is observations of 72 quasars with the ISOPHOT instrument at 8 bands, from 5 to 200 microns. The sample was chosen to span a wide range of redshifts and quasar types. This paper presents an overview of the analysis and reduction techniques, as well as general trends within the data set (comparisons with IRAS fluxes, uncertainties as a function of background sky brightness, and an analysis of vignetting corrections in chopped observing mode). A more detailed look at a few objects in the sample is presented in Wilkes et al. 1999, astro-ph/9902084.

background contribution method result interpretation main claim

What the classifier reports for each sentence. The number is the probability it gave the label.
#sentencerolethe authors' own workstates the main conclusionstrength
s0 The U.S. background 0.78 0.05 0.01 unclear 1.00
s1 ISO Key Project on quasar spectral energy distributions seeks to better understand the very broad-band emission features of quasars from radio to X-rays. contribution 0.53 0.36 0.06 asserted 0.95
s2 A key element of this project is observations of 72 quasars with the ISOPHOT instrument at 8 bands, from 5 to 200 microns. method 0.96 0.82 0.04 asserted 1.00
s3 The sample was chosen to span a wide range of redshifts and quasar types. method 0.96 0.58 0.03 asserted 1.00
s4 This paper presents an overview of the analysis and reduction techniques, as well as general trends within the data set (comparisons with IRAS fluxes, uncertainties as a function of background sky brightness, and an analysis of vignetting corrections in chopped observing mode). contribution 0.86 0.85 0.11 asserted 0.99
s5 A more detailed look at a few objects in the sample is presented in Wilkes et al. 1999, astro-ph/9902084. background 0.49 0.20 0.02 asserted 0.98

What kind of paper the classifier reports this is: dataset or benchmark 0.51 · evidence from observation or experiment 0.58.

What was examined, and what was not

sources read
  • arXiv listing abstract v1
not examined
  • full text
  • figures and tables
  • references and citing sentences
  • relations to other papers
levels run
  • P abstract
not run
  • S sections
  • T body sentences
  • C citations
  • R cross-paper relations

Every quoted sentence on this record is the authors'. Every label is from Pith's closed vocabulary, with the probability shown beside it. Every number in the measurements table is the authors', checked by code. Record as JSON

The paper
Original abstract

The U.S. ISO Key Project on quasar spectral energy distributions seeks to better understand the very broad-band emission features of quasars from radio to X-rays. A key element of this project is observations of 72 quasars with the ISOPHOT instrument at 8 bands, from 5 to 200 microns. The sample was chosen to span a wide range of redshifts and quasar types. This paper presents an overview of the analysis and reduction techniques, as well as general trends within the data set (comparisons with IRAS fluxes, uncertainties as a function of background sky brightness, and an analysis of vignetting corrections in chopped observing mode). A more detailed look at a few objects in the sample is presented in Wilkes et al. 1999, astro-ph/9902084.

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