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Active Galaxy Science in the LSST Deep-Drilling Fields: Footprints, Cadence Requirements, and Total-Depth Requirements

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arxiv 1811.06542 v2 pith:QEPN3FF3 submitted 2018-11-15 astro-ph.IM astro-ph.GAastro-ph.HE

Active Galaxy Science in the LSST Deep-Drilling Fields: Footprints, Cadence Requirements, and Total-Depth Requirements

classification astro-ph.IM astro-ph.GAastro-ph.HE
keywords requirementscadencetotal-depthddfsdeep-drillingfieldsfootprintslsst
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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This white paper specifies the footprints, cadence requirements, and total-depth requirements needed to allow the most-successful AGN studies in the four currently selected LSST Deep-Drilling Fields (DDFs): ELAIS-S1, XMM-LSS, CDF-S, and COSMOS. The information provided on cadence and total-depth requirements will also likely be applicable to enabling effective AGN science in any additional DDFs that are chosen.

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Cited by 4 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. AGN radiative feedback as the main regulator of [O III] outflow activity and obscuration in X-ray AGN

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  2. The Distinctive Evolution and Spectral Energy Distribution of Binary Massive Black Hole Accretion

    astro-ph.HE 2026-07 conditional novelty 6.0

    Combining three accretion disk states for binary massive black holes, the paper predicts a spectrum 'notch' and a mass-ratio evolution attractor at q~1e-3 for extreme-mass-ratio binaries.

  3. VAR-PZnn: A machine-learning framework for AGN photometric redshifts using color and variability-based features

    astro-ph.GA 2026-07 conditional novelty 6.0

    VAR-PZnn combines ZTF g-band variability features with optical, MIR and NIR photometry in a mixture-density network to estimate AGN photometric redshifts with σ_NMAD=0.058 and an 8.2% outlier fraction on a 72,728-sour...

  4. AGN radiative feedback as the main regulator of [O III] outflow activity and obscuration in X-ray AGN

    astro-ph.GA 2026-06 unverdicted novelty 4.0

    Higher Eddington ratio AGN exhibit increased [O III] outflow incidence and reduced obscuration, supporting radiative feedback as the regulator.