The Astrophysical Journal Supplement Series (Jan 2024)

High-quality Extragalactic Legacy-field Monitoring (HELM) with DECam: Project Overview and First Data Release

  • Ming-Yang Zhuang,
  • Qian Yang,
  • Yue Shen,
  • Monika Adamów,
  • Douglas N. Friedel,
  • R. A. Gruendl,
  • Zachary Stone,
  • Junyao Li,
  • Xin Liu,
  • Paul Martini,
  • Timothy M. C. Abbott,
  • Scott F. Anderson,
  • Roberto J. Assef,
  • Franz E. Bauer,
  • Richard Bielby,
  • W. N. Brandt,
  • Colin J. Burke,
  • Jorge Casares,
  • Yu-Ching Chen,
  • Gisella De Rosa,
  • Alex Drlica-Wagner,
  • Tom Dwelly,
  • Alice Eltvedt,
  • Gloria Fonseca Alvarez,
  • Jianyang Fu,
  • Cesar Fuentes,
  • Melissa L. Graham,
  • Catherine J. Grier,
  • Nathan Golovich,
  • Patrick B. Hall,
  • Patrick Hartigan,
  • Keith Horne,
  • Anton M. Koekemoer,
  • Mirko Krumpe,
  • Jennifer I. Li,
  • Chris Lidman,
  • Umang Malik,
  • Amelia Mangian,
  • Andrea Merloni,
  • Claudio Ricci,
  • Mara Salvato,
  • Rob Sharp,
  • David E. Trilling,
  • Brad E. Tucker,
  • Di Wen,
  • Zachary Wideman,
  • Yongquan Xue,
  • Zhefu Yu,
  • Catherine Zucker

DOI
https://doi.org/10.3847/1538-4365/ad7d01
Journal volume & issue
Vol. 274, no. 2
p. 42

Abstract

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High-quality Extragalactic Legacy-field Monitoring (HELM) is a long-term observing program that photometrically monitors several well-studied extragalactic legacy fields with the Dark Energy Camera (DECam) imager on the CTIO 4 m Blanco telescope. Since 2019 February, HELM has been monitoring regions within COSMOS, XMM-LSS, CDF-S, S-CVZ, ELAIS-S1, and SDSS Stripe 82 with few-day cadences in the ( u ) gri ( z ) bands, over a collective sky area of ∼38 deg ^2 . The main science goal of HELM is to provide high-quality optical light curves for a large sample of active galactic nuclei (AGNs), and to build decades-long time baselines when combining past and future optical light curves in these legacy fields. These optical images and light curves will facilitate the measurements of AGN reverberation mapping lags, as well as studies of AGN variability and its dependencies on accretion properties. In addition, the time-resolved and coadded DECam photometry will enable a broad range of science applications from galaxy evolution to time-domain science. We describe the design and implementation of the program and present the first data release that includes source catalogs and the first ∼3.5 yr of light curves during 2019A–2022A.

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