Dust Temperature Mapping

Dust Temperature Mapping is a methodological framework in infrared astronomy that enables the spatial characterization of thermal emission from interstellar dust by deriving temperature distributions from spectral energy fitting across far-infrared and mid-infrared wavelengths.

209

Publications

27.8K

Citations

1.4K

Authors

415

Institutions

Publications per year

2017–2026

31

Authors

1.4K

  1. PG
    P. G. Martin

    University of Toronto, Canada

    15 publications · 2.2K citations

    15

    h-index

  2. MJ
    M. Juvela

    University of Helsinki, Finland

    11 publications · 1.2K citations

    11

    h-index

  3. DW
    D. Ward–Thompson

    Cardiff University, United Kingdom

    11 publications · 1.2K citations

    11

    h-index

  4. SM
    S. Molinari

    National Institute for Astrophysics, Italy

    9 publications · 1.4K citations

    9

    h-index

  5. PM
    P. M. Harvey

    The University of Texas at Austin, United States

    9 publications · 886 citations

    9

    h-index

1–5 of 1.4K

Venues

  1. The Astrophysical Journal

    ApJ · 61 publications · 18.7K citations

    36

    h-index

  2. Astronomy and Astrophysics

    52 publications · 4.5K citations

    33

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    24 publications · 1.1K citations

    18

    h-index

  4. The Astronomical Journal

    AJ · 9 publications · 651 citations

    9

    h-index

  5. Springer Link (Chiba Institute of Technology)

    Repository · 9 publications · 373 citations

    9

    h-index

1–5