Multi-object Spectroscopy

Multi-Object Spectroscopy is a spectroscopic technique in observational astronomy that enables the simultaneous acquisition of spectra from multiple celestial sources within a single field of view, distinguished by its use of configurable aperture arrays or fiber-optic positioners to isolate light from individual targets.

514

Publications

29.6K

Citations

3.9K

Authors

652

Institutions

Publications per year

2017–2026

103

Publications

514

Authors

3.9K

  1. PB
    P. Bonifacio

    Galaxies, Etoiles, Physique et Instrumentation, France

    19 publications · 1.4K citations

    17

    h-index

  2. JB
    Joss Bland‐Hawthorn

    The University of Sydney, Australia

    17 publications · 2K citations

    15

    h-index

  3. GD
    Gavin Dalton

    University of Oxford, United Kingdom

    18 publications · 1.7K citations

    15

    h-index

  4. CJ
    C. J. Evans

    UK Astronomy Technology Centre, United Kingdom

    14 publications · 817 citations

    13

    h-index

  5. MC
    Matthew Colless

    Australian National University, Australia

    13 publications · 1.4K citations

    13

    h-index

1–5 of 3.9K

Venues

  1. 37

    h-index

  2. 37

    h-index

  3. The Astrophysical Journal

    ApJ · 70 publications · 4.6K citations

    36

    h-index

  4. The Astronomical Journal

    AJ · 36 publications · 3.3K citations

    26

    h-index

  5. Astronomy and Astrophysics

    38 publications · 2.6K citations

    25

    h-index

1–5