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Major Mergers Are Not the Dominant Trigger for High-accretion AGNs at z ∼ 2

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The MOSDEF Survey: No Significant Enhancement in Star Formation or Deficit in Metallicity in Merging Galaxy Pairs at 1.5 ≲ z ≲ 3.5∗

Tim J. Wilson, Alice E. Shapley, Ryan L. Sanders, Naveen A. Reddy, William R. Freeman, Mariska Kriek, Irene Shivaei, Alison L. Coil, Brian Siana, Bahram Mobasher, Sedona H. Price, Mojegan Azadi, Guillermo Barro, Laura de Groot, Tara Fetherolf, Francesca M. Fornasini, Gene C. K. Leung and Tom O. Zick
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Observational Constraints on the Merger History of Galaxies since z ≈ 6: Probabilistic Galaxy Pair Counts in the CANDELS Fields

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Automated distant galaxy merger classifications from Space Telescope images using the Illustris simulation

Peter E Freeman, Mark Vogelsberger, Lars Hernquist, et al.
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Time-average properties of z ∼ 0.6 major mergers: mergers significantly scatter high-z scaling relations

M Puech, H Flores, M Rodrigues, F Hammer and Y B Yang
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New criteria for the selection of galaxy close pairs from cosmological simulations: evolution of the major and minor merger fraction in MUSE deep fields

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SDSS-IV MaNGA: Galaxy Pair Fraction and Correlated Active Galactic Nuclei

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The frequency of dwarf galaxy multiples at low redshift in SDSS versus cosmological expectations

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An Alternate Approach to Measure Specific Star Formation Rates at

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Lyman-continuum leakage as dominant source of diffuse ionized gas in the Antennae galaxy

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The SFR–M* Correlation Extends to Low Mass at High Redshift

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