Major merging history in CANDELS. I. Evolution of the incidence of massive galaxy–galaxy pairs from z = 3 to z ∼ 0

Mantha, Kameswara Bharadwaj and McIntosh, Daniel H. and Brennan, Ryan and Ferguson, Henry C. and Kodra, Dritan and Newman, Jeffrey A. and Rafelski, Marc and Somerville, Rachel S. and Conselice, Christopher J. and Cook, Joshua S. and Hathi, Nimish P. and Koo, David C. and Lotz, Jennifer M. and Simmons, Brooke D. and Straughn, Amber N. and Snyder, Gregory F. and Wuyts, Stijn and Bell, Eric F and Dekel, Avishai and Kartaltepe, Jeyhan and Kocevski, Dale D. and Koekemoer, Anton M. and Lee, Seong-Kook and Lucas, Ray A. and Pacifici, Camilla and Peth, Michael A. and Barro, Guillermo and Dahlen, Tomas and Finkelstein, Steven L. and Fontana, Adriano and Galametz, Audrey and Grogin, Norman A. and Guo, Yicheng and Mobasher, Bahram and Nayyeri, Hooshang and Pérez-González, Pablo G. and Pforr, Janine and Santini, Paola and Stefanon, Mauro and Wiklind, Tommy (2018) Major merging history in CANDELS. I. Evolution of the incidence of massive galaxy–galaxy pairs from z = 3 to z ∼ 0. Monthly Notices of the Royal Astronomical Society, 475 (2). pp. 1549-1573. ISSN 1365-2966

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Abstract

The rate of major galaxy–galaxy merging is theoretically predicted to steadily increase with redshift during the peak epoch of massive galaxy development (1 ≤ z ≤ 3). We use close-pair statistics to objectively study the incidence of massive galaxies (stellar M1 > 2 × 1010 M⊙) hosting major companions (1 ≤ M1/M2 ≤ 4; i.e. <4:1) at six epochs spanning 0 < z < 3. We select companions from a nearly complete, mass-limited (≥5 × 109 M⊙) sample of 23 696 galaxies in the five Cosmic Assembly Near-Infrared Deep Extragalactic Legacy Survey fields and the Sloan Digital Sky Survey. Using 5–50 kpc projected separation and close redshift proximity criteria, we find that the major companion fraction fmc(z) based on stellar mass-ratio (MR) selection increases from 6 per cent (z ∼ 0) to 16 per cent (z ∼ 0.8), then turns over at z ∼ 1 and decreases to 7 per cent (z ∼ 3). Instead, if we use a major F160W flux-ratio (FR) selection, we find that fmc(z) increases steadily until z = 3 owing to increasing contamination from minor (MR > 4:1) companions at z > 1. We show that these evolutionary trends are statistically robust to changes in companion proximity. We find disagreements between published results are resolved when selection criteria are closely matched. If we compute merger rates using constant fraction-to-rate conversion factors (Cmerg,pair = 0.6 and Tobs,pair = 0.65 Gyr), we find that MR rates disagree with theoretical predictions at z > 1.5. Instead, if we use an evolving Tobs,pair(z) ∝ (1 + z)−2 from Snyder et al., our MR-based rates agree with theory at 0 < z < 3. Our analysis underscores the need for detailed calibration of Cmerg,pair and Tobs,pair as a function of redshift, mass, and companion selection criteria to better constrain the empirical major merger history.

Item Type: Article
Keywords: galaxies: evolution, galaxies: high-redshift, galaxies: interactions, galaxies: statistics
Schools/Departments: University of Nottingham, UK > Faculty of Science > School of Physics and Astronomy
Identification Number: https://doi.org/10.1093/mnras/stx3260
Depositing User: Eprints, Support
Date Deposited: 14 May 2018 10:53
Last Modified: 15 May 2018 02:22
URI: http://eprints.nottingham.ac.uk/id/eprint/51768

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