Deep Extragalactic VIsible Legacy Survey (DEVILS): Stellar Mass Growth by Morphological Type since z=1

Abdolhosein Hashemizadeh; Simon P. Driver; Luke J. M. Davies; Aaron S. G. Robotham; Sabine Bellstedt; Rogier A. Windhorst; Malcolm Bremer; Steven Phillipps; Matt Jarvis; Benne W. Holwerda; Claudia del P. Lagos; Soheil Koushan; Malgorzata Siudek; Natasha Maddox; Jessica E. Thorne; Pascal Elahi

doi:10.1093/mnras/stab600

Deep Extragalactic VIsible Legacy Survey (DEVILS): Stellar Mass Growth by Morphological Type since z=1

Abdolhosein Hashemizadeh, Simon P. Driver, Luke J. M. Davies, Aaron S. G. Robotham, Sabine Bellstedt, Rogier A. Windhorst, Malcolm Bremer, Steven Phillipps, Matt Jarvis, Benne W. Holwerda, Claudia del P. Lagos, Soheil Koushan, Malgorzata Siudek, Natasha Maddox, Jessica E. Thorne, Pascal Elahi

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Abstract

Using high-resolution Hubble Space Telescope imaging data, we perform a visual morphological classification of $\sim 36,000$ galaxies at $z 1$ as the fraction of irregular galaxies and merger systems (when observed at rest-frame UV/blue wavelengths) dramatically increases. We determine that roughly two-thirds of the total stellar mass of the Universe today was in place by $z \sim 1$. Double-component galaxies dominate the SMD at all epochs and increase in their contribution to the stellar mass budget to the present day. Elliptical galaxies are the second most dominant morphological type and increase their SMD by $\sim 2.5$ times, while by contrast, the pure-disk population significantly decreases by $\sim 85\%$. According to the evolution of both high- and low-mass ends of the SMF, we find that mergers and in-situ evolution in disks are both present at $z

Original language	English
Pages (from-to)	136-160
Number of pages	25
Journal	Monthly Notices of the Royal Astronomical Society
Volume	505
Issue number	1
DOIs	https://doi.org/10.1093/mnras/stab600
Publication status	Published - 1 Jul 2021

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10.1093/mnras/stab600

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Hashemizadeh, A., Driver, S. P., Davies, L. J. M., Robotham, A. S. G., Bellstedt, S., Windhorst, R. A., Bremer, M., Phillipps, S., Jarvis, M., Holwerda, B. W., Lagos, C. D. P., Koushan, S., Siudek, M., Maddox, N., Thorne, J. E., & Elahi, P. (2021). Deep Extragalactic VIsible Legacy Survey (DEVILS): Stellar Mass Growth by Morphological Type since z=1. Monthly Notices of the Royal Astronomical Society, 505(1), 136-160. https://doi.org/10.1093/mnras/stab600

@article{3232820443234014821722492819e578,

title = "Deep Extragalactic VIsible Legacy Survey (DEVILS): Stellar Mass Growth by Morphological Type since z=1",

abstract = " Using high-resolution Hubble Space Telescope imaging data, we perform a visual morphological classification of $\sim 36,000$ galaxies at $z 1$ as the fraction of irregular galaxies and merger systems (when observed at rest-frame UV/blue wavelengths) dramatically increases. We determine that roughly two-thirds of the total stellar mass of the Universe today was in place by $z \sim 1$. Double-component galaxies dominate the SMD at all epochs and increase in their contribution to the stellar mass budget to the present day. Elliptical galaxies are the second most dominant morphological type and increase their SMD by $\sim 2.5$ times, while by contrast, the pure-disk population significantly decreases by $\sim 85\%$. According to the evolution of both high- and low-mass ends of the SMF, we find that mergers and in-situ evolution in disks are both present at $z ",

keywords = "astro-ph.GA, astro-ph.CO",

author = "Abdolhosein Hashemizadeh and Driver, {Simon P.} and Davies, {Luke J. M.} and Robotham, {Aaron S. G.} and Sabine Bellstedt and Windhorst, {Rogier A.} and Malcolm Bremer and Steven Phillipps and Matt Jarvis and Holwerda, {Benne W.} and Lagos, {Claudia del P.} and Soheil Koushan and Malgorzata Siudek and Natasha Maddox and Thorne, {Jessica E.} and Pascal Elahi",

year = "2021",

month = jul,

day = "1",

doi = "10.1093/mnras/stab600",

language = "English",

volume = "505",

pages = "136--160",

journal = "Monthly Notices of the Royal Astronomical Society",

issn = "0035-8711",

publisher = "Oxford University Press",

number = "1",

}

Hashemizadeh, A, Driver, SP , Davies, LJM , Robotham, ASG , Bellstedt, S, Windhorst, RA, Bremer, M, Phillipps, S, Jarvis, M, Holwerda, BW, Lagos, CDP, Koushan, S, Siudek, M, Maddox, N, Thorne, JE & Elahi, P 2021, 'Deep Extragalactic VIsible Legacy Survey (DEVILS): Stellar Mass Growth by Morphological Type since z=1', Monthly Notices of the Royal Astronomical Society, vol. 505, no. 1, pp. 136-160. https://doi.org/10.1093/mnras/stab600

TY - JOUR

T1 - Deep Extragalactic VIsible Legacy Survey (DEVILS)

T2 - Stellar Mass Growth by Morphological Type since z=1

AU - Hashemizadeh, Abdolhosein

AU - Driver, Simon P.

AU - Davies, Luke J. M.

AU - Robotham, Aaron S. G.

AU - Bellstedt, Sabine

AU - Windhorst, Rogier A.

AU - Bremer, Malcolm

AU - Phillipps, Steven

AU - Jarvis, Matt

AU - Holwerda, Benne W.

AU - Lagos, Claudia del P.

AU - Koushan, Soheil

AU - Siudek, Malgorzata

AU - Maddox, Natasha

AU - Thorne, Jessica E.

AU - Elahi, Pascal

PY - 2021/7/1

Y1 - 2021/7/1

N2 - Using high-resolution Hubble Space Telescope imaging data, we perform a visual morphological classification of $\sim 36,000$ galaxies at $z 1$ as the fraction of irregular galaxies and merger systems (when observed at rest-frame UV/blue wavelengths) dramatically increases. We determine that roughly two-thirds of the total stellar mass of the Universe today was in place by $z \sim 1$. Double-component galaxies dominate the SMD at all epochs and increase in their contribution to the stellar mass budget to the present day. Elliptical galaxies are the second most dominant morphological type and increase their SMD by $\sim 2.5$ times, while by contrast, the pure-disk population significantly decreases by $\sim 85\%$. According to the evolution of both high- and low-mass ends of the SMF, we find that mergers and in-situ evolution in disks are both present at $z

AB - Using high-resolution Hubble Space Telescope imaging data, we perform a visual morphological classification of $\sim 36,000$ galaxies at $z 1$ as the fraction of irregular galaxies and merger systems (when observed at rest-frame UV/blue wavelengths) dramatically increases. We determine that roughly two-thirds of the total stellar mass of the Universe today was in place by $z \sim 1$. Double-component galaxies dominate the SMD at all epochs and increase in their contribution to the stellar mass budget to the present day. Elliptical galaxies are the second most dominant morphological type and increase their SMD by $\sim 2.5$ times, while by contrast, the pure-disk population significantly decreases by $\sim 85\%$. According to the evolution of both high- and low-mass ends of the SMF, we find that mergers and in-situ evolution in disks are both present at $z

KW - astro-ph.GA

KW - astro-ph.CO

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U2 - 10.1093/mnras/stab600

DO - 10.1093/mnras/stab600

M3 - Article

SN - 0035-8711

VL - 505

SP - 136

EP - 160

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

IS - 1

ER -

Deep Extragalactic VIsible Legacy Survey (DEVILS): Stellar Mass Growth by Morphological Type since z=1

Abstract

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Hot Fuzz: The evolution of satellite galaxies via mergers and stripping

How Location Governs Longevity in the Lifecycle of Typical Galaxies

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Deep Extragalactic VIsible Legacy Survey (DEVILS): Stellar Mass Growth by Morphological Type since z=1

Abstract

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Projects

Hot Fuzz: The evolution of satellite galaxies via mergers and stripping

How Location Governs Longevity in the Lifecycle of Typical Galaxies

Cite this