xGASS: The impact of photometric bulges on the scatter of HI scaling relations

Robin H. W. Cook; Luca Cortese; Barbara Catinella; Aaron Robotham

doi:10.1093/mnras/stz2789

xGASS: The impact of photometric bulges on the scatter of HI scaling relations

Robin H. W. Cook, Luca Cortese, Barbara Catinella, Aaron Robotham

Research output: Contribution to journal › Article › peer-review

15 Citations (Web of Science)

Abstract

We present a structural decomposition analysis of the galaxies in the extended GALEX Arecibo SDSS Survey (xGASS) using (gri) images from the Sloan Digital Sky Survey. Utilizing the 2D Bayesian light profile fitting code ProFit, we fit single- and double-component models taking advantage of a robust Markov chain Monte Carlo optimization algorithm in which we assume a Sersic profile for single-component models and a combination of a Sersic bulge and near-exponential disc (0.5

Original language	English
Pages (from-to)	4060-4079
Number of pages	20
Journal	Monthly Notices of the Royal Astronomical Society
Volume	490
Issue number	3
DOIs	https://doi.org/10.1093/mnras/stz2789
Publication status	Published - Dec 2019

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10.1093/mnras/stz2789Licence: Other

Data from: xGASS: The impact of photometric bulges on the scatter of HI scaling relations
Cook, R. (Creator), Cortese, L. (Creator), Catinella, B. (Creator) & Robotham, A. (Creator), SAO/NASA Astrophysics Data System (ADS), Dec 2019
https://ui.adsabs.harvard.edu/abs/2019MNRAS.490.4060C/abstract and one more link, https://ui.adsabs.harvard.edu/link_gateway/2019MNRAS.490.4060C/SIMBAD (show fewer)
Dataset

2 Active

Beyond Appearance: revealing the physics of galaxy transformation
Cortese, L.
Australian Research Council
1/10/18 → 30/09/22
Project: Research
ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions
Kewley, L., Wyithe, S., Sadler, E., Staveley-Smith, L., Glazebrook, K., Jackson, C., Bland-Hawthorn, J., Asplund, M., Power, C. & Driver, S.
Australian Research Council
1/01/17 → 31/12/23
Project: Research

Cite this

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title = "xGASS: The impact of photometric bulges on the scatter of HI scaling relations",

abstract = "We present a structural decomposition analysis of the galaxies in the extended GALEX Arecibo SDSS Survey (xGASS) using (gri) images from the Sloan Digital Sky Survey. Utilizing the 2D Bayesian light profile fitting code ProFit, we fit single- and double-component models taking advantage of a robust Markov chain Monte Carlo optimization algorithm in which we assume a Sersic profile for single-component models and a combination of a Sersic bulge and near-exponential disc (0.5",

keywords = "galaxies: evolution, galaxies: ISM, galaxies: structure, EARLY-TYPE GALAXIES, DIGITAL SKY SURVEY, ARECIBO SDSS SURVEY, STAR-FORMING GALAXIES, ATOMIC GAS FRACTIONS, STELLAR MASS, ATLAS(3D) PROJECT, PHYSICAL-PROPERTIES, BLACK-HOLES, MORPHOLOGICAL CLASSIFICATIONS",

author = "Cook, {Robin H. W.} and Luca Cortese and Barbara Catinella and Aaron Robotham",

year = "2019",

month = dec,

doi = "10.1093/mnras/stz2789",

language = "English",

volume = "490",

pages = "4060--4079",

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

issn = "0035-8711",

publisher = "Oxford University Press",

number = "3",

}

TY - JOUR

T1 - xGASS

T2 - The impact of photometric bulges on the scatter of HI scaling relations

AU - Cook, Robin H. W.

AU - Cortese, Luca

AU - Catinella, Barbara

AU - Robotham, Aaron

PY - 2019/12

Y1 - 2019/12

N2 - We present a structural decomposition analysis of the galaxies in the extended GALEX Arecibo SDSS Survey (xGASS) using (gri) images from the Sloan Digital Sky Survey. Utilizing the 2D Bayesian light profile fitting code ProFit, we fit single- and double-component models taking advantage of a robust Markov chain Monte Carlo optimization algorithm in which we assume a Sersic profile for single-component models and a combination of a Sersic bulge and near-exponential disc (0.5

AB - We present a structural decomposition analysis of the galaxies in the extended GALEX Arecibo SDSS Survey (xGASS) using (gri) images from the Sloan Digital Sky Survey. Utilizing the 2D Bayesian light profile fitting code ProFit, we fit single- and double-component models taking advantage of a robust Markov chain Monte Carlo optimization algorithm in which we assume a Sersic profile for single-component models and a combination of a Sersic bulge and near-exponential disc (0.5

KW - galaxies: evolution

KW - galaxies: ISM

KW - galaxies: structure

KW - EARLY-TYPE GALAXIES

KW - DIGITAL SKY SURVEY

KW - ARECIBO SDSS SURVEY

KW - STAR-FORMING GALAXIES

KW - ATOMIC GAS FRACTIONS

KW - STELLAR MASS

KW - ATLAS(3D) PROJECT

KW - PHYSICAL-PROPERTIES

KW - BLACK-HOLES

KW - MORPHOLOGICAL CLASSIFICATIONS

U2 - 10.1093/mnras/stz2789

DO - 10.1093/mnras/stz2789

M3 - Article

VL - 490

SP - 4060

EP - 4079

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

SN - 0035-8711

IS - 3

ER -

xGASS: The impact of photometric bulges on the scatter of HI scaling relations

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Datasets

Data from: xGASS: The impact of photometric bulges on the scatter of HI scaling relations

Projects

Beyond Appearance: revealing the physics of galaxy transformation

ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions

Cite this