The 3XMM/SDSS Stripe 82 Galaxy Cluster Survey – II. X-ray and optical properties of the cluster sample

doi:10.1093/mnras/stz1097

This content will become publicly available on April 17, 2020

Title: The 3XMM/SDSS Stripe 82 Galaxy Cluster Survey – II. X-ray and optical properties of the cluster sample

Full Record
Other Related Research

Authors:

Takey, Ali ^[1]; Durret, Florence ^[2]; Márquez, Isabel ^[3]; Ellien, Amael ^[2]; Molham, Mona ^[1]; Plat, Adèle ^[2]

National Research Institute of Astronomy and Geophysics (NRIAG), 11421 Helwan, Cairo, Egypt
Sorbonne Universités, UPMC Univ. Paris 6 et CNRS, UMR 7095, Institut d’Astrophysique de Paris (IAP), 98bis Bd Arago, F-75014 Paris, France
Instituto de Astrofísica de Andalucía (IAA-CSIC), E-18008 Granada, Spain

Publication Date:: 2019-04-17

Sponsoring Org.:: USDOE

OSTI Identifier:: 1512316

Resource Type:: Published Article

Journal Name:: Monthly Notices of the Royal Astronomical Society

Additional Journal Information:: Journal Name: Monthly Notices of the Royal Astronomical Society Journal Volume: 486 Journal Issue: 4; Journal ID: ISSN 0035-8711

Publisher:: Oxford University Press

Country of Publication:: United Kingdom

Language:: English

Citation Formats


                    Takey, Ali, Durret, Florence, Márquez, Isabel, Ellien, Amael, Molham, Mona, and Plat, Adèle. The 3XMM/SDSS Stripe 82 Galaxy Cluster Survey – II. X-ray and optical properties of the cluster sample.  United Kingdom: N. p., 2019. 
        Web.  doi:10.1093/mnras/stz1097.

Copy to clipboard


                    Takey, Ali, Durret, Florence, Márquez, Isabel, Ellien, Amael, Molham, Mona, & Plat, Adèle. The 3XMM/SDSS Stripe 82 Galaxy Cluster Survey – II. X-ray and optical properties of the cluster sample.  United Kingdom.  doi:10.1093/mnras/stz1097.

Copy to clipboard


                    Takey, Ali, Durret, Florence, Márquez, Isabel, Ellien, Amael, Molham, Mona, and Plat, Adèle. Wed .  
        "The 3XMM/SDSS Stripe 82 Galaxy Cluster Survey – II. X-ray and optical properties of the cluster sample".  United Kingdom.  doi:10.1093/mnras/stz1097.

Copy to clipboard


                    
@article{osti_1512316,

  title        = {The 3XMM/SDSS Stripe 82 Galaxy Cluster Survey – II. X-ray and optical properties of the cluster sample},

  author       = {Takey, Ali and Durret, Florence and Márquez, Isabel and Ellien, Amael and Molham, Mona and Plat, Adèle},

  abstractNote = {},

  doi          = {10.1093/mnras/stz1097},

  journal      = {Monthly Notices of the Royal Astronomical Society},

  number       = 4,

  volume       = 486,

  place        = {United Kingdom},

  year         = {2019},

  month        = {4}

}

Copy to clipboard

Journal Article:

Free Publicly Available Full Text

This content will become publicly available on April 17, 2020

Publisher's Version of Record

DOI: 10.1093/mnras/stz1097

Other availability

Search WorldCat to find libraries that may hold this journal

Save / Share:

Export Metadata

Save to My Library

Similar Records in DOE PAGES and OSTI.GOV collections:

Spectral clustering for optical confirmation and redshift estimation of X-ray selected galaxy cluster candidates in the SDSS Stripe 82

Journal Article Mahmoud, E. ; Takey, A. ; Shoukry, A. - Astronomy and Computing
Cited by 1
DOI: 10.1016/j.ascom.2016.07.001
SDSS-II Supernova survey. An analysis of the largest sample of type IA supernovae and correlations with host-galaxy spectral properties

Journal Article Wolf, Rachel C. ; D’Andrea, Chris B. ; Gupta, Ravi R. ; ... - The Astrophysical Journal (Online)

Using the largest single-survey sample of Type Ia supernovae (SNe Ia) to date, we study the relationship between properties of SNe Ia and those of their host galaxies, focusing primarily on correlations with Hubble residuals (HR). Our sample consists of 345 photometrically-classified or spectroscopicallyconfirmed SNe Ia discovered as part of the SDSS-II Supernova Survey (SDSS-SNS). This analysis utilizes host-galaxy spectroscopy obtained during the SDSS-I/II spectroscopic survey and from an ancillary program on the SDSS-III Baryon Oscillation Spectroscopic Survey (BOSS) that obtained spectra for nearly all host galaxies of SDSS-II SN candidates. In addition, we use photometric hostgalaxy properties from themore »« less
DOI: 10.3847/0004-637X/821/2/115
SDSS-II SUPERNOVA SURVEY: AN ANALYSIS OF THE LARGEST SAMPLE OF TYPE IA SUPERNOVAE AND CORRELATIONS WITH HOST-GALAXY SPECTRAL PROPERTIES

Journal Article Wolf, Rachel C. ; Gupta, Ravi R. ; Sako, Masao ; ... - Astrophysical Journal

Using the largest single-survey sample of Type Ia supernovae (SNe Ia) to date, we study the relationship between properties of SNe Ia and those of their host galaxies, focusing primarily on correlations with Hubble residuals (HRs). Our sample consists of 345 photometrically classified or spectroscopically confirmed SNe Ia discovered as part of the SDSS-II Supernova Survey (SDSS-SNS). This analysis utilizes host-galaxy spectroscopy obtained during the SDSS-I/II spectroscopic survey and from an ancillary program on the SDSS-III Baryon Oscillation Spectroscopic Survey that obtained spectra for nearly all host galaxies of SDSS-II SN candidates. In addition, we use photometric host-galaxy properties frommore »« less
DOI: 10.3847/0004-637X/821/2/115
Weak-lensing mass calibration of the Atacama Cosmology Telescope equatorial Sunyaev-Zeldovich cluster sample with the Canada-France-Hawaii telescope stripe 82 survey

Journal Article Battaglia, N. ; Miyatake, H. ; Hasselfield, M. ; ... - Journal of Cosmology and Astroparticle Physics

Mass calibration uncertainty is the largest systematic effect for using clusters of galaxies to constrain cosmological parameters. We present weak lensing mass measurements from the Canada-France-Hawaii Telescope Stripe 82 Survey for galaxy clusters selected through their high signal-to-noise thermal Sunyaev-Zeldovich (tSZ) signal measured with the Atacama Cosmology Telescope (ACT). For a sample of 9 ACT clusters with a tSZ signal-to-noise greater than five the average weak lensing mass is (4.8±0.8) ×10{sup 14} M{sub ⊙}, consistent with the tSZ mass estimate of (4.70±1.0) ×10{sup 14} M{sub ⊙} which assumes a universal pressure profile for the cluster gas. Our results are consistentmore »« less
DOI: 10.1088/1475-7516/2016/08/013
H I CONTENT AND OPTICAL PROPERTIES OF FIELD GALAXIES FROM THE ALFALFA SURVEY. II. MULTIVARIATE ANALYSIS OF A GALAXY SAMPLE IN LOW-DENSITY ENVIRONMENTS

Journal Article Toribio, M. Carmen ; Solanes, Jose M. ; Giovanelli, Riccardo ; ... - Astrophysical Journal

This is the second paper of two reporting results from a study of the H I content and stellar properties of nearby galaxies detected by the Arecibo Legacy Fast ALFA blind 21 cm line survey and the Sloan Digital Sky Survey in a 2160 deg{sup 2} region of high galactic latitude sky covered by both surveys, in the general Virgo direction. Here, we analyze a complete H I flux-limited subset of 1624 objects with homogeneously measured 21 cm and multi-wavelength optical attributes extracted from the control sample of H I emitters in environments of low local galactic density assembled bymore »« less
DOI: 10.1088/0004-637X/732/2/93

Similar Records