Peculiar-velocity cosmology with Types Ia and II supernovae

Author:

Stahl Benjamin E12ORCID,de Jaeger Thomas31,Boruah Supranta S4,Zheng WeiKang1,Filippenko Alexei V15,Hudson Michael J678ORCID

Affiliation:

1. Department of Astronomy, University of California, Berkeley, CA 94720-3411, USA

2. Department of Physics, University of California, Berkeley, CA 94720-7300, USA

3. Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822, USA

4. Steward Observatory, University of Arizona, Tucson, AZ 85719, USA

5. Miller Institute for Basic Research in Science, University of California, Berkeley, CA 94720, USA

6. Department of Physics and Astronomy, University of Waterloo, Waterloo, ON N2L 3G1, Canada

7. Waterloo Centre for Astrophysics, University of Waterloo, Waterloo, ON N2L 3G1, Canada

8. Perimeter Institute for Theoretical Physics, Waterloo, ON N2L 2Y5, Canada

Abstract

Abstract We present the Democratic Samples of Supernovae (DSS), a compilation of 775 low-redshift Type Ia and II supernovae (SNe Ia & II), of which 137 SN Ia distances are derived via the newly developed snapshot distance method. Using the objects in the DSS as tracers of the peculiar-velocity field, we compare against the corresponding reconstruction from the 2M++ galaxy redshift survey. Our analysis — which takes special care to properly weight each DSS subcatalogue and cross-calibrate the relative distance scales between them — results in a measurement of the cosmological parameter combination $f\sigma _8 = 0.390_{-0.022}^{+0.022}$ as well as an external bulk flow velocity of $195_{-23}^{+22}$ km s−1 in the direction $(\ell , b) = (292_{-7}^{+7}, -6_{-4}^{+5})$ deg, which originates from beyond the 2M++ reconstruction. Similarly, we find a bulk flow of $245_{-31}^{+32}$ km s−1 toward $(\ell , b) = (294_{-7}^{+7}, 3_{-5}^{+6})$ deg on a scale of ∼30 h−1 Mpc if we ignore the reconstructed peculiar-velocity field altogether. Our constraint on fσ8 — the tightest derived from SNe to date (considering only statistical error bars), and the only one to utilise SNe II — is broadly consistent with other results from the literature. We intend for our data accumulation and treatment techniques to become the prototype for future studies that will exploit the unprecedented data volume from upcoming wide-field surveys.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 23 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

同舟云学术

1.学者识别学者识别

2.学术分析学术分析

3.人才评估人才评估

"同舟云学术"是以全球学者为主线,采集、加工和组织学术论文而形成的新型学术文献查询和分析系统,可以对全球学者进行文献检索和人才价值评估。用户可以通过关注某些学科领域的顶尖人物而持续追踪该领域的学科进展和研究前沿。经过近期的数据扩容,当前同舟云学术共收录了国内外主流学术期刊6万余种,收集的期刊论文及会议论文总量共计约1.5亿篇,并以每天添加12000余篇中外论文的速度递增。我们也可以为用户提供个性化、定制化的学者数据。欢迎来电咨询!咨询电话:010-8811{复制后删除}0370

www.globalauthorid.com

TOP

Copyright © 2019-2024 北京同舟云网络信息技术有限公司
京公网安备11010802033243号  京ICP备18003416号-3