Measuring the Growth Rate of Structure with Type IA Supernovae from LSST
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We investigate the peculiar motions of galaxies up to z = 0.5 using Type Ia supernovae (SNe Ia) from the Large Synoptic Survey Telescope (LSST) and predict the subsequent constraints on the growth rate of structure. We consider two cases. Our first is based on measurements of the volumetric SNe Ia rate and assumes we can obtain spectroscopic redshifts and light curves for varying fractions of objects that are detected pre-peak luminosity by LSST (some of which may be obtained by LSST itself, and others that would require additional follow-up observations). We find that these measurements could produce growth rate constraints at that significantly outperform those found using Redshift Space Distortions (RSD) with DESI or 4MOST, even though there are fewer objects. For our second case, we use semi-analytic simulations and a prescription for the SNe Ia rate as a function of stellar mass and star-formation rate to predict the number of LSST SNe IA whose host redshifts may already have been obtained with the Taipan+WALLABY surveys or with a future multi-object spectroscopic survey. We find ∼18,000 and ∼160,000 SNe Ia with host redshifts for these cases, respectively. While this is only a fraction of the total LSST-detected SNe Ia, they could be used to significantly augment and improve the growth rate constraints compared to only RSD. Ultimately, we find that combining LSST SNe Ia with large numbers of galaxy redshifts will provide the most powerful probe of large-scale gravity in the regime over the coming decades.
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This SN sample can be used as a tracer of large-scale structure through peculiar velocities, weak lensing of SN brightnesses, local bulk flow, and low-redshift isotropy constraints.
“This sample of SNe can be used as a tracer of large-scale structure by directly probing the gravitational potential of structure through inferences of their peculiar velocities ( Gordon et al. 2007; Bhattacharya et al. 2011; Howlett et al. 2017 ) , WL of SN brightnesses ( Dodelson & Vallinotto 2006; Quartin et al. 2014; Macaulay et al. 2017; Scovacricchi et al. 2017 ) , and the local bulk fl”
From LSST: From Science Drivers to Reference Design and Anticipated Data Products (2019) · cites this paper as Howlett et al. 2017
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First Constraints on the Intrinsic CMB Dipole and Our Velocity with Doppler and Aberration
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Peculiar-velocity cosmology with Types Ia and II supernovae
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Target selection for the DESI Peculiar Velocity Survey
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Self-citationThe redshift-space momentum power spectrum – I. Optimal estimation from peculiar velocity surveys
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Probing gravity and growth of structure with gravitational waves and galaxies’ peculiar velocity
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Self-citationComplementarity of peculiar velocity surveys and redshift space distortions for testing gravity
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Self-citationGrowth-rate measurement with type-Ia supernovae using ZTF survey simulations
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Measuring the Hubble function with standard candle clustering
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Exploring the redshift-space peculiar velocity field and its power spectrum
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The observed number counts in luminosity distance space
Fonseca, J., Zazzera, S., Baker, T., & Clarkson, C. (2023) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2023/08/050 · Cited by 17 · see citing works
Testing Cosmic Opacity with the Combination of Strongly Lensed and Unlensed Supernova Ia
Ma, Y.-B., Cao, S., Zhang, J., Qi, J., Liu, T., Liu, Y., & Geng, S. (2019) · The Astrophysical Journal · doi:10.3847/1538-4357/ab50c4 · Cited by 17 · see citing works
TiDES: The 4MOST Time Domain Extragalactic Survey
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On the amount of peculiar velocity field information in supernovae from LSST and beyond
Garcia, K., Quartin, M., & Siffert, B. B. (2020) · Physics of the Dark Universe · doi:10.1016/j.dark.2020.100519 · Cited by 16 · see citing works
The lure of sirens: joint distance and velocity measurements with third-generation detectors
Alfradique, V., Quartin, M., Amendola, L., Castro, T., & Toubiana, A. (2022) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stac2920 · Cited by 15 · see citing works
The La Silla Schmidt Southern Survey
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The 6 × 2pt method: supernova velocities meet multiple tracers
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Subpercent accurate fitting of modified gravity growth
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The large-scale environment of thermonuclear and core-collapse supernovae
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Cosmological parameters estimated from peculiar velocity–density comparisons: calibrating 2M++
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On the cosmological performance of photometrically classified supernovae with machine learning
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Using peculiar velocity surveys to constrain neutrino masses
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Self-citationForecast for a growth-rate measurement using peculiar velocities from LSST supernovae
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Self-citationConstraining modified gravity scenarios with the 6dFGS and SDSS galaxy peculiar velocity data sets
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Testing modified gravity scenarios with direct peculiar velocities
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Magnification and evolution bias of transient sources: GWs and SNIa
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Large-scale peculiar velocities in the universe
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Cross-correlating radial peculiar velocities and CMB lensing convergence
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On the correlations of galaxy peculiar velocities and their covariance
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Can a multi-tracer approach improve the constraints on the turnover scale at low redshift?
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Cosmic curl — features and convergence of the vorticity power spectrum in N-body simulations
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Joint curvature and growth rate measurements with supernova peculiar velocities and the CMB
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- Authors
- Howlett, C., Robotham, A. S. G., Lagos, C. D. P., & Kim, A. G.
- Affiliations
- The University of Western Australia (AU)
- Lawrence Berkeley National Laboratory (US)
- Corresponding author
- Howlett, Cullan
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 2017-09-29
- Volume
- 847
- Issue
- 2
- Pages
- 128
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W2751272724
- Cited by
- 59
- References
- 61
- Citations by year
- 2026: 5 · 2025: 7 · 2024: 5 · 2023: 7 · 2022: 9 · 2021: 9 · 2020: 5 · 2019: 6 · 2018: 2 · 2017: 1 · 2016: 3
- FWCI
- 2.09
- Type
- journal article
- Language
- en
- Open access
- bronze
- doi.org
- Licence
- Locations
- The Astrophysical Journal (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- UWA Profiles and Research Repository (UWA) (submittedVersion)
- arXiv (Cornell University)
- Funders
- National Aeronautics and Space Administration
- ARC Centre of Excellence for All-Sky Astrophysics (CE110001020)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Gamma-ray bursts and supernovae
- Keywords
- structure growth, Type Ia supernovae, LSST, redshift-space distortions, large-scale structure, cosmological constraints, DESI, 4MOST
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