Updated Hubble constant from TRGB measurements

In summary: The Hubble Constant is the distance between the galaxies in the cluster.The Hubble Constant has been changing over time, and this new preprint shows that it has been changing a lot.
  • #1
Madeleine Birchfield
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Scolnic et al have put out a new preprint with an updated value for the Hubble constant as measured from the Tip of the Red Giant Branch:

https://arxiv.org/abs/2304.06693
 
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  • #2

CATS: The Hubble Constant from Standardized TRGB and Type Ia Supernova Measurements​

D. Scolnic, A. G. Riess, J. Wu, S. Li, G. S. Anand, R. Beaton, S. Casertano, R. Anderson, S. Dhawan, X. Ke
The Tip of the Red Giant Branch (TRGB) provides a luminous standard candle for constructing distance ladders to measure the Hubble constant. In practice its measurements via edge-detection response (EDR) are complicated by the apparent fuzziness of the tip and the multi-peak landscape of the EDR. As a result, it can be difficult to replicate due to a case-by-case measurement process.

Previously we optimized an unsupervised algorithm, Comparative Analysis of TRGBs (CATs), to minimize the variance among multiple halo fields per host without reliance on individualized choices, achieving state-of-the-art ∼ < 0.05 mag distance measures for optimal data.

Further, we found an empirical correlation at 5σ confidence in the GHOSTS halo survey between our measurements of the tip and their contrast ratios (ratio of stars 0.5 mag just below and above the tip), useful for standardizing the apparent tips at different host locations.

Here, we apply this algorithm to an expanded sample of SN Ia hosts to standardize these to multiple fields in the geometric anchor, NGC 4258.

In concert with the Pantheon+ SN Ia sample, this analysis produces a (baseline) result of H0=73.22±2.06 km/s/Mpc. The largest difference in H0 between this and similar studies employing the TRGB derives from corrections for SN survey differences and local flows used in most recent SN Ia compilations but which were absent in earlier studies. SN-related differences total ∼ 2.0 km/s/Mpc. A smaller share, ∼ 1.4 km/s/Mpc, results from the inhomogeneity of the TRGB calibration across the distance ladder.

We employ a grid of 108 variants around the optimal TRGB algorithm and find the median of variants is 72.94±1.98 km/s/Mpc with an additional uncertainty due to algorithm choices of 0.83 km/s/Mpc. None of these TRGB variants result in H0 less than 71.6 km/s/Mpc.
Comments:Submitted to ApJL, comments welcome
 
  • #3
That's quite a bit northwards of previous TRGB determinations:
1683752081302.png

(Freedman et al. 2019; fig.17)
 
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  • #5
pinball1970 said:
Not sure I get why there would be more than one image separated by time.
The light from the supernova follows different paths around the lensing galaxy cluster. Some paths are longer than others, so it takes correspondingly more or less time. Imagine a light beam going straight to you, and another making a detour - it'd normally leave the source in a direction unaligned with the observer, but the gravity well bends its path so that it turns around towards you. The turning around takes some time, so to speak.
 
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FAQ: Updated Hubble constant from TRGB measurements

What is the Hubble constant?

The Hubble constant (H₀) is a measure of the rate at which the universe is expanding. It is usually expressed in kilometers per second per megaparsec (km/s/Mpc), indicating how fast galaxies are moving away from us per unit distance.

What are TRGB measurements?

TRGB stands for the Tip of the Red Giant Branch. It is a method used in astronomy to determine distances to galaxies. This technique involves identifying the point at which red giant stars reach the end of their stable phase and undergo a helium flash, which can be used as a standard candle to measure distances accurately.

Why are TRGB measurements important for determining the Hubble constant?

TRGB measurements are important because they provide an independent method for determining distances to galaxies, which is crucial for calculating the Hubble constant. By using TRGB, astronomers can reduce uncertainties and cross-check results obtained from other distance measurement methods like Cepheid variables.

How do TRGB measurements compare to other methods for determining the Hubble constant?

TRGB measurements are considered to be more precise and less affected by certain types of systematic errors compared to other methods like Cepheid variables. However, different methods have yielded slightly different values for the Hubble constant, contributing to the ongoing debate known as the "Hubble tension."

What is the current value of the Hubble constant from TRGB measurements?

The current value of the Hubble constant from TRGB measurements is approximately 69.8 km/s/Mpc. This value is slightly lower than those obtained from other methods, such as measurements using Cepheid variables and supernovae, which tend to be around 73-74 km/s/Mpc.

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