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相关论文: Sharpening the Tip of the Red Giant Branch

200 篇论文

The tip of the red giant branch (TRGB) is a well-established standard candle used to measure distances to nearby galaxies. The TRGB luminosity is typically measured in the I-band, where the luminosity has little dependency on stellar age or…

星系天体物理 · 物理学 2019-07-31 Kristen. B. W. McQuinn , Martha Boyer , Evan D. Skillman , Andrew E. Dolphin

We present a new method to measure colors and magnitudes of the tip of the red giant branch in multiple bandpasses simultaneously by fitting an n-dimensional Gaussian to photometry of candidate tip stars. We demonstrate that this method has…

星系天体物理 · 物理学 2020-07-29 M. J. Durbin , R. L. Beaton , J. J. Dalcanton , B. F. Williams , M. L. Boyer

The luminosity of the Tip of the Red Giant Branch (TRGB) provides an excellent measure of galaxy distances and is easily determined in the resolved images of nearby galaxies observed with Hubble Space Telescope. There is now a large amount…

The tip of the red giant (TRGB) is a standardizable candle and is identifiable as the discontinuity at the bright extreme of the red giant branch (RGB) stars in color-magnitude diagram (CMD) space. The TRGB-based distance method has been…

We present an extensive grid of numerical simulations quantifying the uncertainties in measurements of the Tip of the Red Giant Branch (TRGB). These simulations incorporate a luminosity function composed of 2 magnitudes of red giant branch…

太阳与恒星天体物理 · 物理学 2023-06-14 Barry F. Madore , Wendy L. Freedman Kayla A. Owens , In Sung Jang

We examine the reliability of the tip of the red giant branch (TRGB) as a distance indicator for stellar populations with different star formation histories (SFHs) when photometric errors and completeness corrections at the TRGB are small.…

天体物理学 · 物理学 2009-11-10 Michael K. Barker , Ata Sarajedini , Jason Harris

The tip of the red giant branch (TRGB) provides a key standard candle for extragalactic distance measurements and for refining the Hubble constant. We test its robustness by quantifying how metallicity, $\alpha$-element enhancement, age,…

We present the I-band luminosity function of the red giant branch stars in the Large Magellanic Cloud (LMC) using the data from the Magellanic Clouds Photometric Survey (Zaritsky, Harris & Thompson, 1997). Selecting stars in uncrowded,…

天体物理学 · 物理学 2009-10-31 Shoko Sakai , Dennis Zaritsky , Robert Kennicutt

The tip of the red giant branch (TRGB) is an important standard candle for determining luminosity distances. Although several $10^5$ small amplitude red giant stars (SARGs) have been discovered, variability was previously considered…

宇宙学与河外天体物理 · 物理学 2024-03-05 Richard I. Anderson , Nolan W. Koblischke , Laurent Eyer

We present a precise determination of the apparent magnitude of the tip of the red giant branch (TRGB) in the I (0.8 micron), J (1.25 micron), and K_S (2.15 micron) bands from the luminosity function of a sample of data extracted from the…

天体物理学 · 物理学 2007-05-23 Maria-Rosa. L. Cioni , Roeland P. van der Marel , Cecile Loup , Harm J. Habing

The tip of the red giant branch (TRGB) is a standard candle that can be used to help refine the determination of the Hubble constant. $Gaia$ Data Release 3 (DR3) provides synthetic photometry constructed from low-resolution BP/RP spectra…

星系天体物理 · 物理学 2023-07-26 Siyang Li , Stefano Casertano , Adam G. Riess

This study introduces an automated approach for identifying the tip of the red giant branch (TRGB) in globular clusters, combining astronomical data with algorithmic methods. Using a dataset of 160 globular clusters and Python scripts, we…

太阳与恒星天体物理 · 物理学 2026-02-27 Yi Yang , Zhenzhen Shao , Xiaofeng Wang , Xiaochen Zheng

The Tip of the Red Giant (TRGB) method provides one of the most accurate and precise means of measuring the distances to nearby galaxies. Here we present a VIJHK absolute calibration of the TRGB based on observations of TRGB stars in the…

The Tip of the Red Giant Branch (TRGB) is an apparent discontinuity in the color-magnitude diagram (CMD) along the giant branch due to the end of the red giant evolutionary phase and is used to measure distances in the local universe. In…

宇宙学与河外天体物理 · 物理学 2024-05-06 J. Wu , D. Scolnic , A. G. Riess , G. S. Anand , R. Beaton , S. Casertano , X. Ke , S. Li

Accurate distances to galaxies can be determined from the luminosities of stars at the Tip of the Red Giant Branch (TRGB). We use a Maximum Likelihood algorithm to locate the TRGB in galaxy color-magnitude diagrams. The algorithm is…

The luminosity of the Tip of the Red Giant Branch (TRGB) is instrumental for the construction of the distance ladder, and its accurate modelling is key for determining the local Hubble parameter. In this work, we present an extensive…

太阳与恒星天体物理 · 物理学 2022-06-22 Ippocratis D. Saltas , Emanuele Tognelli

In this paper JK_s data from the VISTA Magellanic Cloud (VMC) survey are used to investigate the tip of the red giant branch (TRGB) as a distance indicator. A linear fit to recent theoretical models is used which reads M_{K_s} = -4.196…

太阳与恒星天体物理 · 物理学 2019-01-30 M. A. T. Groenewegen , M. -R. L. Cioni , L. Girardi , R. de Grijs , V. D. Ivanov , M. Marconi , T. Muraveva , V. Ripepi , J. Th. van Loon

We use the latest parallaxes measurements from Gaia DR3 to obtain a geometric calibration of the tip of the red giant branch (TRGB) in Cousins $I$ magnitudes as a standard candle for cosmology. We utilise the following surveys: SkyMapper…

星系天体物理 · 物理学 2023-05-24 M. Dixon , J. Mould , C. Flynn , E. N. Taylor , C. Lidman , A. R. Duffy

We present the ultimate I-band calibration of the tip of the red giant branch (TRGB) standard candle. Our calibration is based on photometry from the outer parts of the Large Magellanic Cloud, 2.75<r<6.5 degs from the center, collected…

The absolute bolometric luminosity of the point of core Helium ignition in old, metal poor, red-giant stars is of roughly constant magnitude, varying only very slightly with mass or metallicity. It can thus be used as a standard candle.…

天体物理学 · 物理学 2009-11-10 A. W. McConnachie , M. J. Irwin , A. M. N. Ferguson , R. A. Ibata , G. F. Lewis , N. Tanvir
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