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相关论文: The Absolute Magnitudes of Red Horizontal Branch S…

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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 consider the application of the tip of the red giant branch (TRGB) in the optical and in the near infrared for the determination of distances to nearby galaxies. We analyze ACS VI (F555W & F814W) data and self-consistently…

星系天体物理 · 物理学 2020-09-30 Barry F. Madore , Wendy L. Freedman

In the next years, several cosmological surveys will rely on imaging data to estimate the redshift of galaxies, using traditional filter systems with 4-5 optical broad bands; narrower filters improve the spectral resolution, but strongly…

Galaxy clusters have their unique advantages for cosmology. Here we collect a new sample of 10 lensing galaxy clusters with X-ray observations to constrain cosmological parameters.The redshifts of lensing clusters lie between 0.1 and 0.6,…

宇宙学与河外天体物理 · 物理学 2015-05-20 Heng Yu , Zong-Hong Zhu

We present a BVI optical photometric study of the old open cluster Ruprecht 6 using the data obtained with the SMARTS 1.0 m telescope at the CTIO, Chile. Its color-magnitude diagrams show the clear existence of the main-sequence stars, of…

The relative age of galaxies at different redshifts can be used to infer the Hubble parameter and put constraints on cosmological models. We select 23,883 quiescent luminous red galaxies (LRGs) from the SDSS DR7 and divide them into four…

宇宙学与河外天体物理 · 物理学 2015-06-11 Gaochao Liu , Youjun Lu , Xuelei Chen , Yongheng Zhao , Wei Du , Xianmin Meng

We recently identified a substantial population of galaxies at z>2 with red rest-frame optical colors. These distant red galaxies (DRGs) are efficiently selected by the simple observed color criterion J-K>2.3. In this paper we present NIR…

As one of the most widely recognized high-quality standard stars, the Stetson standards have been extensively used as a photometric reference for calibrating other surveys. In this work, we present an independent validation and…

太阳与恒星天体物理 · 物理学 2026-03-10 Zhirui Li , Bowen Huang , Kai Xiao , Haibo Yuan , Yang Huang , Dongwei Fan , Mingyang Ma , Tao Wang

This study presents the multi-wavelength investigation of the absolute magnitudes and colours of the red clump (RC) stars selected from APOGEE and GALAH DR2 combined catalogue which is complemented with {\it Gaia} DR2 astrometric data and…

星系天体物理 · 物理学 2020-05-20 Olcay Plevne , Özgecan Önal Taş , Selçuk Bilir , George M. Seabroke

We test whether the peak absolute magnitude Mv(TO) of the Globular Cluster Luminosity Function (GCLF) can be used for reliable extragalactic distance determinations. Starting with the luminosity function of the Galactic Globular Clusters…

天体物理学 · 物理学 2009-11-13 M. Di Criscienzo , F. Caputo , M. Marconi , I. Musella

We present a calibration of the Tip of the Red Giant Branch (TRGB) in the Large Magellanic Cloud (LMC) on the HST/ACS F814W system. We use archival HST observations to derive blending corrections and photometric transformations for two…

星系天体物理 · 物理学 2019-11-21 Wenlong Yuan , Adam G. Riess , Lucas M. Macri , Stefano Casertano , Dan Scolnic

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

We present a new formula for absolute magnitude determination for late-type dwarf stars as a function of (g-r) and (r-i) for Sloan photometry. The absolute magnitudes estimated by this approach are brighter than those estimated by…

天体物理学 · 物理学 2009-11-10 S. Bilir , S. Karaali , S. Tuncel

This paper describes the design principles for a CCD-based photometric system that is highly optimized for ground-based measurement of the size of the Balmer jump in stellar energy distributions. It is shown that, among ultraviolet filters…

天体物理学 · 物理学 2009-11-10 Howard E. Bond

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

We present an empirical calibration of the uvby-beta photometric system to determine the intrinsic colours and indices and the astrophysical parameters of the underlying star, valid for Be stars earlier than B5. The procedure allows the…

天体物理学 · 物理学 2007-05-23 Juan Fabregat , Jose M. Torrejon

We isolate samples of 733 bright (g < 18) and 437 faint (g > 18) high-Galactic latitude blue horizontal branch stars with photometry and spectroscopy in the Sloan Digital Sky Survey (SDSS). Comparison of independent photometric and…

We present wide field JHKs photometry of 16 Galactic globular clusters located towards the Galactic bulge, calibrated on the 2MASS photometric system. Differential reddening corrections and statistical field star decontamination are…

太阳与恒星天体物理 · 物理学 2016-11-15 Roger E. Cohen , Christian Moni Bidin , Francesco Mauro , Charles Bonatto , Douglas Geisler

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…

We present new BVI photometry for the halo globular cluster M5, and examine the B- and I-band luminosity functions (LFs), based on over 20,000 stars. We do not see evidence in the LF of a ``subgiant excess'' or of a discrepancy in the…

天体物理学 · 物理学 2009-10-28 Eric L. Sandquist , Michael Bolte , Peter B. Stetson