Yonsei Evolutionary Population Synthesis (YEPS) Model. III. Surface Brightness Fluctuation of Normal and Helium-enhanced Simple Stellar Populations [PDF]
Astrophysical Journal Supplement Series, 2020 We present an evolutionary population synthesis model of the surface brightness fluctuation (SBF) for normal and He-enriched simple stellar populations (SSPs).
C. Chung +4 more
semanticscholar +1 more source
Anomalous surface brightness fluctuations in NGC 4489 [PDF]
Astronomy & Astrophysics, 2001 Anomalously high K-band surface brightness fluctuations (SBF) have been reported in NGC 4489 by Pahre & Mould (1994), Jensen et al. (1996) and Jensen et al. (1998). However, these conclusions were uncertain because of relatively low signal-to-noise data. New high signal-to-noise data for NGC 4489 have been obtained at the NOAO/KPNO 2.1m and the ESO/
Mei, S., Silva, D. R., Quinn, P. J.
openaire +2 more sources
A Dynamic Threshold Cloud Detecting Approach based on the Brightness Temperature from FY-2 VISSR Data [PDF]
The International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences, 2015 The traditional statistical methods and radiation transfer theory methods for cloud detecting have a high adaptability just only in those areas with a uniform surface coverage and noncomplex terrain.
X. Daxiang +3 more
doaj +1 more source
矿业科学学报, 2023 When the surface strain field of concrete structure is measured by digital image correlation(DIC)technology under complex light conditions, the decorrelation effect of the pattern will be caused by the variation in light intensity.
Yang Denghui +5 more
doaj +1 more source
The Next Generation Virgo Cluster Survey (NGVS). XVIII. Measurement and Calibration of Surface Brightness Fluctuation Distances for Bright Galaxies in Virgo (and Beyond) [PDF]
, 2018 We describe a program to measure surface brightness fluctuation (SBF) distances to galaxies observed in the Next Generation Virgo Cluster Survey (NGVS), a photometric imaging survey covering 104 deg2 of the Virgo cluster in the u*, g, i, and z bandpasses
M. Cantiello +9 more
semanticscholar +1 more source
An I-band calibration of surface brightness fluctuation measurements at blue colours
Astronomy and Astrophysics, 2006 S. Mieske, M. Hilker, L. Infante
semanticscholar +3 more sources
Measuring Distances to Low-luminosity Galaxies Using Surface Brightness Fluctuations [PDF]
The Astrophysical Journal, 2021 Abstract We present an in-depth study of surface brightness fluctuations (SBFs) in low-luminosity stellar systems. Using the MIST models, we compute theoretical predictions for absolute SBF magnitudes in the LSST, HST ACS/WFC, and proposed Roman Space Telescope filter systems.
Johnny P. Greco +4 more
openaire +2 more sources
MEASURING INFRARED SURFACE BRIGHTNESS FLUCTUATION DISTANCES WITH HST WFC3: CALIBRATION AND ADVICE [PDF]
, 2015 We present new calibrations of the near-infrared (near-IR) surface brightness fluctuation (SBF) distance method for the F110W ( J 110 ?> ) and F160W ( H 160 ?> ) bandpasses of the Wide Field Camera 3 Infrared Channel (WFC3/IR) on the Hubble Space ...
J. Jensen +7 more
semanticscholar +1 more source
Surface Brightness Fluctuations as Stellar Population Indicators [PDF]
AIP Conference Proceedings, 2009 8 pages, Invited review presented at "Probing Stellar Populations out to the Distant Universe," September 2008, Cefalu ...
John P. Blakeslee +7 more
openaire +2 more sources