Shang-Shan Chong

ORCID: 0000-0003-3366-0403
Publications
Citations
Views
---
Saved
---
About
Contact & Profiles
Research Areas
  • Advanced Statistical Methods and Models
  • Spectroscopy and Chemometric Analyses
  • Galaxies: Formation, Evolution, Phenomena
  • NMR spectroscopy and applications
  • Astronomy and Astrophysical Research
  • Statistical Methods and Applications
  • Gamma-ray bursts and supernovae
  • Material Dynamics and Properties
  • Theoretical and Computational Physics
  • Impact of Light on Environment and Health
  • Advanced Thermodynamics and Statistical Mechanics
  • Clay minerals and soil interactions
  • Astronomical Observations and Instrumentation
  • Fractal and DNA sequence analysis
  • Stellar, planetary, and galactic studies
  • Zeolite Catalysis and Synthesis
  • Remote Sensing in Agriculture

Carnegie Mellon University
2003-2006

National Energy Technology Laboratory
2005

We present a catalog of 100,563 unresolved, UV-excess (UVX) quasar candidates to g=21 from 2099 deg^2 the Sloan Digital Sky Survey (SDSS) Data Release One (DR1) imaging data. Existing spectra 22,737 sources reveals that 22,191 (97.6%) are quasars; accounting for magnitude dependence this efficiency, we estimate 95,502 (95.0%) objects in quasars. Such high efficiency is unprecedented broad-band surveys This ``proof-of-concept'' sample designed be maximally efficient, but still has 94.7% completeness g

10.1086/425356 article EN The Astrophysical Journal Supplement Series 2004-12-01

Abstract We investigated the evolution of fractions late-type cluster galaxies as a function redshift using one largest, most uniform samples available. The sample consisted 514 clusters in range $0.02 \leq z\leq 0.3$ from Sloan Digital Sky Survey “Cut and Enhance” galaxy catalog. This catalog was created single automated cluster-finding algorithm applied to data telescope, with accurate CCD photometry, thus minimizing selection biases. used four independent methods analyze fraction....

10.1093/pasj/55.4.739 article EN Publications of the Astronomical Society of Japan 2003-08-25

I present here a review of past and multi-disciplinary research the Pittsburgh Computational AstroStatistics (PiCA) group. This group is dedicated to developing fast efficient statistical algorithms for analysing huge astronomical data sources. begin with short multi-resolutional kd-trees which are building blocks many our algorithms. For example, quick range queries n-point correlation functions. will new results from use Mixture Models (Connolly et al. 2000) in density estimation...

10.48550/arxiv.astro-ph/0110230 preprint EN other-oa arXiv (Cornell University) 2001-01-01
Coming Soon ...