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The Astrophysical Journal Supplement Series is a peer-reviewed journal published by American Astronomical Society, covering Stellar, planetary, and galactic studies, Astronomy and Astrophysical Research, Galaxies: Formation, Evolution, Phenomena. Over its lifetime it has published 8,381 papers, which have received 790,742 citations.
| Publisher | American Astronomical Society |
|---|---|
| Reference style | Author–year (AAS) Author–year — (Smith, 2023) in the text Smith, A., Jones, B., & Lee, C. 2023, The Astrophysical Journal Supplement Series, 12, 45
Formats any DOI in The Astrophysical Journal Supplement Series style. No sign-up. |
| Publishes research in | Stellar, planetary, and galactic studies Astronomy and Astrophysical Research Galaxies: Formation, Evolution, Phenomena Astrophysics and Star Formation Studies Gamma-ray bursts and supernovae |
| ISSN | 0067-0049 |
| Citation impact (2-yr) | 5.39 |
| h-index | 378 |
| i10-index | 6,131 |
| Article processing charge | $4,499 |
| Open access | Yes — indexed in DOAJ |
| Top institutions publishing here | California Institute of Technology |
| Journal website | iopscience.iop.org |
| You get | A submission-ready PDF and the editable LaTeX source — ready to submit. |
Citations each year’s papers have accumulated so far — the most recent years are still building up.
WMAP precision data enables accurate testing of cosmological models. We find that the emerging standard model of cosmology, a flat Lambda-dominated universe seeded by nearly scale-invariant adiabatic Gaussian fluctuations, fits the WMAP data. With parameters fixed only by WMAP data, we can fit finer scale CMB measurements and measurements of large scle structure (galaxy surveys…
(Abridged) The 7-year WMAP data and improved astrophysical data rigorously test the standard cosmological model and its extensions. By combining WMAP with the latest distance measurements from BAO and H0 measurement, we determine the parameters of the simplest LCDM model. The power-law index of the primordial power spectrum is n_s=0.968+-0.012, a measurement that excludes the…
A simple cosmological model with only six parameters (matter density,mh 2, baryon density,bh 2, Hubble con-stant, H0, amplitude of fluctuations, 8, optical depth, , and a slope for the scalar perturbation spectrum, ns) fits not only the 3 yearWMAP temperature and polarization data, but also small-scale CMB data, light element abundances, large-scale structure observations, and…
(Abridged) The WMAP 5-year data strongly limit deviations from the minimal LCDM model. We constrain the physics of inflation via Gaussianity, adiabaticity, the power spectrum shape, gravitational waves, and spatial curvature. We also constrain the properties of dark energy, parity-violation, and neutrinos. We detect no convincing deviations from the minimal model. The parameters of the…
This paper describes the Seventh Data Release of the Sloan Digital Sky Survey (SDSS), marking the completion of the original goals of the SDSS and the end of the phase known as SDSS-II. It includes 11,663 deg2 of imaging data, with most of the ~2000 deg2 increment over the previous data release lying in regions…
