Write in a clean editor, then format for The Astrophysical Journal in one click — DocuGuru applies the official American Astronomical Society template with author–year references and exports a submission-ready PDF plus the editable LaTeX source. Free to start.
The Astrophysical Journal is a peer-reviewed journal published by American Astronomical Society, covering Stellar, planetary, and galactic studies, Astronomy and Astrophysical Research, Astrophysics and Star Formation Studies. Over its lifetime it has published 133,882 papers, which have received 7,508,001 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, 12, 45
Formats any DOI in The Astrophysical Journal style. No sign-up. |
| Publishes research in | Stellar, planetary, and galactic studies Astronomy and Astrophysical Research Astrophysics and Star Formation Studies Galaxies: Formation, Evolution, Phenomena Astrophysical Phenomena and Observations |
| ISSN | 0004-637X |
| Citation impact (2-yr) | 5.11 |
| h-index | 699 |
| i10-index | 97,041 |
| Article processing charge | $4,499 |
| Open access | Yes — indexed in DOAJ |
| Top institutions publishing here | Center for Astrophysics Harvard & Smithsonian |
| Journal website | iopscience.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.
We report measurements of the mass density, ΩM, and cosmological-constant energy density, ΩΛ of the universe based on the analysis of 42 type Ia supernovae discovered by the Supernova Cosmology Project. The magnitude-redshift data for these supernovae, at redshifts between 0.18 and 0.83, are fitted jointly with a set of supernovae from the Calán/Tololo Supernova…
We present a full-sky 100 km map that is a reprocessed composite of the COBE/DIRBE and IRAS/ ISSA maps, with the zodiacal foreground and conrmed point sources removed. Before using the ISSA maps, we remove the remaining artifacts from the IRAS scan pattern. Using the DIRBE 100 and 240 km data, we have constructed a…
The parameterized extinction data of Fitzpatrick and Massa (1986, 1988) for the ultraviolet and various sources for the optical and near-infrared are used to derive a meaningful average extinction law over the 3.5 micron to 0.125 wavelength range which is applicable to both diffuse and dense regions of the interstellar medium. The law depends on…
We use high-resolution N-body simulations to study the equilibrium density profiles of dark matter halos in hierarchically clustering universes. We find that all such profiles have the same shape, independent of halo mass, of initial density fluctuation spectrum, and of the values of the cosmological parameters. Spherically averaged equilibrium profiles are well fit over two…
The evolutionary significance of the observed luminosity function for main-sequence stars in the solar neighborhood is discussed. The hypothesis is made that stars move off the main sequence after burning about 10 per cent of their hydrogen mass and that stars have been created at a uniform rate in the solar neighborhood for the last…
