The Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST, also called the Guo Shou Jing Telescope) is a special reflecting Schmidt telescope. LAMOST's special design allows both a large aperture (effective aperture of 3.6 m-4.9 m) and a wide field of view (FOV) (5 degrees). It has an innovative active reflecting Schmidt configuration which continuously…
Research in Astronomy and Astrophysics Template
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About the Research in Astronomy and Astrophysics format
Research in Astronomy and Astrophysics is a peer-reviewed journal published by IOP Publishing, covering Stellar, planetary, and galactic studies, Astronomy and Astrophysical Research, Astrophysics and Star Formation Studies.
| Publisher | IOP Publishing |
|---|---|
| Reference style | Numbered (IOP) Numbered — [1], [2] in the text [1] Smith A, Jones B and Lee C 2023 A representative article title Research in Astronomy and Astrophysics 12 45–58
Formats any DOI in Research in Astronomy and Astrophysics style. No sign-up. |
| Publishes research in | Stellar, planetary, and galactic studies Astronomy and Astrophysical Research Astrophysics and Star Formation Studies Gamma-ray bursts and supernovae Galaxies: Formation, Evolution, Phenomena |
| ISSN | 1674-4527 |
| Citation impact (2-yr) | 1.52 |
| h-index | 63 |
| i10-index | 820 |
| Total citations | 36,532 |
| Top institutions publishing here | Chinese Academy of Sciences |
| Journal website | iopscience.iop.org |
| You get | A submission-ready PDF and the editable LaTeX source — ready to submit. |
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Most-cited papers in Research in Astronomy and Astrophysics
LAMOST (Large sky Area Multi-Object fiber Spectroscopic Telescope) is a Chinese national scientific research facility operated by National Astronomical Observatories, Chinese Academy of Sciences (NAOC). After two years of commissioning beginning in 2009, the telescope, instruments, software systems and operations are nearly ready to begin the main science survey. Through a spectral survey of millions…
Abstract Observing and timing a group of millisecond pulsars with high rotational stability enables the direct detection of gravitational waves (GWs). The GW signals can be identified from the spatial correlations encoded in the times-of-arrival of widely spaced pulsar-pairs. The Chinese Pulsar Timing Array (CPTA) is a collaboration aiming at the direct GW detection with…
By adopting the differential age method, we utilize selected 17832 luminous red galaxies (LRGs) from Sloan Digital Sky Survey Data Release Seven (SDSS DR7) covering redshift $0<z<0.4$ to measure Hubble parameters. Using a full spectrum fitting package UlySS, these spectra are reduced with single stellar population (SSP) models and optimal age information of our selected…
The Large sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) general survey is a spectroscopic survey that will eventually cover approximately half of the celestial sphere and collect 10 million spectra of stars, galaxies and QSOs. Objects in both the pilot survey and the first year regular survey are included in the LAMOST DR1. The pilot…