Zobrazeno 1 - 3
of 3
pro vyhledávání: '"Y. Homayouni"'
Autor:
Karen Kinemuchi, Gordon T. Richards, Eric Morganson, Donald P. Schneider, Linhua Jiang, Patrick B. Hall, Guangtun Zhu, D. A. Starkey, Ian D. McGreer, Paul J. Green, Hengxiao Guo, Eugene A. Magnier, Rolf-Peter Kudritzki, Jonathan R. Trump, Christopher Waters, Yue Shen, K. C. Chambers, Luis C. Ho, Nick Kaiser, Jennifer I-Hsiu Li, Catherine J. Grier, T. Simm, Y. Homayouni, Shu Wang, W. N. Brandt, Patrick Petitjean, Keith Horne
Publikováno v:
Astrophysical Journal Supplement
Astrophysical Journal Supplement, American Astronomical Society, 2019, 241 (2), pp.34. ⟨10.3847/1538-4365/ab074f⟩
Astrophysical Journal Supplement, American Astronomical Society, 2019, 241 (2), pp.34. ⟨10.3847/1538-4365/ab074f⟩
We present a detailed characterization of the 849 broad-line quasars from the Sloan Digital Sky Survey Reverberation Mapping (SDSS-RM) project. Our quasar sample covers a redshift range of 0.1
Comment: Updated to match the accepted version (mino
Comment: Updated to match the accepted version (mino
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e463a186ebc753913c70d7b4a3611565
https://hdl.handle.net/10023/17606
https://hdl.handle.net/10023/17606
Autor:
Shu Wang, Yue Shen, Linhua Jiang, Jennifer I-Hsiu Li, Catherine J. Grier, Donald P. Schneider, Luis C. Ho, Y. Homayouni, Keith Horne, W. N. Brandt, Jonathan R. Trump
The width of the broad emission lines in quasars is commonly characterized either by the full-width-at-half-maximum (FWHM) or the square root of the second moment of the line profile ($\sigma_{\rm line}$), and used as an indicator of the virial veloc
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::25a110a2a801668223596e8074fe44ad
http://arxiv.org/abs/1903.10015
http://arxiv.org/abs/1903.10015
Autor:
Patrick B. Hall, Donald P. Schneider, Luis C. Ho, Y. Homayouni, Yue Shen, Jonathan R. Trump, Jennifer I-Hsiu Li, D. A. Starkey, Keith Horne, W. N. Brandt, Catherine J. Grier
Publikováno v:
The Astrophysical Journal. 884:119
We investigate the performance of different methodologies that measure the time lag between broad-line and continuum variations in reverberation mapping data using simulated light curves that probe a range of cadence, time baseline, and signal-to-noi