4.7 Article

REVERBERATION MAPPING OF THE SEYFERT 1 GALAXY NGC7469

期刊

ASTROPHYSICAL JOURNAL
卷 795, 期 2, 页码 -

出版社

IOP PUBLISHING LTD
DOI: 10.1088/0004-637X/795/2/149

关键词

galaxies: active; galaxies: individual (NGC 7469); galaxies: nuclei; galaxies: Seyfert

资金

  1. National Science Foundation [AST-1008882]
  2. NSF through CAREER [AST-1253702]
  3. NSF through award [AST-1302093]
  4. Marie Curie Actions of the European Union's Seventh Framework Programme under REA grant [300553]
  5. NSF Fellowships
  6. NSF grants
  7. Kitzman Fellowship
  8. Israel-Niedersachsen collaboration program
  9. Zeff Fellowship
  10. Target Scientific Research Complex Programme of the National Academy of Sciences of Ukraine
  11. Russian Foundation of Research (RFBR) [12-02-01237-a]
  12. CrAO CCD through US Civilian Research and Development [UP1-2116, UP1-2549-CR-03.]
  13. Ministry of Education, Science, Culture and Sports of Japan. [17104002, 20041003, 21018003, 21018005, 22253002, 22540247]
  14. [AST-1009756]
  15. Division Of Astronomical Sciences
  16. Direct For Mathematical & Physical Scien [1008882] Funding Source: National Science Foundation
  17. Division Of Astronomical Sciences
  18. Direct For Mathematical & Physical Scien [1009756, 1253702, 1302093] Funding Source: National Science Foundation
  19. Grants-in-Aid for Scientific Research [22540247, 21018005, 24103003] Funding Source: KAKEN
  20. STFC [ST/J001651/1] Funding Source: UKRI
  21. Science and Technology Facilities Council [ST/J001651/1] Funding Source: researchfish

向作者/读者索取更多资源

A large reverberation-mapping study of the Seyfert 1 galaxy NGC7469 has yielded emission-line lags for H beta lambda 4861 and He He II lambda 4686 and a central black hole mass measurement M-BH approximate to 1 x 10(7)M(circle dot) , consistent with previous measurements. A very low level of variability during the monitoring campaign precluded meeting our original goal of recovering velocity-delay maps from the data, but with the new H beta measurement, NGC7469 is no longer an outlier in the relationship between the size of the H beta-emitting broad-line region and the luminosity of the active galactic nucleus. It was necessary to detrend the continuum and H beta and He He II lambda 4686 line light curves and those from archival UV data for different time-series analysis methods to yield consistent results.

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