Sign on

SAO/NASA ADS Astronomy Abstract Service


· Find Similar Abstracts (with default settings below)
· Also-Read Articles (Reads History)
·
· Translate This Page
Title:
Spitzer 3.6 and 5.8 micron Monitoring of the Seyfert 1 NGC 4051
Authors:
Gorjian, Varoujan; Adkins, J.; Borders, K.; Kelly, S.; Martin, C.; Mendez, B.; Paradis, J.; Perreira, V.; Pittman, P.; Sepulveda, B.; NGC 4051 Monitoring Group
Affiliation:
AA(Spitzer Science Center/JPL/Caltech), AB(Spitzer/WISE/RBSE), AC(Spitzer/WISE/RBSE), AD(Spitzer/WISE/RBSE), AE(Spitzer/WISE/RBSE), AF(Space Sciences Laboratory), AG(Spitzer/WISE/RBSE), AH(Spitzer/WISE/RBSE), AI(Spitzer/WISE/RBSE), AJ(Spitzer/WISE/RBSE), AK()
Publication:
American Astronomical Society, AAS Meeting #213, #420.06; Bulletin of the American Astronomical Society, Vol. 41, p.236
Publication Date:
01/2009
Origin:
AAS
Bibliographic Code:
2009AAS...21342006G

Abstract

We used the Spitzer Space Telescope Infrared Array Camera (IRAC) to monitor the Seyfert 1 active galactic nucleus NGC 4051. We took data at 3.6 and 5.8 microns every day for 10 days in June 2008. We also observed in the optical at B, V, and R bands starting a month before the IRAC observations with various ground based observatories, though we were unable to achieve daily coverage. We will present the IR and optical light curves and will search for correlated variability that may be evidence of dust reverberation. For the education and public outreach component of this program please see Sepulveda et al.
Bibtex entry for this abstract   Preferred format for this abstract (see Preferences)

   

Find Similar Abstracts:

Use: Authors
Title
Abstract Text
Return: Query Results Return    items starting with number
Query Form
Database: Astronomy
Physics
arXiv e-prints