Title: Megan E. Eckart
1The SEXSI Survey Recent Progress
- Megan E. Eckart
- Caltech
- with Fiona Harrison, David Helfand, Daniel
Stern, Luke Kotredes -
2Overview
- Introduction to the SEXSI sample and optical
followup - Highlights of the optical/X-ray sample
composition - Spitzer data
- high-z type 2 quasar candidates
- SEDs of spectroscopically IDd sources
3SEXSI Survey
- Study dominant contributors to XRB
- 1034 2-10 keVsources from 27 Chandra
pointings (2 deg2) - R-band imaging
- 438 spectroscopic redshifts from Keck
Harrison et al. 2003, ApJ, 596, 944-956 (Paper 1)
4SEXSI Survey
Harrison et al. 2003, ApJ, 596, 944-956 (Paper 1)
5Redshift Distribution
- Peak z 0.7
- 34 narrow-lined Lxgt1044 sources(type-2 quasar
candidates) - nine z gt 2, obscured type-2 quasar candidates
Eckart et al. 2006, ApJS, 165, 19-56 (Paper 3)
6Fraction Obscured
- SEXSI - excellent statistics over flux range
- 50 obscuredindependent of luminosity
Fraction with log(NH) gt 22
log (Unobscured 2-10 keV Luminosity erg s-1)
Eckart et al. 2006, ApJS, 165, 19-56 (Paper 3)
7Spitzer Data
- Spitzer data over five SEXSI fields (IRAC
MIPS) - 250 SEXSI X-ray sources covered
- 140 with spectroscopic ID
- 62 of total X-ray sources are in wedge
- 86 of BLAGN
- 67 of NLAGN
- 28 of ELG
- 15 of sources with Lxlt10 43.5 erg s-1
- wedge from Stern et al. (2005)
8High-z QSO 2
- quadrant split from Martinez-Sansigre, Lacy et
al. (2005)
9High-z QSO 2
- quadrant split from Martinez-Sansigre, Lacy et
al. (2005)
10BLAGN SEDs
- Many BLAGN fit a typical quasar SED (Elvis et
al. 1994) - BUT, there are many that fit a star forming
template better in mid-IR/optical (Devriendt et
al. 1999 template plotted above)
11NLAGN SEDs
- Bad match to both templates
- (would match an absorbedAGN spectrum )
- Fits star forming template in IR
12ELG SEDs
- Overwhelming majority (but not all) of ELG fit
starforming template
13In Progress
- Synthesis of spectrally identified and
unidentified SEDs - X-ray stacking of Spitzer sources
- with Chandra nondetections
- Acknowledgements Fiona Harrison, David Helfand,
Dan Stern, Luke Kotredes
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