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Megan E. Eckart

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high-z type 2 quasar candidates. SED's of spectroscopically ID'd sources. 3. SEXSI Survey ... Many BLAGN fit a typical quasar SED (Elvis et al. 1994) ... – PowerPoint PPT presentation

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Title: Megan E. Eckart


1
The SEXSI Survey Recent Progress
  • Megan E. Eckart
  • Caltech
  • with Fiona Harrison, David Helfand, Daniel
    Stern, Luke Kotredes

2
Overview
  • 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

3
SEXSI 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)
4
SEXSI Survey
Harrison et al. 2003, ApJ, 596, 944-956 (Paper 1)
5
Redshift 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)
6
Fraction 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)
7
Spitzer 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)
8
High-z QSO 2
- quadrant split from Martinez-Sansigre, Lacy et
al. (2005)
9
High-z QSO 2
- quadrant split from Martinez-Sansigre, Lacy et
al. (2005)
10
BLAGN 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)

11
NLAGN SEDs
  • Bad match to both templates
  • (would match an absorbedAGN spectrum )
  • Fits star forming template in IR

12
ELG SEDs
  • Overwhelming majority (but not all) of ELG fit
    starforming template

13
In 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

14
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