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Multiwavelength Monitoring of TeV Blazars

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Bright stars in FOV and galaxy nearby to target make analysis of thermal band data tricky. ... use of 7 comparison stars (statistics issues?) MRK 421 PAIRITEL ... – PowerPoint PPT presentation

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Title: Multiwavelength Monitoring of TeV Blazars


1
Multiwavelength Monitoring of TeV Blazars
  • Andy Smith
  • Smithsonian Astrophysical Observatory
  • (Whipple 10m Telescope)

2
X-Ray
Gamma Ray
Whipple 10m
RXTE All Sky Monitor
350 GeV -gt 10 TeV
2-gt10keV
IR
I
OPTICAL
PAIRITEL
FLWO 48in
3
Catalog of TeV AGN c. 2005
4
Wondering Why?
  • Previous MW campaigns show strong correlation
    between emission variability across bands
  • Understanding HE emission from AGN requires
    understanding of jet ejection events- need MW
    data to trace evolution and constrain models with
    improved SED
  • Previous campaigns have been limited by time-
    current Whipple campaign is longest HE monitoring
    campaign to date- also utilizes instruments with
    close proximity

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AGN Jet Emission Mechanisms
  • Electron Progenitors
  • Synchrotron Self Compton
  • External Compton
  • Proton Progenitors
  • Proton Cascades
  • Proton Synchrotron

Electron Synchrotron Self Compton Models most
consistent with TeV AGN-but observations are
complex and require more sophisticated modeling
of jets. Need MW data to model accretion/ejection
phenomena.
7
MRK421 SED from previous MW
SYNCHROTRON
COMPTON
COMPTON
Similar double peaked Power Spectra seen in other
AGN
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MRK 421 PAIRITEL DATA
  • Bright stars in FOV and galaxy nearby to target
    make analysis of thermal band data tricky......
  • Performed night to night photometry in J,H,K
    bands for 34 nights (Dec-gt May)
  • FOV issues only allowed use of 7 comparison
    stars (statistics issues?)

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PRELIMINARY Courtesy of D. Horan
14
Courtesy of ASM/RXTE team
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Results
  • Similar trend in variability seen in all H, J, K
    bands. Inconclusive as to whether this
    variability is linked to HE flaring events.
  • Need further IR (analyzed optical data) in
    between and during flares to determine
    correlation between low energy emission and
    flaring events.

19
To Be Continued....
  • Will continue to monitor blazars with Whipple and
    FLWO 48in next season, as well as RXTE (ToO with
    SWIFT), hopefully PAIRITEL also?
  • Upcoming VERITAS array will join in next spring
    (100 GeV -gt 50TeV)
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