SMARTS Optical/IR Observations
of LAT Monitored Blazars

1406-076 Historical Data

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Information | Spectral Energy Distribution | Lightcurves | Spectra

1406-076 Information

• Coordinates: α= 14:08:56.4811, δ= -07:52:26.665 (2000), z= 1.494
• Classification: FSRQ

1406-076 Spectral Energy Distribution

X-ray Spectral Energy Distribution The black line is a single-zone synchrotron inverse Compton model using the input parameters referenced in the paper. XMM-Newton data are indicated with black filled symbols, the remaining symbols and lines are archival data. Foschini, L. et al., 2006, A&A, 453, 824-828

1406-076 Lightcurves

Radio Light Curve (37 Ghz) Lahteenmaki, A. and Valtoaja, E., 2003, ApJ, 590,95-108

Optical Light Curve Wagner, S.J. et al., 1995, ApJL, 454, 97-100

Optical and Gamma Ray Light Curve Wagner, S.J. et al., 1995, ApJL, 454, 97-100

Gamma Ray Light Curve Instrument: EGRET Nandikotkur, G. et al., 2007, ApJ, 657 ,706-724

Gamma Ray Light Curve Gamma-ray light curve in the energy range 70MeV < E < 10 GeV during January 1993. Instrument: EGRET Mukherjee, R. et al., 1997, ApJ, 490, 116-135

Gamma Ray Light Curve Wagner, S.J. et al., 1995, ApJL, 454, 97-100

1406-076 Spectra

Gamma Spectra (37 Ghz) Gamma-ray spectrum in the EGRET energy range. Wagner, S.J. et. al., 1995, ApJL, 454, 97-100

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