Table 4
Flare NIR spectral measurements.
References | Dates | Instruments | Bands | αa |
|
||||
[1] ............... | 2009 Apr. 3 | VLT/NACO | 2.1, 3.8 μm | −0.4 ± 0.3 |
[2] ............... | 2005 Jul. 16, 31, 2006 May 2, Jul. 17 | Keck/NIRC2 | 1.6, 2.1, 3.8, 4.7 μm | −0.6 ± 0.2 |
[3] ............... | 2007 Apr. 2, 5 | HST/NICMOS | 1.45, 1.7 μm | −0.7 ± 0.2, −1 ± 0.3 |
[4, 5] .......... | 2007 Apr. 4 | VLT/NACO, VISIR | 3.8, 11.8 μm | > –1 |
[6] ............... | 2005 Apr. 29 | Keck/OSIRIS | 2.02–2.38 μm | −2.6 ± 0.9 |
[7] ............... | 2005 Jun. 18 | VLT/SINFONI | 2–2.45 μm | −(0.6–1.3) ± 0.2 |
[8] ............... | 2004 Jul. 15, 17 | VLT/SINFONI | 1.7–2.45 μm | −4 ± 1 |
[9] ............... | 2004 Jul. 26 | Keck/NIRC2 | 2.1, 3.8 μm | −0.5 ± 0.3 |
Notes.
α is defined by Fν ∝ ν α; indicates when there is a correlation observed between the flux and the spectral index. In the case of Yusef-Zadeh et al. (2009), only the brightest flares are reported.
References. [1] This work, [2] Hornstein et al. (2007), [3] Yusef-Zadeh et al. (2009), [4] Dodds-Eden et al. (2009), [5] Trap et al. (2010), [6] Krabbe et al. (2006), [7] Gillessen et al. (2006), [8] Eisenhauer et al. (2005), [9] Ghez et al. (2005).
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