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Table 2

The sample of ATLAS3D ETGs with a Spitzer-IRS class.

Galaxy Morpho. T P λ re/ 2 ϵ re/ 2 V/σre/ 2 FR/SRre/2 n tot MIR
RSA class class
NGC 821 E6 –4.8±0.4 cuspy 0.27 0.39 0.29 FR 10.4±0.7 0
NGC 2685 S03(7) pec –1.0±0.8 cuspy 0.63 0.19 0.73 FR 4.3±0.4 2
NGC 2974 E4 –4.2±1.2 cuspy 0.66 0.40 0.81 FR 4.0±0.4 2
NGC 3193 E2 –4.8±0.5 core 0.20 0.14 0.21 FR 5.3±0.1 0
NGC 3245 S01 –2.1±0.5 cuspy 0.59 0.44 0.58 FR 3.2±1.9 3
NGC 3377 E6 –4.8±0.4 cuspy 0.52 0.50 0.56 FR 5.0±0.5 0
NGC 3379 E0 –4.8±0.5 core 0.16 0.10 0.15 FR 5.3±0.9 0
NGC 3608 E1 –4.8±0.5 core 0.04 0.19 0.05 SR 3.9±0.5 0
NGC 4036 S03(8)/Sa –2.6±0.7 ... 0.68 0.54 0.80 FR 2.0±0.1 2
NGC 4261 E3 –4.8±0.4 core 0.09 0.22 0.09 SR 5.1±0.4 4
NGC 4339 S01/2(0) –4.7±0.8 cuspy 0.31 0.06 0.30 FR 4.1±0.6 0
NGC 4365 E3 –4.8±0.5 core 0.09 0.25 0.11 SR 5.2±0.4 0
NGC 4371 SB02/3(r)(3) –1.3±0.6 cuspy 0.48 0.31 0.54 FR 3.8±0.6 2
NGC 4374 E1 –4.3±1.2 core 0.02 0.15 0.03 SR 6.0±0.3 2
NGC 4377 S01(3) –2.6±0.6 cuspy 0.34 0.23 0.31 FR 2.2±1.2 0
NGC 4382 S01(3) pec –1.3±0.6 core 0.16 0.20 0.17 FR 5.1±1.3 1
NGC 4435 SB01(7) –2.1±0.5 ... 0.60 0.46 0.67 FR 4.7±0.3 3
NGC 4442 SB01(6) –1.9±0.4 cuspy 0.34 0.31 0.33 FR 2.8±0.2 0
NGC 4472 E1/S01(1) –4.8±0.5 core 0.08 0.17 0.07 SR 4.7±0.1 1
NGC 4473 E5 –4.7±0.7 core 0.25 0.40 0.26 FR 5.7±0.5 0
NGC 4474 S01(8) –2.0±0.5 cuspy 0.35 0.47 0.35 FR 3.5±0.4 2
NGC 4477 SB01/2/SBa –1.9±0.4 cuspy 0.22 0.13 0.21 FR 4.1±1.2 2
NGC 4478 E2 –4.8±0.4 core 0.18 0.17 0.17 FR 2.0±0.1 0
NGC 4486 E0 –4.3±0.6 core 0.02 0.04 0.02 SR 2.9±0.2 4
NGC 4550 E7/S01(7) –2.1±0.7 cuspy 0.06 0.63 0.07 SR 1.7±0.1 3
NGC 4552 S01(0) –4.6±0.9 core 0.05 0.05 0.05 SR 6.2±0.4 2
NGC 4564 E6 –4.8±0.5 cuspy 0.54 0.48 0.53 FR 2.9±0.2 0
NGC 4570 S01(7)/E7 –2.0±0.7 cuspy 0.50 0.55 0.47 FR 2.4±0.2 0
NGC 4621 E5 –4.8±0.5 cuspy 0.29 0.36 0.27 FR 4.3±0.2 0
NGC 4636 E0/S01(6) –4.8±0.5 core 0.04 0.09 0.04 SR 5.5±0.5 2
NGC 4649 S01(2) –4.6±0.8 core 0.13 0.16 0.12 FR 5.1±0.5 1
NGC 4660 E5 –4.7±0.5 cuspy 0.47 0.32 0.52 FR 3.5±0.2 0
NGC 4697 E6 –4.4±0.8 cuspy 0.47 0.32 0.36 FR 4.6±0.2 3
NGC 5273 S0/a –1.9±0.4 cuspy 0.48 0.12 0.51 FR 1.8±1.1 4
NGC 5353 S01(7)/E7 –2.1±0.6 ... 0.53 0.54 0.54 FR 3.3±0.5 2
NGC 5631 S03(2)/Sa –1.9±0.4 ... 0.17 0.17 0.19 FR 4.3±0.5 2
NGC 5638 E1 –4.8±0.4 ... 0.23 0.08 0.22 FR 3.5±0.2 0
NGC 5813 E1 –4.8±0.4 core 0.07 0.17 0.16 SR 5.8±1.7 1
NGC 5831 E4 –4.8±0.5 cuspy 0.06 0.20 0.16 SR 4.3±0.2 0
NGC 5846 S01(0) –4.7±0.7 core 0.03 0.06 0.04 SR 3.9±0.2 1
NGC 7332 S02/3 –1.9±0.5 cuspy 0.34 0.44 0.29 FR 2.3±0.4 1
NGC 1339 E4 –4.3±0.5 cuspy ... ... ... ... ... 0
NGC 1351 S01(6)/E6 –3.1±0.6 core ... ... ... ... ... 0
NGC 1374 E0 –4.4±1.1 core ... ... ... ... ... 0
NGC 1389 S01(5)/SB01 –2.8±0.7 cuspy ... ... ... ... ... 0
NGC 1399 E1 –4.6±0.5 core ... ... ... ... ... 0
NGC 1404 E2 –4.8±0.5 core ... ... ... ... ... 1
NGC 1427 E5 –4.0±0.9 core ... ... ... ... ... 0
IC 2006 E1 –4.2±0.9 cuspy ... ... ... ... ... 1

Notes. ETGs in ATLAS3D (top part of the table), including the Virgo sample, plus Fornax cluster ETGs (Turner et al. 2012) represent the global sample used for the core vs. cuspy and FR vs. SR analyses. Morphological classifications in Cols. 2 and 3 are from RSA and LEDA, respectively. For the ATLAS3D sample, the profile type (Col. 4), P, is cuspy (originally \ = power law, ∧ = intermediate) and core (originally ∩) is taken from Krajnović et al. (2013b). The specific angular momentum (Col. 5), λre/ 2; the ellipticity (Col. 6), ϵe/ 2; the rotation velocity to velocity dispersion ratio (Col. 7), V/σre/ 2; and the kinematical class (Col. 8), FR/SR, at re/2 are from Emsellem et al. (2011). The Sersic index (Col. 9), ntot, is from Krajnović et al. (2013a). The MIR class (Col. 10) is taken from Rampazzo et al. (2013).

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