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Table 5.

Physical parameters inferred from the optical spectra of the ILRTs sample.

Date MJD Phase (a) v (Hα) (b) L (Hα) (c) LHα/L[Ca II] (c) TBB
(d) (km s−1) (1038erg s−1) (K)
AT 2010dn

20100602 55349.9 −5.0 695 2.12 2.9 7095 ± 355
20100603 55350.9 −4.0 671 1.85 2.6 6890 ± 240
20100604 55351.9 −3.0 588 3.47 2.5 6540 ± 330
20100605 55352.9 −2.0 6435 ± 320
20100607 55354.9 +0.0 577 2.29 2.6 6760 ± 340
20100609 55356.9 +2.0 < 823 2.63 2.5 6830 ± 340
20100611 55358.9 +4.0 563 1.86 2.3 6690 ± 195
20100616 55363.9 +9.0 442 2.12 2.2 6820 ± 320
20100617 55364.9 +10.0 438 1.81 2.1 6710 ± 280
20100707 55384.9 +30.0 < 142 0.58 1.8 5020 ± 250

AT 2012jc

20120329 56015.1 −8.4 < 1097 5.30 8380 ± 420
20120331 56017.3 −6.2 614 5.30 15.4 7385 ± 740
20120414 56031.2 +7.7 < 960 5.27 10.2 7995 ± 205
20120501 56048.3 +24.8 < 617 2.97 5.5 6780 ± 340
20120623 56101.2 +77.7 842 2.36 5445 ± 525

AT 2013lb

20130207 56330.1 +5.6 < 640 3.33 6865 ± 685
20130207 56330.4 +5.9 < 777 3.36 13.4 6450 ± 645
20130207 56330.4 +5.9 < 460 3.29 6250 ± 315
20130209 56332.3 +7.8 < 1006 5850 ± 585
20130219 56343.3 +18.8 < 1006 2.29 8.2 6390 ± 640
20130304 56356.3 +31.8 < 617 1.87 4.8 6450 ± 325
20130422 56404.3 +79.8 680 2.33 4375 ± 220

AT 2013la (d)

20140108 56665.2 +13.2 < 640 6.31 5880 ± 295
20140115 56672.2 +20.2 < 457 5.92 7110 ± 1420
20140203 56692.2 +40.2 778 6050 ± 1210
20140205 56694.2 +42.2 < 709 5.33 5345 ± 270
20140228 56717.2 +65.2 400 4.99 5290 ± 265
20140322 56739.1 +87.1 < 480 5.04 6005 ± 1200
20140716 56854.9 +202.9 446 3.98 5055 ± 255
20140814 56883.9 +231.9 503 3.87 4285 ± 225
20141220 57012.3 +360.3 499 2.68 4485 ± 180

AT 2018aes

20180331 58208.1 −3.0 708 0.85 2.7 6620 ± 330
20180426 58234.1 +23.0 609 0.77 2.2 5675 ± 285

Notes.

(a)

Phases are relative to the R/r-band light curve peaks.

(b)

Most of our measurements are limited by the instrumental resolution constraints, hence the FWHM velocities may have large error bars, and in many cases they should be regarded as upper limits.

(c)

We adopt conservative errors of ∼20% for the Hα luminosity and the LHα/L[Ca II] ratio because of the uncertainty in the flux calibration of the spectra.

(d)Hα has a complex profile in AT 2013la, and was therefore fitted with multiple components. The narrowest Gaussian emission and absorption components are usually below the instrumental resolution limit. For this reason, only the FWHM velocities of the broader Lorentzian components are reported here.

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