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Table B.1.

DUSTY results for the Miras in the DEATHSTAR sample for which distances were derived using our new PL relation.

Source P dust* T⋆ Tdust τ10 rPL(M)
[days] [K] [K] [L⊙] [L⊙] [L⊙] [pc] [pc] [pc]
C-type
AFGL 3068 696 AMC 2500 800 1.2 11890 1013 1108 1220 60 70
AI Vol 511 AMC 2500 1300 0.28 7897 525 563 730 60 50
CL Mon 493 AMC 3100 1300 0.05 7532 485 518 910 30 40
CZ Hya 442 AMC 2500 1200 0.09 6518 376 399 1470 60 70
HV Cas 527 AMC 3100 1300 0.09 8226 563 604 1320 70 80
IRAS 15194-5115 576 AMC 3000 1200 0.36 9254 683 738 670 40 40
IRC+10216 630 AMC 3100 1300 0.5 10420 826 897 190 20 20
IRC+60041 280 AMC 2500 1300 0.07 3561 104 107 640 50 60
LP And 614 AMC 2500 1300 3 10071 783 849 1760 120 100
PQ Cep 442 AMC 2500 1300 0.04 6517 376 399 1080 80 130
R For 386 AMC 2500 1300 0.06 5447 268 282 650 50 50
R Lep 445 AMC 3300 1100 0.02 6576 382 405 380 20 10
R Vol 453 AMC 2500 1300 0.13 5076 233 244 840 60 50
RV Aqr 453 AMC 3100 1300 0.1 6733 398 423 600 30 30
RZ Peg 437 AMC 2700 900 0.01 6420 365 388 1380 70 80
S Cep 484 AMC 3100 1300 0.03 7350 465 496 390 20 20
T Dra 422 AMC 2500 1300 0.07 6134 337 356 670 50 30
U Cyg 463 AMC 3000 800 0.02 6930 419 446 870 50 60
V CrB 358 AMC 3100 1300 0.02 4930 220 230 640 20 30
V Cyg 421 AMC 2500 1200 0.07 6116 335 354 420 10 20
V358 Lup 632 AMC 2500 1300 0.75 10464 831 903 1050 60 60
V384 Per 535 AMC 3100 1200 0.12 8393 582 626 700 30 30
V688 Mon 1770 AMC 2900 1000 0.34 40914 5699 6622 3370 250 260
V821 Her 524 AMC 2500 1300 0.2 8165 556 597 700 61 50
V1259 Ori 696 AMC 2500 1300 0.75 11890 1013 1108 1550 90 90
V1426 Cyg 470 AMC 2500 1300 0.07 7070 435 463 600 40 20
V1968 Cyg 395 AMC 2600 1300 0.55 5625 286 301 990 80 100
S-type
GI Lup 469 AMC 2600 900 0.01 7050 432 461 1190 70 80
IRC−10401 480 AMS 2600 600 5 7270 456 487 3470 120 110
NSV 24833 418 AMS 2400 900 4 6053 328 347 3500 120 140
R And 409 AMS 3400 600 0.06 5885 312 329 390 30 20
R Cyg 427 AMS 2600 600 0.03 6226 346 366 560 40 30
R Gem 370 AMC 3200 1300 0.03 5151 241 252 1000 30 30
R Lyn 366 AMC 3200 1300 0.03 5076 233 244 1300 40 50
RT Sco 449 AMS 2600 1200 0.3 6655 391 415 710 60 60
S Cas 608 AMS 3000 1000 0.7 9946 767 831 880 60 50
S Lyr 438 AMS 3100 600 0.44 6447 369 391 2060 80 80
ST Sgr 400 AMS 2600 600 0.03 5711 294 310 720 40 70
T Cam 369 AMC 2500 1300 0.04 5138 239 251 980 30 40
T Sgr 396 AMC 2700 1000 0.02 5635 287 302 1010 50 50
TT Cen 462 AMS 3000 1200 0.11 6910 417 444 1510 70 70
VX Aql 643 AMC 2700 700 0.01 10706 862 937 2450 110 120
W And 397 AMS 2600 600 0.02 5660 289 305 350 20 20
W Aql 479 AMS 2700 1200 0.7 7249 454 484 340 31 30
WY Cas 482 AMS 2700 600 0.12 7300 460 490 1080 50 50
χ Cyg 408 AMS 2600 1200 0.17 5862 309 326 180 10 5
M-type
BW Cam 628 AMS 3000 800 0.8 10376 820 891 1250 50 60
GX Mon 527 AMS 3500 800 5 8227 563 605 1430 70 70
GY Aql 464 AMS 2900 1200 0.3 6950 421 449 410 40 40
IK Tau 470 AMS 3000 900 0.8 7070 435 463 250 10 10
IRC−10529 675 AMS 3600 1200 4 11417 952 1039 930 70 60
IRC−30398 575 AMS 3100 1200 1.4 9233 681 735 670 50 40
IRC+10365 455 AMS 3000 600 0.7 6773 403 428 780 30 30
IRC+40004 720 AMS 2400 1200 2.5 12435 1085 1189 1160 60 70
KU And 720 AMS 2400 1200 2.5 12435 1085 1189 1170 70 60
NV Aur 635 AMS 3500 1100 4 10530 840 912 1325 65 65
R Cas 430 AMS 2900 1200 0.28 6293 353 374
R Hor 408 AMS 3100 600 0.04 5862 309 326 250 10 10
R Leo 312 AMS 2900 1200 0.11 4113 148 154 100 5 5
R LMi 372 AMS 2900 1200 0.19 5191 244 256 320 10 10
T Ari 314 AMS 3100 700 0.01 4145 151 157 290 5 10
T Cep 388 AMS 2900 800 0.02 5487 273 287 150 2 2
TX Cam 559 AMS 3000 1200 0.7 8894 640 690 410 60 60
U Men 409 AMS 2900 600 0.04 5881 311 328 330 20 10
WX Psc 660 AMS 3400 1100 4 11082 909 991 720 30 30

Notes. P: period in days. * dust type taken from Ramstedt et al. (2006). AMC: amorphous carbon. AMS: amorphous silicate. T⋆ is the stellar temperature; Tdust the dust temperature; τ10 the optical depth at 10 μm. the median luminosity; the lower/upper uncertainties on the luminosity. rPL(M) the median distance calculated with our new PL relation; the lower/upper uncertainties on the PL distance.

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