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Table 2

Stellar fluxes (in Jy) in the apertures listed between parenthesis (in arcseconds) of the AGB and post-AGB stars observed per October 17th. Add 1342100000 to the AOR number quoted to obtain the Observation ID. Date refers to the observing date (format yy-mm-dd), when two are listed the first refers to the PACS observations, the second to the date of the SPIRE observations.

Object PACS blue Red SPIRE PSW PMW PLW AOR Date Remarks
70 μm 160 μm 250 μm 350 μm 500 μm

AFGL 190 42.9 (33) 6.26 (31) 89183, 89184 10-01-12
AFGL 2155 54.1 (35) 8.57 (34) 92777, 92778 10-03-26
AFGL 2688 2047 (110) 488 (118) 119 (106) 48.9 (140) 18.2 (92) 95837, 95838, 88168 10-05-05, 09-12-16
AFGL 278 22.7 (29) 3.30 (28) 89840, 89841 10-01-28
AFGL 3068 175 (40) 27.6 (34) 6.93 (56) 3.32 (136) 1.26 (92) 88178, 88378, 88379 09-12-21, 09-12-16
AFGL 3116 73.0 (46) 12.6 (50) 88490, 88491 09-12-23
AFGL 618 953 (104) 196 (86) 46.1 (101) 19.0 (87) 8.91 (92) 93132, 93133, 91183 10-03-31, 10-02-25
α ORI 294 (130) 35.5 (82) 6.18 (57) 2.84 (68) 1.56 (92) 104435, 104436, 92099 10-09-13, 10-03-11 c
AQ AND 0.914 (14) 0.391 (28) 88488, 88489 09-12-23 a
AQ SGR 2.05 (14) 0.354 (28) 95702, 95703 10-04-30
CIT 6 8.81 (72) 3.77 (85) 1.77 (92) 106689 10-10-17
CW LEO 3653 (244) 610 (253) 138 (211) 57.7 (325) 23.2 (276) 86298, 86299, 86293 09-10-25
EP AQR 26.6 (31) 4.14 (31) 95460, 95461 10-04-23 b
HD 161796 109 (42) 14.5 (44) 2.39 (45) 0.731 (63) 0.254 (92) 88155, 91127, 91128 10-02-24, 09-12-15
HD 179821 439 (63) 62.0 (55) 93490, 93491 10-04-03
HD 235858 60.2 (42) 7.98 (28) 96757, 96758 10-05-20 c
HD 44179 139 (49) 32.5 (55) 9.51 (50) 4.46 (67) 2.46 (92) 85549, 85550, 83682 09-10-09, 09-09-12
HD 56126 1.21 (45) 0.190 (92) 0.388 (63) 93007 10-03-28
IRAS 11385-5517 207 (55) 62.8 (62) 102339, 102340 10-08-09
IRAS 15194-5115 106 (48) 22.9 (72) 90247, 90248 10-02-05
IRAS 16594-4656 82.0 (39) 12.3 (28) 93052, 93053 10-03-30
IRAS 19343+2926 116 (44) 33.9 (46) 91951, 91952 10-03-10
IRC -10 529 77.9 (40) 12.1 (44) 96034, 96035 10-05-09
χ CYG 53.5 (48) 8.49 (38) 88320, 88321 09-12-20
 μ CEP 100 (86) 8.47 (39) 91945, 91946 10-03-10 b
NML CYG 786 (82) 109 (35) 95485, 95486 10-04-24 c
NML TAU 202 (69) 27.6 (67) 5.99 (63) 2.71 (119) 0.876 (92) 90343, 90344, 91180 10-02-10, 10-02-25 c
OH 127.8+0.0 87.9 (41) 9.90 (31) 89181, 89182 10-01-12
OH 26.5+0.6 317 (44) 35.4 (28) 91817, 91818 10-03-09 c
o CET 245 (99) 35.2 (90) 6.87 (63) 2.71 (73) 1.27 (92) 90335, 90336, 89423 10-02-09, 10-01-17 c
o ORI 1.79 (14) 0.368 (28) 91108, 91109 10-02-23
π GRU 48.6 (56) 6.50 (47) 1.54 (45) 0.687 (63) 0.313 (92) 96799, 96800,93791 10-05-21, 10-04-05 c
R AQR 1.03 (45) 0.423 (63) 0.226 (92) 88166 09-12-16
R CAS 2.90 (45) 1.51 (63) 0.917 (92) 88578 09-12-25 c
R DOR 193 (79) 32.7 (57) 9.63 (62) 4.73 (154) 2.19 (92) 97685, 97686, 88164 10-06-03, 09-12-16
R FOR 9.00 (21) 1.38 (28) 88502, 88503 09-12-24
R HYA 49.5 (37) 7.95 (32) 2.88 (47) 1.50 (85) 0.841 (92) 102231, 102232, 88662 10-08-06, 09-12-27
R LEP 16.5 (28) 2.51 (28) 90304, 90305 10-02-07
R SCL 1.63 (45) 0.692 (63) 0.303 (92) 88657 09-12-26
RT CAP 2.34 (16) 0.363 (28) 96036, 96037 10-05-09
RT VIR 23.4 (39) 3.80 (34) 101181, 101182 10-07-24
RX BOO 1.44 (25) 0.798 (63) 0.402 (92) 88158, 09-12-16
RY DRA 4.61 (19) 0.810 (28) 88338, 88339 09-12-21
RZ SGR 4.19 (22) 2.88 (31) 93532, 93533 10-04-03 b
S CAS 19.6 (26) 2.64 (28) 105040, 105041 10-09-22
S CEP 15.7 (27) 3.03 (28) 1.09 (45) 0.759 (63) 0.410 (92) 88342, 88343, 103604 09-12-21, 10-08-24 a
ST CAM 3.04 (16) 0.477 (28) 106044, 106045 10-10-07
ST HER 8.68 (26) 1.23 (28) 88324, 88325 09-12-20
θ APS 30.2 (37) 4.38 (33) 1.05 (45) 0.476 (63) 0.174 (92) 93048, 93049, 103637 10-03-30, 10-08-24 a
T LYR 2.92 (15) 0.673 (28) 95694, 95695 10-04-30
T MIC 17.2 (26) 2.90 (28) 93036, 93037 10-03-30 c
TT CYG 0.725 (14) 0.139 (14) 93500, 93501 10-04-03 a
TW HOR 3.55 (18) 0.537 (28) 88373, 88374 09-12-21
TX PSC 8.34 (43) 1.61 (35) 88344, 88345 09-12-21 b
U ANT 6.35 (14) 2.51 (28) 0.491 (25) 0.210 (25) 0.074 (25) 88474, 88475, 88161 09-12-23, 09-12-16 d
U CAM 8.65 (21) 1.69 (28) 0.891 (45) 0.515 (63) 0.239 (92) 90307, 90308, 103608 10-02-07, 10-08-24
UU AUR 8.52 (26) 1.44 (28) 106332, 106333 10-10-12
UX DRA 2.08 (17) 0.481 (28) 0.156 (45) 0.110 (63) 0.099 (92) 88340, 88341, 103603 09-12-21, 10-08-24 a
V CRB 3.01 (17) 0.580 (28) 88326, 88327 09-12-20
V CYG 28.1 (37) 4.97 (28) 88462, 88463 09-12-22 b
V ERI 11.3 (27) 1.55 (28) 89943, 89944 10-01-31
V HYA 2.74 (50) 1.31 (63) 0.552 (92) 88160 09-12-16
V PAV 5.18 (19) 0.845 (28) 104278, 104279 10-09-10
VX SGR 179 (62) 22.7 (36) 91799, 91800 10-03-09
VY CMA 1096 (102) 137 (28) 94070, 94071 10-04-07
W AQL 70.5 (58) 11.3 (59) 94084, 94085 10-04-08 b
W HYA 7.50 (49) 3.39 (67) 1.66 (92) 89519 10-01-19 c
W ORI 8.07 (22) 1.41 (28) 90965, 90966 10-02-22
W PIC 2.44 (14) 0.575 (28) 90974, 90975 10-02-22
WX PSC 105 (50) 19.0 (68) 88486, 88487 09-12-23
X HER 25.6 (47) 4.07 (40) 88322, 88323 09-12-20 b
X TRA 7.90 (25) 1.30 (28) 93050, 93051 10-03-30
Y CVN 10.4 (27) 1.89 (28) 0.630 (45) 0.468 (63) 0.235 (92) 88330, 88331, 88157 09-12-20, 09-12-15 b
Y PAV 2.94 (16) 0.468 (28) 88157 09-12-15

Notes. Remarks: Sources are listed alphabetically. Internal errors in the fluxes are small and of order 0.01 Jy (PACS) and 0.02 Jy (SPIRE). The errors in the fluxes are dominated by the flux calibration accuracy, currently estimated to be 10% for the PACS 70 μm band and better than 15% at 160 μm, and 15% for all SPIRE bands.

(a)

Aperture includes only the central star;

(b)

Aperture includes (part of) the extended emission;

(c)

Some contamination by extended emission in the aperture or sky annulus;

(d)

Only PACS blue and red and SPIRE PSW are essentially free from emission of the detached shell.

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