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Table C.1

Observation settings of carbon-rich AGB stars observed with the PACS instrument onboard Herschel in the MESS and OT2 programs.

Target RA Dec Obsid OD Date of obs. (UTC) tobs (s) Mode Bands

RW LMi 10:16:02.27 30:34:18.60 1342197799 387 Jun. 05 14:38:11 2010 2373 SED B2B-R1B
1342197800 387 Jun. 05 15:08:40 2010 1125 SED B2A-R1A
V Hya 10:51:37.25 –21:15:00.30 1342197790 387 Jun. 05 07:56:09 2010 4605 SED B2B-R1B
1342197791 387 Jun. 05 08:54:29 2010 2124 SED B2A-R1A
II Lup 15:23:04.91 –51:25:59.00 1342215685 665 Mar. 10 07:59:32 2011 2373 SED B2B-R1B
1342215686 665 Mar. 10 08:30:02 2011 1125 SED B2A-R1A
V Cyg 20:41:18.27 48:08:28.80 1342208939 550 Nov. 15 02:00:33 2010 1125 SED B2A-R1A
1342208940 550 Nov. 15 02:31:02 2010 2373 SED B2B-R1B
LL Peg 23:19:12.39 17:11:35.40 1342199417 412 Jun. 30 09:29:02 2010 1125 SED B2A-R1A
1342199418 412 Jun. 30 09:59:30 2010 2373 SED B2B-R1B
LP And 23:34:27.66 43:33:02.40 1342212512 607 Jan. 11 00:55:51 2011 2124 SED B2A-R1A
1342212513 607 Jan. 11 01:54:11 2011 4605 SED B2B-R1B

R Scl 01:26:58.09 –32:32:35.40 1342247730 1149 Jul. 06 01:16:10 2012 2863 LINE B2B-R1A-R1B
1342247731 1149 Jul. 06 01:44:54 2012 547 LINE B3A
V384 Per 03:26:29.51 47:31:48.60 1342250571 1209 Sep. 04 02:22:04 2012 1261 LINE R1A
1342250572 1209 Sep. 04 02:59:51 2012 3231 LINE B2B-R1B
1342250573 1209 Sep. 04 03:31:41 2012 547 LINE B3A
R Lep 04:59:36.35 –14:48:22.50 1342249508 1188 Aug. 14 11:43:13 2012 895 LINE R1A
1342249509 1188 Aug. 14 12:11:34 2012 2465 LINE B2B-R1B
1342249510 1188 Aug. 14 12:37:01 2012 547 LINE B3A
W Ori 05:05:23.72 01:10:39.50 1342249502 1188 Aug. 14 09:40:23 2012 1993 LINE R1A
1342249503 1188 Aug. 14 10:24:16 2012 3231 LINE B2B-R1B
1342249504 1188 Aug. 14 10:56:06 2012 547 LINE B3A
S Aur 05:27:07.45 34:08:58.60 1342250895 1216 Sep. 11 13:24:59 2012 1627 LINE R1A
1342250896 1216 Sep. 11 14:18:34 2012 4761 LINE B2B-R1B
1342250897 1216 Sep. 11 15:09:57 2012 1363 LINE B3A
U Hya 10:37:33.27 –13:23:04.40 1342256946 1307 Dec. 11 11:07:39 2012 1627 LINE R1A
1342256947 1307 Dec. 11 11:48:29 2012 3231 LINE B2B-R1B
1342256948 1307 Dec. 11 12:20:19 2012 547 LINE B3A
QZ Mus 11:33:57.91 –73:13:16.30 1342247718 1148 Jul. 05 06:26:18 2012 3609 LINE B2B-R1A-R1B
1342247719 1148 Jul. 05 07:04:35 2012 547 LINE B3A
Y CVn 12:45:07.83 45:26:24.90 1342254304 1269 Nov. 02 17:45:29 2012 1261 LINE R1A
1342254305 1269 Nov. 02 18:16:53 2012 2465 LINE B2B-R1B
1342254306 1269 Nov. 02 18:45:44 2012 955 LINE B3A
AFGL 4202 14:52:24.29 –62:04:19.90 1342250003 1195 Aug. 21 10:00:56 2012 895 LINE R1A
1342250004 1195 Aug. 21 10:29:17 2012 2465 LINE B2B-R1B
1342250005 1195 Aug. 21 10:54:44 2012 547 LINE B3A
V821 Her 18:41:54.39 17:41:08.50 1342244456 1068 Apr. 16 12:01:59 2012 2863 LINE B2B-R1A-R1B
1342244457 1068 Apr. 16 12:30:43 2012 547 LINE B3A
V1417 Aql 18:42:24.68 –02:17:25.20 1342244470 1068 Apr. 16 20:05:15 2012 2863 LINE B2B-R1A-R1B
1342244471 1068 Apr. 16 20:33:59 2012 547 LINE B3A
S Cep 21:35:12.83 78:37:28.20 1342246553 1115 Jun. 01 18:47:49 2012 3258 LINE B2B-R1A-R1B
1342246554 1115 Jun. 01 19:22:51 2012 547 LINE B3A
RV Cyg 21:43:16.33 38:01:03.00 1342247466 1140 Jun. 27 11:54:06 2012 2815 LINE B2B-R1A
1342247467 1140 Jun. 27 12:34:59 2012 2055 LINE B2B-R1A-R1B
1342247468 1140 Jun. 27 13:00:23 2012 955 LINE B3A
LL Peg 23:19:12.39 17:11:35.40 1342257222 1310 Dec. 14 13:16:04 2012 547 LINE B3A
1342257635 1317 Dec. 21 09:38:25 2012 2465 LINE B2B-R1B
1342257684 1319 Dec. 22 16:45:23 2012 1261 LINE R1A

Notes. Given are the right ascension (RA) and declination (Dec), observation identifier (Obsid), day of observation from the start of operations (OD), date of observation, total observation time including overhead (tobs), observation mode (SED for full spectral-range scan from the MESS program, or LINE for line scan from the OT2 program), and bands in which spectra were taken. All observations were single pointings and were performed in chop-nodded mode. Line scans denoted as LINE were observed with the range-scan observing template and were treated as line scans in the data reduction. LL Peg is listed twice, as it was observed in both the MESS and OT2 programs. The OT2-program target R Scl is included for completeness, but is not used in the remainder of this study.

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