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Table 1

Source summary.

ID Name RA Dec ObsIDs Fν 70 μm Fν 160 μm SpT Cloud Ref SD Multiplicity
(J2000) (J2000) [mJy] [mJy]
1 SSSPM1102 11 02 09.83 −34 30 35.5 1342221849/50 9.80 ± 1.03 8.02 ± 1.10 M8.5 TWA 1, 2
2 2M1207 12 07 33.47 −39 32 54.0 1342202557/58 7.24 ± 1.03 <17 M8.0 TWA 3, 2 binary
3 2MJ160859 16 08 59.54 −38 56 27.6 1342227823/24 7.4 ± 2.0 <35 M8.0 Lup III 4, 2
4 GY92 3 (ISO 032) 16 26 21.90 −24 44 39.8 1342238816/17 49.75 ± 5.58 <647 M8.0 Oph 5, 6
5 GY92 264 16 27 26.58 −24 25 54.4 1342238816/17 33.26 ± 5.45 <1489 M8.0 Oph 5, 6
6 GY92 310 16 27 38.63 −24 38 39.2 1342238816/17 120.28 ± 5.45 <1032 M8.5 Oph 7, 6 Y1
7 CFHTWIR96 16 27 40.84 −24 29 00.7 1342227841/42 <193 <1192 M8.25 Oph 8, 2
8 OTS 44 11 10 09.34 −76 32 17.9 1342238816/17 4.63 ± 1.03 <211 M9.5 Cha I 9, 10
9 2MJ111145 11 11 45.34 −76 36 50.5 1342223476/77 2.84 ± 1.03 <33 M8.0 Cha I 11, 2
10 J125758.7-770120 12 57 58.70 −77 01 19.5 1342212708/09 − <243 M9.0 Cha II 12, 13
11 KPNO 6 04 30 07.24 +26 08 20.8 1342227011/12 <4 <47 M9.0 Tau 14, 2
12 KPNO 7 04 30 57.19 +25 56 39.5 1342227999/8000 2.61 ± 1.03 <69 M8.25 Tau 14, 2
13 J04574903+3015195∗ 04 57 49.03 +30 15 19.5 1342243478/79 <8 <14 M9.25 Tau 15, 16
14 J04354526+2737130∗ 04 35 45.26 +27 37 13.1 1342243466/67 <11 <14 M9.2 Tau 17, 16
15 J04334291+2526470∗ 04 33 42.92 +25 26 47.0 1342243084/85 <7 <20 M8.75 Tau 17, 16
16 J04335245+2612548 04 33 52.46 +26 12 54.9 1342243080/81 8.00 ± 2.32 <26 M8.5 Tau 18, 16 Y1
17 J04290068+2755033 04 29 00.68 +27 55 03.4 1342243066/67 <9 <36 M8.25 Tau 17, 16
18 KPNO 4∗ 04 27 28.00 +26 12 05.3 1342242064/65 <9 <13 L0 Tau 15, 16
19 J04215450+2652315∗ 04 21 54.51 +26 52 31.5 1342242033/34 <7 <23 M8.5 Tau 17, 16
20 J04263055+2443558 04 26 30.55 +24 43 55.9 1342242023/24 8.00 ± 2.22 <33 M8.75 Tau 17, 16 Y1
21 J04274538+2357243∗ 04 27 45.38 +23 57 24.3 1342242021/22 <9 <23 M8.25 Tau 17, 16
22 J04302365+2359129 04 30 23.66 +23 59 13.0 1342242009/10 <7 <13 M8.5 Tau 17, 16
23 J04311907+2335047∗ 04 31 19.07 +23 35 04.7 1342242007/08 <8 <15 M8.0 Tau 19, 16
24 KPNO 9 04 35 51.43 +22 49 12.0 1342241979/80 <12 <16 M8.5 Tau 20, 16
25 J04361030+2159364 04 36 10.31 +21 59 36.5 1342241975/76 <8 <16 M8.5 Tau 17, 16
26 J04325119+1730092∗ 04 32 51.20 +17 30 09.2 1342241957/58 <9 <19 M8.25 Tau 21, 16
27 KPNO 1∗ 04 15 14.71 +28 00 09.6 1342241914/15 <6 <19 M8.75 Tau 15, 16
28 KPNO 12 04 19 01.27 +28 02 48.7 1342241888/89 <6 <49 M9.25 Tau 15, 16
29 J04221332+1934392 04 22 13.32 +19 34 39.2 1342241878/79 <10 <24 M8.0 Tau 17, 16 binary
30 J04414489+2301513 04 41 44.90 +23 01 51.4 1342240750/51 <12 <17 M8.5 Tau 17, 16 Y1 binary
31 ISO 138 11 08 18.51 −77 30 40.8 1342218699/700 4.52 ± 1.02 <89 M6.5 Cha I 22, 2
32 ISO 217 11 09 52.16 −76 39 12.8 1342223474/75 10.47 ± 1.10 <507 M6.25 Cha I 23, 2
33 CHAHA6 11 08 39.52 −77 34 16.7 1342223486/87 14.50 ± 1.10 <54 M5.75 Cha I 23, 2
34 2MJ110703 11 07 03.69 −77 24 30.7 1342223480/81 28.48 ± 1.02 <447 M7.5 Cha I 24, 2 Y1, Y2
35 CHAHA9 11 07 18.61 −77 32 51.7 1342223482/83 15.30 ± 1.01 <220 M5.5 Cha I 23, 2 Y1
36 ISO 252 11 10 41.42 −77 20 48.1 1342223478/79 8.81 ± 1.10 <122 M6.0 Cha I 23, 2
37 ISO 165 11 08 54.97 −76 32 41.1 1342223470/71 45.46 ± 1.02 31.89 ± 7.03 M5.5 Cha I 23, 2
38 CHAII1258 12 58 06.76 −77 09 09.5 1342224206/07 5.06 ± 1.01 <116 M6.0 Cha II 25, 2
39 CHAII1308 13 08 27.14 −77 43 23.3 1342224204/05 6.43 ± 1.01 <37 M6.0 Cha II 25, 2
40 CFHTTAU12 04 33 09.46 +22 46 48.7 1342227013/14 <7 <54 M6.5 Tau 17, 2
41 CFHTTAU9 04 24 26.46 +26 49 50.4 1342227059/60 10.64 ± 1.09 <26 M6.25 Tau 17, 2
42 SORI053825 05 38 25.44 −02 42 41.3 1342226721/22 <12 <22 M7.0 σ Ori 26, 2
43 OPHALL1622 16 22 44.94 −23 17 13.4 1342227839/40 5.75 ± 1.02 <160 M6.0 Oph 25, 2 Y1
44 2MJ160737 16 07 37.73 −39 21 38.8 1342227813/14 16.15 ± 1.02 8.54 ± 1.61 M5.75 Lup III 4, 2
45 DENIS 1603 16 03 34.71 −18 29 30.4 1342227831/32 3.60 ± 1.01 <22 M5.5 Upper Sco 27, 2
46 USCO112 16 00 26.70 −20 56 31.6 1342227140/41 <5 <12 M5.5 Upper Sco 28, 2
47 USCO128 15 59 11.36 −23 38 00.2 1342227134/35 5.69 ± 1.02 <25 M7.0 Upper Sco 28, 2 Y2
48 USCO55 16 02 45.60 −23 04 50.0 1342227136/37 13.26 ± 1.02 <11 M5.5 Upper Sco 28, 2 Y2
49 USD155556 15 55 56.01 −20 45 18.7 1342227138/39 15.92 ± 1.01 <11 M6.5 Upper Sco 27, 2 Y1, Y2
50 USD155601 15 56 01.04 −23 38 08.1 1342227132/33 7.52 ± 1.01 <37 M6.5 Upper Sco 27, 2 Y2
51 USD160603 16 06 03.91 −20 56 44.4 1342227142/43 3.49 ± 1.01 <24 M7.5 Upper Sco 27, 2
52 USD160958 16 09 58.53 −23 45 18.6 1342227146/47 6.07 ± 1.01 <18 M6.5 Upper Sco 27, 2
53 USD161005 16 10 05.42 −19 19 36.3 1342227829/30 5.37 ± 1.01 8.80 ± 1.61 M7.0 Upper Sco 27, 2
54 USD161833 16 18 33.18 −25 17 50.5 1342227827/28 10.42 ± 1.02 <93 M6.0 Upper Sco 27, 2 binary
55 USD161939 16 19 39.76 −21 45 35.0 1342227835/36 15.88 ± 1.01 <42 M7.0 Upper Sco 27, 2 binary

Notes. (1) (2) The horizontal line divides the sample into a group of late-type BDs (M8 and later, top) and a group of early-type BDs (earlier than M8, bottom). (3) The ObsIDs contain both the scan and cross scan ID numbers of the observations. Taking SSSPM1102 as an example, 1342221849 is the scan ID and 1342221850 is the cross-scan ID. All ObsIDs follow the same convention. (4) First reference listed is for spectral type. Further information (e.g., near- and mid-IR photometry) can be found in the second reference and references therein. (5) The column “SD” marks the objects for which the re-measured PACS photometry are significantly different from the literature values at 70 μm (Y1) and 160 μm (Y2) respectively, see Sect. 3.3.

(∗)

Marks sources without clear excess emission at near- and mid-IR wavelengths.

Reference. (1) Scholz et al. (2005); (2) Harvey et al. (2012a); (3) Gizis (2002); (4) Allen et al. (2007); (5) Wilking et al. (2005); (6) Alves de Oliveira et al. (2013); (7) Wilking et al. (1999); (8) Alves de Oliveira et al. (2010); (9) Luhman et al. (2004); (10) Joergens et al. (2013); (11) Luhman (2007); (12) Spezzi et al. (2008); (13) Spezzi et al. (2013); (14) Guieu et al. (2007); (15) Canty et al. (2013); (16) Bulger et al. (2014); (17) Luhman (2006); (18) Luhman et al. (2006); (19) Slesnick et al. (2006); (20) Briceño et al. (2002); (21) Luhman et al. (2009); (22) Luhman (2004); (23) Damjanov et al. (2007); (24) Luhman et al. (2008); (25) Gully-Santiago et al. (2011); (26) Rigliaco et al. (2011); (27) Martín et al. (2004); (28) Ardila et al. (2000).

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