A Herschel PACS survey of the dust and gas in Upper Scorpius disks

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Table 1

Target properties.

Object	Name^a	Sp.Type^b	A_V	log (L)	log (T)	M_star	W_λ(Hα)^c	SED	Accretion^d
			Mags	L_sun	K	M_sun	Å	class	state

1	HIP 76310	A0V	0.1	1.43	3.960	2.2	< −0.1	debris	No
2	HIP 77815	A5V	0.7	1.06	3.914	2.0	...	none	...
3	HIP 77911	B9V	0.3	1.88	4.050	2.8	< −0.1	debris	No
4	HIP 78099	A0V	0.5	1.43	3.960	2.2	< −0.1	none	No
5	HIP 78996	A9V	0.4	1.10	3.870	1.8	< −0.1	debris	No
6	HIP 79156	A0V	0.5	1.42	3.980	2.2	< −0.1	debris	No
7	HIP 79410	B9V	0.6	1.63	4.020	2.5	< −0.1	debris	No
8	HIP 79439	B9V	0.6	1.65	4.020	2.5	< −0.1	debris	No
9	HIP 79878	A0V	0.0	1.51	3.980	2.3	< −0.1	debris	No
10	HIP 80088	A9V	0.4	0.91	3.880	1.7	< −0.1	debris	No
11	HIP 80130	A9V	0.6	1.20	3.920	1.9	< −0.1	none	No
12	RX J1600.7-2343	M2	0.5	-0.95	3.557	0.5	...	none	...
13	ScoPMS 31	M0.5V	0.9	-0.43	3.570	0.4	–21.06	II	C
14	[PBB2002] J155624.8-222555	M4	1.7	–1.12	3.516	0.3	–5.4, –5.51	II	W
15	[PBB2002] J155706.4-220606	M4	2.0	–1.31	3.513	0.2	–3.6, –9.92	II	W
16	[PBB2002] J155729.9-225843	M4	1.4	–1.30	3.511	0.2	–7.0, –6.91	II	W
17	[PBB2002] J155829.8-231007	M3	1.3	–1.63	3.532	0.3	–250, –158	II	C
18	[PBB2002] J160210.9-200749	M5	0.8	–1.40	3.501	0.2	–3.5	none	W
19	[PBB2002] J160245.4-193037	M5	1.1	–1.31	3.495	0.2	–1.1	none	W
20	[PBB2002] J160357.9-194210	M2	1.7	–0.87	3.546	0.5	–3.0, –2.70	II	W
21	[PBB2002] J160525.5-203539	M5	0.8	–1.30	3.499	0.2	–6.1, –8.61	III	W
22	[PBB2002] J160532.1-193315	M5	0.6	–1.88	3.499	0.1	–26.0, –152	III	C
23	[PBB2002] J160545.4-202308	M2	2.2	–0.98	3.560	0.6	–35.0, –2.04	II	C
24	[PBB2002] J160600.6-195711	M5	0.6	–0.82	3.505	0.3	–7.5, –4.11	II	W
25	[PBB2002] J160622.8-201124	M5	0.2	–1.47	3.499	0.2	–6.0, –3.12	II	W
26	[PBB2002] J160643.8-190805	K6	1.8	–0.31	3.623	0.8	–2.39	III	W
27	[PBB2002] J160702.1-201938	M5	1.0	–1.37	3.501	0.2	–30.0, –8.3	II	C
28	[PBB2002] J160801.4-202741	K8	1.5	–0.45	3.601	0.7	–2.3	none	W
29	[PBB2002] J160823.2-193001	K9	1.5	–0.49	3.586	0.7	–6.0, –2.75	II	W
30	[PBB2002] J160827.5-194904	M5	1.1	–1.11	3.495	0.2	–12.3, –14.5	III	W
31	[PBB2002] J160900.0-190836	M5	0.7	–1.45	3.503	0.2	–15.4, –12.8	II	W
32	[PBB2002] J160900.7-190852	K9	0.8	–0.60	3.592	0.7	–12.7, –20.0	II	C
33	[PBB2002] J160953.6-175446	M3	1.9	–1.03	3.539	0.4	–22.0, –22.2	II	C
34	[PBB2002] J160959.4-180009	M4	0.7	–1.26	3.518	0.3	–4.0, –4.41	II	W
35	[PBB2002] J161115.3-175721	M1	1.6	–0.42	3.574	0.6	–2.4, –4.47	II	W
36^e	[PBB2002] J161420.3-190648	K5	1.8	–0.59	3.630	0.8	–52.0, –43.7	II	C
37	[PZ99] J153557.8-232405	K3	0.7	–0.12	3.649	0.9	0.0	none	W
38	[PZ99] J154413.4-252258	M1	0.6	–0.43	3.564	0.4	–3.15	none	W
39	[PZ99] J160108.0-211318	M0	0.0	–0.36	3.576	0.4	–2.4	none	W
40	[PZ99] J160357.6-203105	K5	0.9	–0.24	3.630	0.8	–11.57	II	C
41^f	[PZ99] J160421.7-213028	K2	1.0	–0.12	3.658	1.0	–0.57	II	W
42	[PZ99] J160654.4-241610	M3	0.0	–0.34	3.538	1.0	–3.62	none	W
43	[PZ99] J160856.7-203346	K5	1.4	–0.11	3.630	0.7	–0.47	none	W
44	[PZ99] J161402.1-230101	G4	2.0	0.30	3.724	1.5	0.0	none	No
45	[PZ99] J161411.0-230536	K0	2.4	0.74	3.676	1.0	0.96, 0.8, 0.38	II	W

Notes.

^(a)

Names with [PZ99] indicate naming based on Preibisch & Zinnecker (1999), and [PBB2002] indicates naming based on Preibisch et al. (2002).

^(b)

Spectral types from Hernández et al. (2005); Preibisch et al. (1998, 2002).

^(c)

W_λ(Hα) from Hernández et al. (2005); Preibisch et al. (1998, 2002); Riaz et al. (2006).

^(d)

Accretion determinations from Mathews et al. (2012b). For A and G stars, this indicates whether the star has detectable Hα emission possibly tracing accretion. For K & M stars, this indicates whether the star exhibits strong enough Hα emission to be classified as accreting according to the spectral type dependent criteria of White & Basri (2003). Objects with no Hα measurement in the literature are shown with no value.

^(e)

Referred to as J1614-1906 in the text.

^(f)

Referred to as J1604-2130 in the text.

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