Gas structure inside dust cavities of transition disks: Ophiuchus IRS 48 observed by ALMA

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Table 2

Observed continuum fluxes.

Instrument	Wavelength	Flux	Reference
	(μm)	(Jy)

Photometry

NOMAD	0.43	1.60(−5)	Zacharias et al. (2005)
NOMAD	0.64	3.26(−4)	Zacharias et al. (2005)
2MASS	1.24	9.46(−2)	Cutri et al. (2003)
2MASS	1.66	3.05(−1)	Cutri et al. (2003)
2MASS	2.16	6.18(−1)	Cutri et al. (2003)
WISE	3.4	1.29	Wright et al. (2010)
IRAC	3.6	1.41	van Kempen et al. (2009)
IRAC	4.5	1.60	van Kempen et al. (2009)
WISE	4.6	2.45	Wright et al. (2010)
IRAC	5.8	4.06	van Kempen et al. (2009)
IRAC	8.0	6.00	van Kempen et al. (2009)
IRAS	12.0	7.81	Helou & Walker (1988)
WISE	12.0	6.26	Wright et al. (2010)
AKARI	18.7	21.0	Yamamura et al. (2010)
VISIR	18.7	31.8	Geers et al. (2007)
WISE	22.0	36.5	Wright et al. (2010)
IRAS	25.0	46.5	Helou & Walker (1988)
IRAS	60.0	<65.5	Helou & Walker (1988)
MIPS	70.0	17.0	van Kempen et al. (2009)
PACS	70.0	31.0	Fedele et al. (2013)
IRAS	100.0	<225.0	Helou & Walker (1988)
ALMA	450.0	9.50(−1)	van der Marel et al. (2013a)
SCUBA	450.0	<1.57	Andrews & Williams (2007)
SCUBA	850.0	1.80(−1)	Andrews & Williams (2007)
SMA	880.0	1.60(−1)	Andrews & Williams (2007)
SMA	1300.0	6.00(−2)	Andrews & Williams (2007)

Spectroscopy

IRS	5.9−36.89		McClure et al. (2010)
PACS	60.0−73.3 (B1)		Fedele et al. (2013)
	69.8−95.0 (B1)		Fedele et al. (2013)
	105.0−146.6 (R1)		Fedele et al. (2013)
	139.6−180.9 (R2)		Fedele et al. (2013)

Notes.a(b) means a × 10^b.

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