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Table 1

Overview of the observations of the dust shell of W Hya using different telescopes.

Instrument Date Φ Ref. λ [μm] FOV [“×”] Identifier

ISO SWS 1 14-02-1996 0.12 Sloan et al. (2003) 2.36–45.39 14 × 20 to 17 × 40 08902004
ISO SWS 2 07-01-1997 0.17 Justtanont et al. (2004) 2.36–45.39 14 × 20 to 17 × 40 41800303
ISO LWS 1 07-02-1996 0.1 ISO data archivea 43.05–195.5 80 × 80 to 70 × 70 08200208
ISO LWS 2 05-02-1997 0.1 ISO data archivea 43.05–195.5 80 × 80 to 70 × 70 44700672
ISO LWS 3 02-08-1997 0.6 ISO data archivea 43.05–195.5 80 × 80 to 70 × 70 62500572
PACS Spec B2A 09-07-2011 0.8 Khouri et al. (2014a) 55–73 30 × 30 1342212604
PACS Spec R1A 09-07-2011 0.8 Khouri et al. (2014a) 102–146 30 × 30 1342212604
PACS Spec B2B 14-01-2011 0.4 Khouri et al. (2014a) 70–105 30 × 30 1342223808
PACS Spec R1B 14-01-2011 0.4 Khouri et al. (2014a) 140–210 30 × 30 1342223808
SPIRE Spec 09-01-2010 0.27 Khouri et al. (2014a) 124–671 37 × 37 to 18 × 18 1342189116
PACS Image 70 08-02-2011 0.47 Cox et al. (2012) 60–85 1440 × 1440 1342213848
PACS Image 160 08-02-2011 0.47 Cox et al. (2012) 130–210 1440 × 1440 1342213849
SCUBA 450 and 850
VLT - MIDI 04-2007 – 09-2009 Zhao-Geisler et al. (2011) 8–13
VLT - NACO 03-2009 and 06-2010 0.2b Norris et al. (2012) 1.04, 1.24 and 2.06

Notes. The phase Φ of the pulsation period is given based on observations of visible light made available by the AAVSO (American Association of Variable Star Observers) at http://www.aavso.org/;

(b)

Visual phase given by Norris et al. (2012).

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