First light of the VLT planet finder SPHERE - II. The physical properties and the architecture of the young systems PZ Telescopii and HD 1160 revisited

A.-L. Maire; M. Bonnefoy; C. Ginski; A. Vigan; S. Messina; D. Mesa; R. Galicher; R. Gratton; S. Desidera; T. G. Kopytova; M. Millward; C. Thalmann; R. U. Claudi; D. Ehrenreich; A. Zurlo; G. Chauvin; J. Antichi; A. Baruffolo; A. Bazzon; J.-L. Beuzit; P. Blanchard; A. Boccaletti; J. de Boer; M. Carle; E. Cascone; A. Costille; V. De Caprio; A. Delboulbé; K. Dohlen; C. Dominik; M. Feldt; T. Fusco; J. H. Girard; E. Giro; D. Gisler; L. Gluck; C. Gry; T. Henning; N. Hubin; E. Hugot; M. Jaquet; M. Kasper; A.-M. Lagrange; M. Langlois; D. Le Mignant; M. Llored; F. Madec; P. Martinez; D. Mawet; J. Milli; O. Möller-Nilsson; D. Mouillet; T. Moulin; C. Moutou; A. Origné; A. Pavlov; C. Petit; J. Pragt; P. Puget; J. Ramos; S. Rochat; R. Roelfsema; B. Salasnich; J.-F. Sauvage; H. M. Schmid; M. Turatto; S. Udry; F. Vakili; Z. Wahhaj; L. Weber; F. Wildi

doi:10.1051/0004-6361/201526594

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Volume 587 (March 2016)

A&A, 587 (2016) A56

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Table 1

Log of the SPHERE observations.

Object	UT date	Seeing (′′)	Mode	Bands	DIT (s) × NDIT		N_exp	ΔPA (°)
					IRDIS or ZIMPOL	IFS

PZ Tel	2014/07/15	0.88−1.11	IRDIFS	H2H3+YJ	20 × 6	60 × 2	16	7.6
PZ Tel	2014/08/06	0.5−0.7	IRDIS-LRS	YJH K_s	20 × 10	−	6	−
PZ Tel	2014/08/06	0.6−0.7	IRDIS-MRS	YJH	30 × 5	−	6	−
PZ Tel	2014/08/08	0.78−1.05	IRDIFS_EXT	K1K2+YJH	12 × 5	30 × 2	16	9.0
PZ Tel	2014/08/16	1.12−1.58	ZIMPOL	R′ I′	50 × 12	−	3	14.1
PZ Tel	2014/10/11	1.12−1.97	IRDIFS	H2H3+YJ	8 × 1^a	32 × 20^a	1	3.7^b
HD 1160	2014/08/13	0.54−0.84	IRDIFS_EXT	K1K2+YJH	4 × 20	8 × 15	16	18.4

Notes. The seeing is the value measured by the differential image motion monitor (DIMM) at 0.5 μm. DIT (detector integration time) refers to the single exposure time, NDIT (Number of Detector InTegrations) to the number of frames in a single data cube, N_exp to the number of data cubes, and ΔPA to the amplitude of the parallactic rotation.

^(a)

This sequence was a test and we only used the coronagraphic images with the satellite spots for measuring the astrometry of the companion.

^(b)

For the IFS data.

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