The GAPS Programme at TNG - XXXVI. Measurement of the Rossiter-McLaughlin effect and revising the physical and orbital parameters of the HAT-P-15, HAT-P-17, HAT-P-21, HAT-P-26, HAT-P-29 eccentric planetary systems

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Table 1

Details of the spectroscopic observations of the planetary transits recorded with HARPS-N.

Object	Date^(a)	UT start	UT end	N_obs	T_exp [sl	Airmass^(b)	Moon^(c)	2^nd fibre
HAT-P-15	2015-11-16	21:29	05:59	33	900	1.62→1.02→1.59	NO	Sky
HAT-P-17	2013-10-13	19:29	01:28	23	900	1.07→1.00→1.67	73%/41°	Sky
HAT-P-21	2014-03-07	22:24	04:37	36	600	1.28→1.02→1.28	46%/85°	Sky
HAT-P-26	2015-03-26	23:48	04:30	27	600	1.60→1.10→1.17	NO	Sky
HAT-P-29	2013-10-16	00:15	06:15	23	900	1.12→1.09→1.72	96%/56°	Sky

Notes. ^(a) Dates refer to the beginning of the night. ^(b) Values at first → meridian → last exposure. ^(c)Fraction of illumination and angular distance from the target.

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