On the use of field RR Lyrae as Galactic probes - VII. Light curve templates in the LSST photometric system

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Volume 689 (September 2024)

A&A, 689 (2024) A349

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Table 2

Pulsation and fitting properties of the DECam z light curves of RRLs.

S19 ID	RA	Dec	P	mag	Ampl	$T_{r i s}^{z}$ $T_{ris}^z$	n	Fit	rej
	(deg)	(deg)	(days)	(mag)	(mag)	(days)
1131110	271.1231	−29.5742	0.537080	15.978	0.463	2456424.8524	55	F	0
1131438	271.1378	−29.5703	0.586080	15.851	0.381	2456453.6499	26	P	0
1132394	271.1834	−29.6777	0.495820	15.670	0.728	2456423.6250	51	F	0
1132647	271.1952	−29.6191	0.561640	16.003	0.425	2456423.4108	55	F	0
1133227	271.2210	−29.6234	0.711310	15.593	0.633	2456423.2454	73	F	0
1289124	271.3183	−29.6729	0.403450	16.326	0.797	2456423.4856	67	P	0
1290186	271.3692	−29.5505	0.588420	16.983	0.406	2456424.3231	57	P	0
1290223	271.3707	−29.6014	0.561410	15.892	0.385	2456423.1651	39	F	0
1290809	271.3985	−29.6636	0.494860	16.016	0.720	2456423.4253	67	P	0
1291217	271.4183	−29.5910	0.526810	15.883	0.663	2456452.4864	36	P	0

Notes. Fit: “F” indicates that the best fit is a Fourier series; “P” indicates that the best fit is a PLOESS. Only the first ten lines are displayed. The full table is available on the CDS.

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