Exoplanets & Stellar Populations Group

Rosenberg early ground-based survey Here we publish the images, color-magnitude diagrams, and the F439W and F55W WFPC2 photometry for 74 GCs presented in Piotto et al. (2002), A&A, 391, 945.

Related papers to the program:

• Piotto et al. (2002), A&A, 391, 945

This is the collection of the dataset from a number of snapshot HST program carried out in Cycles 5-9. Click on header (from 1^st to 6^th column) to sort in ascending/descending order.

Key nomenclature below.

N.	Cluster ID	alias	Telescope	Fields n.	Stars n.	Identification, Positional & Metallicity parameters	PHotometric parameters	Kinematics & Structural parameters
1	NGC 104	47Tuc	D	1	5000	IPM table	PH table	KS table
2	NGC 288	-	D	2	5300	IPM table	PH table	KS table
3	NGC 362	-	D	1	2700	IPM table	PH table	KS table
4	NGC 1261	-	D	2	5000	IPM table	PH table	KS table
5	NGC 1851	-	D	1	7000	IPM table	PH table	KS table
6	NGC 1904	M79	D	1	4500	IPM table	PH table	KS table
7	NGC 2298	-	D	2	2800	IPM table	PH table	KS table
8	NGC 2808	-	D	3	14000	IPM table	PH table	KS table
9	E3	-	D	2	750	IPM table	PH table	KS table
10	NGC 3201	-	D	3	9000	IPM table	PH table	KS table
11	NGC 4372	-	D	2	7000	IPM table	PH table	KS table
12	NGC 4590	M68	D	2	3600	IPM table	PH table	KS table
13	NGC 4833	-	D	2	6200	IPM table	PH table	KS table
14	NGC 5053	-	JKT	1	5300	IPM table	PH table	KS table
15	NGC 5139	ω Cen	D	2	14700	IPM table	PH table	KS table
16	NGC 5272	M3	JKT	1	18800	IPM table	PH table	KS table
17	NGC 5466	-	JKT	1	5000	IPM table	PH table	KS table
18	NGC 5897	-	D	1	3400	IPM table	PH table	KS table
19	NGC 5904	M5	JKT	1	18300	IPM table	PH table	KS table
20	NGC 5927	-	D	1	4100	IPM table	PH table	KS table
21	NGC 5986	-	D	1	3400	IPM table	PH table	KS table
22	NGC 6093	M80	D	2	6800	IPM table	PH table	KS table
23	NGC 6101	-	D	1	1600	IPM table	PH table	KS table
24	NGC 6121	M4	D	2	4100	IPM table	PH table	KS table
25	NGC 6171	M107	D	2	3800	IPM table	PH table	KS table
26	NGC 6205	M13	JKT	1	15600	IPM table	PH table	KS table
27	NGC 6218	M12	JKT	1	7100	IPM table	PH table	KS table
28	NGC 6254	M10	JKT	1	13000	IPM table	PH table	KS table
29	NGC 6266	M62	D	1	2500	IPM table	PH table	KS table
30	NGC 6304	-	D	1	2800	IPM table	PH table	KS table
31	NGC 6341	M92	JKT	1	13900	IPM table	PH table	KS table
32	NGC 6352	-	D	1	5100	IPM table	PH table	KS table
33	NGC 6362	-	JKT	1	5500	IPM table	PH table	KS table
34	NGC 6366	-	D	1	3600	IPM table	PH table	KS table
35	NGC 6397	-	D	2	5600	IPM table	PH table	KS table
36	NGC 6496	-	D	1	3600	IPM table	PH table	KS table
37	NGC 6535	-	JKT	1	6500	IPM table	PH table	KS table
38	NGC 6541	-	D	1	4400	IPM table	PH table	KS table
39	NGC 6544	-	D	2	7300	IPM table	PH table	KS table
40	NGC 6624	-	D	1	4700	IPM table	PH table	KS table
41	NGC 6626	M28	D	1	5300	IPM table	PH table	KS table
42	NGC 6637	M69	D	1	3600	IPM table	PH table	KS table
43	NGC 6638	-	D	1	5000	IPM table	PH table	KS table
44	NGC 6656	M22	D	2	9100	IPM table	PH table	KS table
45	NGC 6681	M70	D	1	4500	IPM table	PH table	KS table
46	NGC 6717	Pal9	D	1	2500	IPM table	PH table	KS table
47	NGC 6723	-	D	1	2800	IPM table	PH table	KS table
48	NGC 6752	-	D	1	4700	IPM table	PH table	KS table
49	NGC 6779	M56	JKT	1	11200	IPM table	PH table	KS table
50	NGC 6809	M55	D	1	4700	IPM table	PH table	KS table
51	NGC 6838	M71	JKT	1	12300	IPM table	PH table	KS table
52	NGC 7078	M15	JKT	1	27000	IPM table	PH table	KS table

Legend

N. :	Progressive number.
Cluster ID :	Individual Schedules for each cluster are presented. Each schedule is comprehensive of CM diagram, fields images, cluster image...
alias :	other name (if any).
Telescope :	Telescope used for the observations. D = ESO Dutch Telescope; JKT = Jacobus Kapteyn Telescope.
Fields n. :	Number of fields obtained per cluster (only frames between 1200 s and 1800 s).
Stars n. :	Aproximate number of stars found in the field(s).
IPM parameters :	Identification, Positional data and Metallicity estimates IPM table.
PH parameters :	PHotometric parameters PH table.
KS parameters :	Kinematics and Structural parameters KS table.

Standard Stars & the calibration curves for each individual night used in each observing run are here.