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Table 1

Hubble Space Telescope observations of NGC 362 used in this work.

Instrument Date Filter No. of images Proposal ID PI N × Exp. time (s)
ACS/WFC 2003 Dec. 04 F435W 4 10 005 Lewin 4 × 340
ACS/WFC 2003 Dec. 04 F625W 4 10 005 Lewin 2 × 110, 2 × 120
ACS/WFC 2003 Dec. 04 F658N 4 10 005 Lewin 2 × 440, 2 × 500
ACS/HRC 2004 Dec. 06 F435W 16 10 401 Chandar 16 × 85
ACS/WFC 2006 Jun. 02 F606W 5 10 775* Sarajedini 4 × 150, 1 × 10
ACS/WFC 2006 Jun. 02 F814W 5 10 775* Sarajedini 4 × 170, 1 × 10
WFC3/UVIS 2012 Apr. 13 F390W 14 12 516 Ferraro 14 × 348
WFC3/UVIS 2012 Apr. 13 F555W 10 12 516 Ferraro 1 × 160, 1 × 200, 1 × 145, 1 × 144, 6 × 150
WFC3/UVIS 2012 Apr. 13 F814W 15 12 516 Ferraro 3 × 390, 12 × 348
WFC3/UVIS 2016 Sept. 18 F225W 18 14 155 Kalirai 3 × 30, 3 × 680, 8 × 700, 3 × 650, 1 × 580
WFC3/UVIS 2016 Sept. 18 F275W 7 14 155 Kalirai 2 × 30, 680, 2 × 700, 2 × 650

Notes. From left to right: HST instrument name, date of observation, filter of the observation, number of images, proposal ID, principal investigator and exposure time in seconds for each image. The asterisk (*) in the fifth column denotes the HST observations that were also used by Kumawat et al. (2024). Conversely, the observations used in their work but not used in our analysis are the WFC3/UVIS images from Proposal GO-12605, specifically in the F275W, F336W, and F438W filters. All WFC3/UVIS and ACS/HRC observations listed in the table were processed following the photometric reduction described in Sects. 2.1 and 2.2, and the resulting catalogues were subsequently used in the analysis. The only external catalogue used in this study is the one from Libralato et al. (2018, 2022) , constructed from the ACS/WFC observations.

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