Equivalent widths of Lyman α emitters in MUSE-Wide and MUSE-Deep

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Table 1.

Properties of HST filter bands used in this paper, for the CANDELS GOODS-S and COSMOS area.

HST filter	Sensitivity	Spatial resolution	Spatial sampling	Exposure time
		(arcsec)	(per pixel)	(s)
ACS F435W	27.8 ^(a,^c)	^(a,^b)		7200 ^(a)
ACS F606W	27.8 ^(a,^c)	^(a,^b)		3040 ^(a)
ACS F775W	27.1 ^(a,^c)	^(a,^b)		3040 ^(a)
ACS F814W	28.32 ^(d,^e)	^(d,^b)		5761 ^(d)
WFC 3 F125W	27.04 ^(d,^e)	^(d,^b)		1963 ^(d)
WFC 3 F160W	27.15 ^(d,^e)	^(d,^b)		3480 ^(d)

Notes.

^(a)

Information taken from Giavalisco et al. (2004).

^(b)

The FWHM of the point spread function (PSF).

^(c)

10σ point source sensitivity in AB magnitudes in an aperture with a diameter of .

^(d)

Information taken from Koekemoer et al. (2011).

^(e)

5σ magnitude for a point source using an aperture of three detector pixels for ACS F814W and four detector pixels for WFC 3 F125W and F160W for the CANDELS UDS field.

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