The Lyman alpha reference sample - VI. Lyman alpha escape from the edge-on disk galaxy Mrk 1486

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Volume 587 (March 2016)

A&A, 587 (2016) A77

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Table 1

HST imaging observations that are used in this present analysis of Mrk 1486.

Filter	Instrument	Bandpass	Pivot wavelength	Exposure time
		(Å)	(Å)	(s)

Archive data

F125LP (FUV)^a	ACS/SBC	1218−1987	1453	2669
F140LP (FUV)^a	ACS/SBC	1313−1989	1538	2669
F150LP (FUV)^a	ACS/SBC	1420−1992	1618	2669

New observations

F336W (U)^b	WFC3/UVIS	3014−3707	3355	1020
F438W (B)^b	WFC3/UVIS	3895−4710	4324	850
F775W (I)^b	WFC3/UVIS	6869−8571	7648	620
F502N (Hβ)^b	WFC3/UVIS	4963−5059	5010	2000
F673N (Hα)^b	WFC3/UVIS	6681−6860	6766	871

Notes.From the left column, we list the HST filters, the instrument or camera, the bandpass width (λ_min − λ_max), the pivot wavelength, and the exposure time for each filter in question.

^(a)

Archival observations from the program # GO 11110 (PI McCandliss).

^(b)

New imaging observations from the program # GO 12310 (PI G. Ostlin).

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