MUSE Analysis of Gas around Galaxies (MAGG) - VI. The cool and enriched gas environment of z ≳ 3 Lyα emitters

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Volume 690 (October 2024)

A&A, 690 (2024) A7

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Table 1.

MAGG sightlines targeted by the new VLT/X-shooter program PID 0109.A–0559.

Sightline	Redshift	S/N_3000 Å^(a)	S/N_3600 Å^(b)	Wavelength (Å) ^(c)
J010619+004823	4.4402	14	12	10 195–24 768
J033413−161205	4.3800	23	17	9817–24 767
J033900−013318	3.2040	21	18	10 194–24 766
J094932+033531	4.1072	26	28	10 195–24 767
J095852+120245	3.2746	16	21	10 195–24 768
J102009+104002	3.1528	23	20	10 195–24 768
J120917+113830	3.0836	15	13	10 195–24 769
J123055−113909	3.5570	15	19	10 195–24 771
J142438+225600	3.6340	128	115	10 194–24 765
J193957−100241	3.7870	31	52	9816–24 767
J200324−325144	3.7850	16	24	10 195–24 768
J205344−354652	3.4900	12	18	9817–24 766
J230301−093930	3.4774	22	25	10 195–24 768
J231543+145606	3.3971	18	15	10 194–24 767
J233446−090812	3.3261	19	23	10 195–24 768

Notes.

^(a)

Median signal-to-noise ratio per pixel at rest-frame λ_RF = 3000 Å computed within the range Δλ_RF = 2990 − 3010 Å.

^(b)

Median signal-to-noise at λ_RF = 3600 Å within the range Δλ_RF = 3590 − 3610 Å.

^(c)

NIR wavelength coverage.

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