CALYMHA -S16-373 , the SIMBAD biblio

CALYMHA -S16-373 , the SIMBAD biblio (6 results)

C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST06:30:37

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Bibcode/DOI	Score	in a table	in teXt, Caption, ...	Nb occurence	Nb objects in ref	Citations (from ADS)	Title	First 3 Authors
`2014ApJ...788...74S`	`16`	`D`		`1`	`44`	`121`	What is the physical origin of strong Lyα emission? II. Gas kinematics and distribution of Lyα emitters.	SHIBUYA T., OUCHI M., NAKAJIMA K., et al.
`2015ApJ...812..157H`	`524`	`D`	`X C`	`13`	`16`	`56`	A close comparison between observed and modeled Lyα lines for z ∼ 2.2 Lyα emitters.	HASHIMOTO T., VERHAMME A., OUCHI M., et al.
`2017MNRAS.465.1543H`	`16`	`D`		`1`	`18`	`16`	Lyα emitters with very large Lyα equivalent widths, EW₀(Lyα) ~= 200-400 Å, at z ∼ 2.	HASHIMOTO T., OUCHI M., SHIMASAKU K., et al.
`2018MNRAS.477.2817S`	`17`	`D`		`3`	`42`	`71`	The nature of luminous Ly α emitters at z ∼ 2-3: maximal dust-poor starbursts and highly ionizing AGN.	SOBRAL D., MATTHEE J., DARVISH B., et al.
`2021MNRAS.505.1382M`	`17`	`D`		`1`	`37`	`36`	The X-SHOOTER Lyman α survey at z = 2 (XLS-z2) I: what makes a galaxy a Lyman α emitter?	MATTHEE J., SOBRAL D., HAYES M., et al.
`2022MNRAS.510.4582N`	`146`	`D`	`X`	`4`	`33`	`60`	The synchrony of production and escape: half the bright Lyα emitters at z ≃ 2 have Lyman continuum escape fractions ≃50.	NAIDU R.P., MATTHEE J., OESCH P.A., et al.