SIMBAD references

2002ApJ...576L..25A - Astrophys. J., 576, L25-L28 (2002/September-1)

A new high-redshift Lyα emitter: possible superwind galaxy at z=5.69.

AJIKI M., TANIGUCHI Y., MURAYAMA T., NAGAO T., VEILLEUX S., SHIOYA Y., FUJITA S.S., KAKAZU Y., KOMIYAMA Y., OKAMURA S., SANDERS D.B., OYABU S., KAWARA K., OHYAMA Y., IYE M., KASHIKAWA N., YOSHIDA M., SASAKI T., KOSUGI G., AOKI K., TAKATA T., SAITO Y., KAWABATA K.S., SEKIGUCHI K., OKITA K., SHIMIZU Y., INATA M., EBIZUKA N., OZAWA T., YADOUMARU Y., TAGUCHI H., ANDO H., NISHIMURA T., HAYASHI M., OGASAWARA R. and ICHIKAWA S.-I.

Abstract (from CDS):

During the course of our deep optical imaging survey for Lyα emitters at z~5.7 in the field around the z=5.74 quasar SDSSp J104433.04-012502.2, we found a candidate strong emission line source. Follow-up optical spectroscopy shows that the emission-line profile of this object is asymmetric, showing excess red wing emission. These properties are consistent with an identification of Lyα emission at a redshift of z=5.687±0.002. The observed broad line width (ΔvFWHM≃340 km.s–1) and excess red wing emission also suggest that this object hosts a galactic superwind.

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Journal keyword(s): Galaxies: Formation - galaxies: individual (LAE J1044-0130) - Galaxies: Starburst

Nomenclature: [ATM2002] LAE JHHMM+DDMM N=1.

Simbad objects: 12

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