J/MNRAS/473/30 Catalog of Ly{alpha} emitters (Caruana+, 2018) ================================================================================ The MUSE-Wide survey: a measurement of the Ly{alpha} emitting fraction among z > 3 galaxies. Caruana J., Wisotzki L., Herenz E.C., Kerutt J., Urrutia T., Schmidt K.B., Bouwens R., Brinchmann J., Cantalupo S., Carollo M., Diener C., Drake A., Garel T., Marino R.A., Richard J., Saust R., Schaye J., Verhamme A. =2018MNRAS.473...30C (SIMBAD/NED BibCode) ================================================================================ ADC_Keywords: Galaxy catalogs ; Ultraviolet ; Redshifts Keywords: galaxies: high-redshift - galaxies: star formation - galaxies: statistics Abstract: We present a measurement of the fraction of Lyman {alpha} (Ly{alpha}) emitters (X_Ly{alpha}_) amongst HST continuum-selected galaxies at 3~0.5 for most of the redshift range covered, with 29 per cent of the Ly{alpha} sample exhibiting rest equivalent widths (rest-EWs)<=15{AA}. Adopting a range of rest-EW cuts (0~75{AA}), we find no evidence of a dependence of XLy{alpha} on either redshift or ultraviolet luminosity. Description: The MUSE-Wide project (see also Herenz et al., 2017A&A...606A..12H, Cat. J/A+A/606/A12) is a blind spectroscopic survey (PI: L. Wisotzki) using the MUSE panoramic integral field spectrograph at the ESO-VLT, carried out as a part of the GTO awarded to the MUSE consortium. The final survey covers some 100-arcmin^2^ in areas with deep HST imaging and complementary multiwavelength data, with the Chandra Deep Field-South (CDFS) as the primary region of interest. MUSE covers a fixed spectral range from 4750 to 9300{AA} with a resolution of 2.5{AA} (full width at half-maximum). This paper uses data from the first 24 MUSE-Wide pointings in the CDFS-Deep part of the CANDELS HST imaging survey (Cosmic Assembly Near-Infrared Deep Extragalactic Legacy Survey), which in turn was built on top of the earlier GOODS imaging campaign (Giavalisco et al., 2004ApJ...600L..93G, Cat. II/261). Our 24 MUSE fields are also all located within the footprint of the 3D-HST grism survey (Brammer et al., 2012ApJS..200...13B; Momcheva et al., 2016, Cat. J/ApJS/225/27). File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file tablea1.dat 57 100 The catalog of Ly{alpha} emitters -------------------------------------------------------------------------------- See also: II/261 : GOODS initial results (Giavalisco+, 2004) J/ApJS/225/27 : 3D-HST Survey: grism spectra master catalog (Momcheva+, 2016) J/A+A/606/A112 : Abundance analysis of ALW Carina 8 (Susmitha+, 2017) Byte-by-byte Description of file: tablea1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 I5 --- IDSkelton ID number in Skelton et al., Cat. J/ApJS/214/24, in GOODS-S field 7- 11 I5 --- IDGuo ID number in Guo et al., Cat. J/ApJS/207/24 13- 18 F6.2 mag MUV Absolute UV (F814W) magnitude 20- 28 F9.2 10-23W/m2 Flux Flux of the Ly{alpha} line at 3-Kron radius 30- 37 F8.2 10-23W/m2 e_Flux rms uncertainty on Flux 39- 45 F7.2 0.1nm rest-EW Rest equivalent width 47- 52 F6.2 0.1nm e_rest-EW rms uncertainty on rest-EW 54- 57 F4.2 --- z Redshift -------------------------------------------------------------------------------- History: From electronic version of the journal ================================================================================ (End) Patricia Vannier [CDS] 29-Jul-2020