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J/A+A/608/A8        MUSE Hubble Ultra Deep Field Survey. VIII  (Leclercq+, 2017)

The MUSE Hubble Ultra Deep Field Survey: VIII. Extended Lyman-α haloes around high-z star-forming galaxies. Leclercq F., Bacon R., Wisotzki L., Mitchell P., Garel T., Verhamme A., Blaizot J., Hashimoto T., Herenz E.C., Conseil S., Cantalupo S., Inami H., Contini T., Richard J., Maseda M., Schaye J., Marino R.A., Akhlaghi M., Brinchmannand J., Carollo M. <Astron. Astrophys. 608, A8 (2017)> =2017A&A...608A...8L (SIMBAD/NED BibCode)
ADC_Keywords: Galaxies, optical; Diffuse clouds; Spectrophotometry Keywords: galaxies: high-redshift - galaxies: formation - galaxies: evolution - cosmology: observations Abstract: We present the detection of 145 extended Lyman-alpha haloes around individual high-z (3-6) star-forming galaxies in the UDF field observed by MUSE/VLT. Using a 2D, two-component (continuum-like and halo) decomposition of Lyman-alpha emission assuming circular exponential distributions, we measure scale lengths and luminosities of Lyman-alpha haloes. Description: Fitted parameters, measurements and general properties of the 145 Lyman-alpha emitters surrounded by a halo in the MUSE UDF data. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file tableb1.dat 136 184 Properties the 145 Lyman-alpha emitters surrounded by a halo detected in the MUSE UDF data
See also: J/A+A/608/A2 : MUSE Hubble Ultra Deep Field Survey. II. (Inami+, 2017) Byte-by-byte Description of file: tableb1.dat
Bytes Format Units Label Explanations
1- 4 I4 --- MUSE Source identifier in Inami et al., 2017, Cat. J/A+A/608/A2 (I17) 6 I1 --- Field [1/2] Field: 1 for udf-10 and 2 for mosaic (1) 8- 16 F9.6 deg RAdeg Right ascension (J2000) in I17 18- 27 F10.6 deg DEdeg Declination (J2000) in I17 29- 32 F4.2 --- zMuse MUSE redshift in I17 34- 37 F4.1 mag F775W ?=- Continuum AB magnitude in the HST filter band F775W used for the study (see section 3.1.2) from I17 39- 43 F5.2 mag mUVMAG ?=- Opposite of the absolute far-UV magnitude (-UVMAG) 45- 50 F6.2 10-21W/m2 FLya Total Lyα flux (in 10-18erg/cm2/s) 52- 56 F5.2 10-21W/m2 e_FLya Error on FLya 58- 62 F5.2 [10-7W] logLLya Logarithm of the Lyα luminosity 64- 68 F5.1 0.1nm EWLya ?=- Lyα rest-frame equivalent width (in Angstroem) 70- 73 F4.1 kpc RCoG CoG method radius in physical kpc 75 A1 --- l_RScont Upper limit flag on RScont (2) 76- 80 F5.3 kpc RScont Exponential scale length of the UV continuum 82- 87 F6.3 kpc e_RScont ?=-1 Error on RScont (If negative RScont is an upper limit) 89 A1 --- l_RShalo Upper limit flag on RShalo 90- 95 F6.3 kpc RShalo Exponential scale length of the Lyα halo component 97-102 F6.3 kpc e_RShalo ?=-1 Error on RShalo (If negative RShalo is an upper limit) 104-108 F5.2 10-21W/m2 Fcont Integrated flux of the 'continuum-like' Lyman-alpha component 110-113 F4.2 10-21W/m2 e_Fcont Error on Fcont 115-119 F5.2 10-21W/m2 Fhalo Integrated flux of the 'Halo' Lyman-alpha component 121-124 F4.2 10-21W/m2 e_Fhalo Error on Fhalo 126-132 F7.5 --- 1-P0 Confidence level that the scale lengths (RScont and RShalo) are not identical, P0 being the probability of the two scale lengths to be identical 134-136 I3 km/s FWHM0 ?=- Rest-frame full width at half maximum of the Lyman-alpha line
Note (1): Field as follows: 1 = UDF-10 2 = MOSAIC Note (2): Upper limits are given if the object is considered as a point source.
Acknowledgements: Floriane Leclercq, floriane.leclercq(at)univ-lyon1.fr References: Bacon et al., Paper I 2017A&A...608A...1B Inami et al., Paper II 2017A&A...608A...2I, Cat. J/A+A/608/A2 Brinchmann et al., Paper III 2017A&A...608A...3B Maseda et al., Paper IV 2017A&A...608A...4M Guerou et al., Paper V 2017A&A...608A...5G Drake et al., Paper VI 2017A&A...608A...6D Finley et al., Paper VII 2017A&A...608A...7F Ventou et al., Paper IX 2017A&A...608A...9V Hashimoto et al., Paper X 2017A&A...608A..10H
(End) Patricia Vannier [CDS] 08-Nov-2017
The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line

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