2011MNRAS.418L.104Z


Query : 2011MNRAS.418L.104Z

2011MNRAS.418L.104Z - Mon. Not. R. Astron. Soc., 418, L104-L108 (2011/November-3)

The Hubble Space Telescope colours of high-redshift population III galaxies with strong Lyα emission.

ZACKRISSON E., INOUE A.K., RYDBERG C.-E. and DUVAL F.

Abstract (from CDS):

Population III (pop III) galaxies, made partly or exclusively of metal-free stars, are predicted to exist at high redshifts and may produce very strong Lyα emission. A substantial fraction of these Lyα photons are likely absorbed in the intergalactic medium at z > 6, but recent simulations suggest that significant Lyα emission may be detectable up to z ≈ 8.5, i.e. well into the reionization epoch. Here, we argue that high-redshift pop III galaxies with strong Lyα emission can be identified in Hubble Space Telescope imaging data because of their unusual colours. We quantify this effect in some of the filters used in Y-band dropout searches for galaxies at z ≈ 8 and find that pop III galaxies with high Lyα fluxes may exhibit much bluer J-H colours at z ≈ 8–10 than any normal type of galaxy at these redshifts. This colour signature can arise even if pop III stars account for as little as ∼ 10–3 to 10–2 of the stellar mass in these galaxies. Some of the anomalously blue objects reported in current Y-band dropout samples do in fact meet the colour criteria for Lyα-emitting pop III galaxies.

Abstract Copyright: 2011 The Authors Monthly Notices of the Royal Astronomical Society2011 RAS

Journal keyword(s): stars: Population III - galaxies: high-redshift - dark ages, reionization, first stars

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 JADES-GS+053.16556-27.77266 EmG 03 32 39.728 -27 46 21.33   31.1568       ~ 18 0

Query : 2011MNRAS.418L.104Z

Basic data :
JADES-GS+053.16556-27.77266 -- Emission-line galaxy
Other object types:
otypes_help
G (2011ApJ,[ADW2016b],...), EmG (2023ApJS), NIR (JADES)
ICRS coord. (ep=J2000) :
03 32 39.728 -27 46 21.33 (Optical) [ 90 90 0 ] B 2015AJ....150...31R
FK4 coord. (ep=B1950 eq=1950) :
03 30 34.152 -27 56 26.00 [ 90 90 0 ]
Gal coord. (ep=J2000) :
223.523519 -54.389352 [ 90 90 0 ]
Radial velocity / Redshift / cz :
V(km/s) 291090 [~] / z(emission) 7.240 [~] / cz 2170497 [~]
   (Opt) C 2024A&A...683A.238J
Fluxes (4) :
B (AB) 31.1568 [0.5287] B 2015AJ....150...31R
J (AB) 28.3675 [0.0877] B 2015AJ....150...31R
H (AB) 28.4547 [0.0945] B 2015AJ....150...31R
z (AB) 31.0954 [0.6794] B 2015AJ....150...31R
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Identifiers (15) :
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JADES-GS+053.16556-27.77266 [ADW2016b] ID36 [FPG2010] 515 [OBI2010] UDFz-39736214
JADES-GS NC 131752 [BIO2011] UDFz-39726213 [MDB2013] UDF12-3973-6214 [RTG2015] 9224
JADES-GS NS 9886 [BIO2015] XDFZ-2397246213 [MDC2010] 2502 [YWH2010] zdrop-A057
JADES-GS NS 30142600 [BWE2010] zD10 [MDD2011] HUDF 2641

References (18 between 1850 and 2026) (Total 18)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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