2013A&A...556A...5B

Query : 2013A&A...556A...5B

2013A&A...556A...5B - Astronomy and Astrophysics, volume 556A5-5 (2013/8-1)

Effects of Lyman-alpha scattering in the IGM on clustering statistics of Lyman-alpha emitters.

BEHRENS C. and NIEMEYER J.

Abstract (from CDS):

We investigate the correlations between the observed fraction of Lyman-alpha (Lyα) emission from star-forming galaxies and the large-scale structure by post-processing snapshots of a large, high-resolution hydrodynamical simulation with a Lyα radiative transfer code at redshifts z=4, 3, 2. We find correlations of the observed fraction with density, density gradient along the line of sight, velocity, and velocity gradient along the line of sight, all within the same order of magnitude (tens of percent). Additionally, a correlation with the angular momentum of the dark matter halo is detected. In contrast to a previous study, we find no significant deformation of the two-point correlation function due to selection effects from radiative transfer in the intergalactic medium within the limited statistics of the simulation volume.

Abstract Copyright: ∼

Journal keyword(s): large-scale structure of Universe - radiative transfer - galaxies: high-redshift - intergalactic medium

CDS comments: In ref list Verhamme et al. 2012, A&A, 543, A13 is a misprint for Verhamme et al. 2012, A&A, 546, A111.

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	V* V2457 Ori	Or*	05 35 26.97000	-05 09 54.4644					18.858	~	166	0

Query : 2013A&A...556A...5B

Basic data :

V* V2457 Ori -- Orion Variable

Y*O (2012AJ,HOPS,...), IR (2014ApJ,2MASSI,...), V* (2009A&A,V*,...), smm (JCMTSE,JCMTSF,...), cor (2017A&A,[KSS2017]), * ([H97b],[KPM2006]), Rad ([LSK98],[RRC99]), NIR (2MASS,VISION), MIR (WISEA,WISE), Or* (2017ARep)

05 35 26.97000 -05 09 54.4644 (Near-IR) [ 60 60 90 ] C 2003yCat.2246....0C

05 32 59.25265 -05 11 47.0309 [ 60 60 90 ]

208.81950224 -19.24349324 [ 60 60 90 ]

0.047 0.077 ~ (mm) E 2017A&A...600A.141K

I 18.858 [0.025] D 2009A&A...502..883R

J 15.193 [0.048] C 2003yCat.2246....0C

H 14.7830 [0.021] C 2019A&A...622A.149G

K 13.1050 [0.011] C 2019A&A...622A.149G

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`2MASS J05352697-0509544`	`TIC 427393744`	`WISE J053527.04-050955.5`	`[MGM2012] 2293`
`HOPS 64`	`TKK J05352701-0509544`	`[CHS2001] 10255`	`[MWZ90] OMC-2 FIR 4`
`ISOY J053526.99-050954.3`	`TKK 835`	`[H97b] 20951`	`[NCM2003] MIR 24`
`JCMTSE J053526.8-050956`	*`V V2457 Ori`**	`[KPM2006] 127`	`[RRC99] VLA 12`
`JCMTSF J053526.8-050956`	`VISION J05352698-0509542`	`[KSS2017] 24`	`[TSO2008] 29`
`2MASSI J0535269-050954`	`WISEA J053527.04-050955.5`	`[LSK98] 23`	`[TSO2008] J053527-051002`

References (166 between 1850 and 2026) (Total 166)
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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2MASS J05352697-0509544 2MASSI J0535269-050954 V* V2457 Ori WISEA J053527.04-050955.5 WISE J053527.04-050955.5

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