2014
DOI: 10.1051/0004-6361/201423771
|View full text |Cite
|
Sign up to set email alerts
|

An excess of dusty starbursts related to the Spiderweb galaxy

Abstract: We present APEX LABOCA 870 μm observations of the field around the high-redshift radio galaxy MRC1138−262 at z = 2.16. We detect 16 submillimeter galaxies (SMGs) in this ∼140 arcmin 2 bolometer map with flux densities in the range 3-11 mJy. The raw number counts indicate a density of SMGs that is up to four times that of blank field surveys. Based on an exquisite multiwavelength database, including VLA 1.4 GHz radio and infrared observations, we investigate whether these sources are members of the protocluster… Show more

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1
1

Citation Types

31
211
1
1

Year Published

2016
2016
2021
2021

Publication Types

Select...
7

Relationship

2
5

Authors

Journals

citations
Cited by 159 publications
(244 citation statements)
references
References 112 publications
(244 reference statements)
31
211
1
1
Order By: Relevance
“…The identification of thisz 2.1 structure, along with previous findings of DSFG-or AGN-rich structures in known protoclusters (Tamura et al 2009;Digby-North et al 2010;Dannerbauer et al 2014;Smail et al 2014), demonstrate that the excess of these rare systems indeed traces bona-fide overdensities (of mass) and protoclusters (also see Casey et al 2015). In fact, searching for the overdensities of DSFGs or AGNs can be an efficient probe 15 of large structure across several tens of Mpc at  z 2, and there is potentially a large population of such DSFG-rich protoclusters as revealed by Herschel and Planck observations (Planck Collaboration et al 2015).…”
supporting
confidence: 75%
See 2 more Smart Citations
“…The identification of thisz 2.1 structure, along with previous findings of DSFG-or AGN-rich structures in known protoclusters (Tamura et al 2009;Digby-North et al 2010;Dannerbauer et al 2014;Smail et al 2014), demonstrate that the excess of these rare systems indeed traces bona-fide overdensities (of mass) and protoclusters (also see Casey et al 2015). In fact, searching for the overdensities of DSFGs or AGNs can be an efficient probe 15 of large structure across several tens of Mpc at  z 2, and there is potentially a large population of such DSFG-rich protoclusters as revealed by Herschel and Planck observations (Planck Collaboration et al 2015).…”
supporting
confidence: 75%
“…If we define potential cluster members using the FoF analysis instead of a fixed 10′ aperture, then there are also nine DSFGs (four of them are X-ray luminous AGNs) included in the large-scale structure. Such an excess of DSFGs and AGNs within and around the ZFIRE clusters is comparable to several DSFG-and AGN-rich structures at  z 1.5 (Chapman et al 2009;Tamura et al 2009;Digby-North et al 2010;Dannerbauer et al 2014;Smail et al 2014;Casey et al 2015;Ma et al 2015, see a compilation by Casey 2016).…”
Section: Distribution Of Sfgs and Rare Sourcesmentioning
confidence: 60%
See 1 more Smart Citation
“…SCUBA and LABOCA maps (Stevens et al 2003;Dannerbauer et al 2014), but those extensions were on a much larger scale than the separation seen in Fig. 1.…”
Section: The Hzrgmentioning
confidence: 85%
“…Many of these galaxies are clumpy and star-forming (Pentericci et al 1998;Miley et al 2006;Dannerbauer et al 2014). Hatch et al (2009) predict that most of the satellite galaxies within 150 kpc will merge with the central HzRG and that the final merger galaxy will contain very little gas owing to the high star formation rate (SFR) of the satellite galaxies.…”
Section: Introductionmentioning
confidence: 99%