Submillimetre galaxies represent a rapid growth phase of both star formation and massive galaxies. Mapping SMGs in galaxy protoclusters provides key insights into where and how these extreme starbursts take place in connections with the assembly of the large-scale structure in the early Universe. We search for SMGs at 850 μ m using JCMT/SCUBA-2 in two massive protoclusters at z = 2.24, BOSS1244 and BOSS1542, and detect 43 and 54 sources with S850 > 4 mJy at the 4σ level within an effective area of 264 arcmin2, respectively. We construct the intrinsic number counts and find that the abundance of SMGs is 2.0 ± 0.3 and 2.1 ± 0.2 times that of the general fields, confirming that BOSS1244 and BOSS1542 contain a higher fraction of dusty galaxies ...
High-redshift protoclusters are ideal places to study the formation of the largest structures in the...
We present detailed observations of a z ~ 1.99 cluster of submillimeter galaxies (SMGs), discovered ...
Context. Protoclusters are progenitors of galaxy clusters and they serve as an important key in stud...
Submillimetre galaxies represent a rapid growth phase of both star formation and massive galaxies. M...
There is controversy in the literature regarding whether distant, massive, and dusty starbursts sele...
There is controversy in the literature regarding whether distant, massive, and dusty starbursts sele...
International audienceThree billion years after the big bang (at redshift z = 2), half of the most m...
We present APEX LABOCA 870 μm observations of the field around the high-redshift radio gal...
Three billion years after the big bang (at redshift z = 2), half of the most massive galaxies were a...
We investigate the relationship between the quenching of star formation and the structural transform...
We present APEX LABOCA 870 μm observations of the field around the high-redshift radio galaxy MRC113...
I will next describe an ambitious survey for early structures forming in the Universe, which represe...
Overdensity of galaxies at high-z are often suspected to be progenitors of local massive clusters, h...
Radio galaxies have been used quite successfully as protocluster tracers. However, because they are ...
Massive galaxy overdensities at the peak epoch of cosmic star formation provide ideal testbeds for t...
High-redshift protoclusters are ideal places to study the formation of the largest structures in the...
We present detailed observations of a z ~ 1.99 cluster of submillimeter galaxies (SMGs), discovered ...
Context. Protoclusters are progenitors of galaxy clusters and they serve as an important key in stud...
Submillimetre galaxies represent a rapid growth phase of both star formation and massive galaxies. M...
There is controversy in the literature regarding whether distant, massive, and dusty starbursts sele...
There is controversy in the literature regarding whether distant, massive, and dusty starbursts sele...
International audienceThree billion years after the big bang (at redshift z = 2), half of the most m...
We present APEX LABOCA 870 μm observations of the field around the high-redshift radio gal...
Three billion years after the big bang (at redshift z = 2), half of the most massive galaxies were a...
We investigate the relationship between the quenching of star formation and the structural transform...
We present APEX LABOCA 870 μm observations of the field around the high-redshift radio galaxy MRC113...
I will next describe an ambitious survey for early structures forming in the Universe, which represe...
Overdensity of galaxies at high-z are often suspected to be progenitors of local massive clusters, h...
Radio galaxies have been used quite successfully as protocluster tracers. However, because they are ...
Massive galaxy overdensities at the peak epoch of cosmic star formation provide ideal testbeds for t...
High-redshift protoclusters are ideal places to study the formation of the largest structures in the...
We present detailed observations of a z ~ 1.99 cluster of submillimeter galaxies (SMGs), discovered ...
Context. Protoclusters are progenitors of galaxy clusters and they serve as an important key in stud...