A Multiwavelength Study of ELAN Environments (AMUSE$^2$). Mass budget,
  satellites spin alignment and gas infall in a massive $z\sim3$ quasar host
  halo
  The systematic targeting of extended Ly$\alpha$ emission around high-redshift
quasars resulted in the discovery of rare and bright Enormous Ly$\alpha$
Nebulae (ELANe) associated with multiple active galactic nuclei (AGN). We here
initiate "a multiwavelength study of ELAN environments" (AMUSE$^2$) focusing on
the ELAN around the $z\sim3$ quasar SDSS J1040+1020, a.k.a. the Fabulous ELAN.
We report on VLT/HAWK-I, APEX/LABOCA, JCMT/SCUBA-2, SMA/850$\mu$m, ALMA/CO(5-4)
and 2mm observations and compare them to previously published VLT/MUSE data.
The continuum and line detections enable a first estimate of the star-formation
rates, dust, stellar and molecular gas masses in four objects associated with
the ELAN (three AGNs and one Ly$\alpha$ emitter), confirming that the quasar
host is the most star-forming (${\rm SFR}\sim500$ M$_\odot$ yr$^{-1}$) and
massive galaxy ($M_{\rm star}\sim10^{11}$ M$_{\odot}$) in the system, and thus
can be assumed as central. All four embedded objects have similar molecular gas
reservoirs ($M_{\rm H_2}\sim10^{10}$ M$_{\odot}$), resulting in short depletion
time scales. This fact together with the estimated total dark-matter halo mass,
$M_{\rm DM}=(0.8-2)\times10^{13}$ M$_{\odot}$, implies that this ELAN will
evolve into a giant elliptical galaxy. Consistently, the constraint on the
baryonic mass budget for the whole system indicates that the majority of
baryons should reside in a massive warm-hot reservoir (up to $10^{12}$
M$_{\odot}$), needed to complete the baryons count. Additionally, we discuss
signatures of gas infall on the compact objects as traced by Ly$\alpha$
radiative transfer effects and the evidence for the alignment between the
satellites' spins and their directions to the central.
