Highlights

An EU-funded Design Study for the Atacama Large Aperture Submillimeter telescope (AtLAST) is about to start

“Towards an Atacama Large Aperture Submillimeter Telescope”, in short AtLAST, is a three years long design study for a new astronomical sub-millimetre observatory. Our project paves the way for building the largest single-dish sub-millimetre telescope in the world, which will deliver the deepest and widest maps of the sky ever obtained at these wavelengths. Read the full article here.


See also this press release by the UK Research and Innovation (UKRI).

The EU project will start in 2021. A proper website is coming soon. Meanwhile, we are collecting emails of potential external collaborators. If you are interest in AtLAST, use this form.

Cicone et al. (2020, A&A)

We found an exceptional boost of the CN/CO(1-0) line luminosity ratio in the massive molecular outflow of Mrk231, suggesting that the outflow material is exposed to a strong UV field. Additionally, we spectrally resolved the high-velocity HCN and HCO+(1-0) line wings into several narrow sub-structures with velocity dispersions of ~7-20 km/s, which we interpret as individual dense clumps entrained in the outflow. ADS link to the article.

Sirressi, Cicone, Severgnini et al. (2019, MNRAS)

Using ALMA CO(1-0) observations we ruled out the presence of a momentum-boosted molecular outflow in MCG-03-58-007, which hosts an extremely powerful X-ray ultra fast outflow. The residual emission shown in the figure is obtained by subtracting the rotation of the main disk from the ALMA data. The favoured interpretation of the residual CO emission in MCG-03-58-007 is a biconical molecular outflow, whose momentum rate is comparable to that of the X-ray outflow. Alternatively, the residuals may trace a circumnuclear disk (CND), which however would be a factor 10-100 larger in size and mass than typical CNDs observed in local Seyferts so far. ADS link to the article.

Cicone et al. (2019, Astro2020 Science WP)

Traditionally the circumgalactic medium (CGM) was thought to consist of warm and hot gas, but recent breakthroughs are presenting a new scenario according to which an important fraction of its mass may reside in the cold atomic and molecular phase. Such cold CGM, especially in local galaxies where its projected size is expected to be of several arcminutes, cannot be imaged by interferometers due to spatial scale filtering of large-scale structures. The only way to probe the multiphase CGM including its coldest component is through a large (e.g. 50-m class) single dish (sub-)mm telescope. This issue is illustrated in the figure, which shows the expected molecular CGM of a star forming galaxy at z = 0.02 as seen by different (sub-)mm facilities after 10 hours of observations. Full white paper available at this link.

Cicone et al. (2018, ApJ)

ALMA observations of the neutral Carbon line ([CI]1-0) in NGC6240 shed light on the state of the gas entrained in the massive molecular outflow, hence allowing us to constrain its extreme energetics. Furthermore, the high-resolution ALMA [CI] images surprisingly reveal that the outflow is launched between the two AGNs rather than from either of the two. ADS link to the article.

Severgnini, Cicone et al. (2018, MNRAS)

The 123-month Swift-BAT monitoring of the nearby Seyfert galaxy MCG+11-11-032 reveals a modular behaviour with peaks and dips occurring almost every 25 months. Under the hypothesis of an SMBH pair, such variability would imply a small sub-pc separation with an orbital velocity of ~0.06c. This value is in remarkable agreement with the energy offset of the two FeK emission lines detected in the Swift XRT spectrum of this source.

ADS link to the article.