Pith. sign in

REVIEW 3 cited by

ESO-Athena Synergy White Paper

Not yet reviewed by Pith; the record is open.

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 1705.06064 v1 pith:KNZYEWFX submitted 2017-05-17 astro-ph.HE astro-ph.COastro-ph.GAastro-ph.IMastro-ph.SR

classification astro-ph.HEastro-ph.COastro-ph.GAastro-ph.IMastro-ph.SR
keywords athenasciencefacilitiessynergyalmascientificuniversewhite
verification ladder T0 review T1 audit T2 compute T3 formal

Signed reviews

No signed human review yet.

0 comments
read the original abstract

The Advanced Telescope for High ENergy Astrophysics (Athena) is the X-ray observatory mission selected by ESA within its Cosmic Vision 2015-2025 programme to address the Hot and Energetic Universe scientific theme. The ESO-Athena Synergy Team (EAST) has been tasked to single out the potential scientific synergies between Athena and optical/near-infrared (NIR) and sub/mm ground based facilities, in particular those of ESO (i.e., the VLT and ELT, ALMA and APEX), by producing a White Paper to identify and develop the: 1. needs to access ESO ground-based facilities to achieve the formulated Athena science objectives; 2. needs to access Athena to achieve the formulated science objectives of ESO facilities contemporary to Athena; 3. science areas where the synergetic use of Athena and ESO facilities in the late 2020s will result in scientific added value. Community input to the process happened primarily via a dedicated ESO - Athena Synergy Workshop that took place on Sept. 14 - 16, 2016 at ESO, Garching. This White Paper presents the results of the EAST's work, sorted by synergy area, and deals with the following topics: 1. the Hot Universe: Early groups and clusters and their evolution, Physics of the Intracluster medium, Missing baryons in cosmic filaments; 2. the Energetic Universe: Supermassive black hole (SMBH) history, SMBH accretion disks, Active Galactic Nuclei feedback - Molecular outflows, Ultra-fast outflows, Accretion Physics, Transient Science; 3. Observatory Science: Star Formation, Stars. It then discusses the optical-NIR-sub-mm perspective by providing details on VLT/MOONS, the E-ELT instruments, in particular the MOS, VISTA/4MOST, the ESO and ALMA archives, future ALMA and ESO developments, and finally the (likely) ESO - Athena astronomical scene in the 2020s. (abridged)

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Multi-messenger tests of gravity with weakly lensed gravitational waves

    astro-ph.CO 2019-08 conditional novelty 6.0 of 10

    The authors show that cross-correlating GW source convergence with CMB lensing can measure a GR prediction (identical geodesics for GWs and photons) at high SNR for LISA-class detectors.

  2. Slow and fat: low-spin SMBHs are more massive

    astro-ph.GA 2019-08 conditional novelty 5.0 of 10

    Low-spin supermassive black holes keep growing during the gas-clearing phase because their low radiative efficiency makes feedback less effective, so they end up more massive than high-spin ones at fixed galaxy veloci...

  3. The NewAthena mission concept in the context of the next decade of X-ray astronomy

    astro-ph.IM 2025-01 conditional novelty 4.0 of 10

    NewAthena, a reformulation of the Athena mission concept, is proposed as the next large X-ray observatory to deliver order-of-magnitude gains in sensitivity and spectroscopy across many areas of astrophysics.

Pith tools