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20132026
most citedAGN wind scaling relations and the co-evolution of black holes and galaxies

605 citations · 13.7k across the 314 of their papers we have counts for

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Showing 2022Show all

23 papers · 1 filter

astro-ph.GA2022★ 16 cited

Radio jet-ISM interaction and positive radio-mechanical feedback in Abell 1795

Prathamesh D. Tamhane, Brian R. McNamara, Helen R. Russell +8

We present XSHOOTER observations with previous ALMA, MUSE and observations to study the nature of radio-jet triggered star formation and the interaction of radio jets with th…

astro-ph.GA2022★ 28 cited

[CII] halos in ALPINE galaxies: smoking-gun of galactic outflows?

E. Pizzati, A. Ferrara, A. Pallottini +3

ALMA observations have revealed that many high redshift galaxies are surrounded by extended (10-15 kpc) [CII]-emitting halos which are not predicted by even the most advanced zoom-…

astro-ph.GA2022★ 20 cited

Evidence of extended cold molecular gas and dust halos around Extremely Red Quasars with ALMA

J. Scholtz, R. Maiolino, G. C. Jones +1

Large-scale outflows are believed to be an important mechanism in the evolution of galaxies. We can determine the impact of these outflows by studying either current galaxy outflow…

astro-ph.GA2022

Spectroscopic confirmation of four metal-poor galaxies at z=10.3-13.2

Emma Curtis-Lake, Stefano Carniani, Alex Cameron +56

Finding and characterising the first galaxies that illuminated the early Universe at cosmic dawn is pivotal to understand the physical conditions and the processes that led to the…

astro-ph.GA2022★ 274 cited

Identification and properties of intense star-forming galaxies at redshifts z>10

B. E. Robertson, S. Tacchella, B. D. Johnson +53

Surveys with James Webb Space Telescope (JWST) have discovered candidate galaxies in the first 400 Myr of cosmic time. Preliminary indications have suggested these candidate galaxi…

astro-ph.GA2022★ 14 cited

Is the star formation rate in quasars overestimated?

Fabio Di Mascia, Stefano Carniani, Simona Gallerani +4

The large total infrared (TIR) luminosities () observed in quasars are generally converted into high star formation rates ($SFR \gtr…

astro-ph.GA2022★ 14 cited

Evidence for extended gaseous reservoirs around AGN at cosmic noon from ALMA CO(3-2) observations

G. C. Jones, R. Maiolino, C. Circosta +3

Gaseous outflows are key phenomena in the evolution of galaxies, as they affect star formation (either positively or negatively), eject gas from the core or disk, and directly caus…

astro-ph.GA2022★ 44 cited

A new look at the infrared properties of z 5 galaxies

L. Sommovigo, A. Ferrara, S. Carniani +6

Recent ALMA large surveys unveiled the presence of significant dust continuum emission in star-forming galaxies at . Unfortunately, such large programs -- i.e. ALPINE ($z\sim…

astro-ph.GA2022★ 73 cited

Shaken, not blown: the gentle baryonic feedback of nearby starburst dwarf galaxies

A. Marasco, F. Belfiore, G. Cresci +12

Baryonic feedback is expected to play a key role in regulating the star formation of low-mass galaxies by producing galaxy-scale winds associated with mass-loading factors $β\!\sim…

astro-ph.GA2022★ 80 cited

Morpheus Reveals Distant Disk Galaxy Morphologies with JWST: The First AI/ML Analysis of JWST Images

Brant E. Robertson, Sandro Tacchella, Benjamin D. Johnson +21

The dramatic first images with James Webb Space Telescope (JWST) demonstrated its power to provide unprecedented spatial detail for galaxies in the high-redshift universe. Here, we…

astro-ph.GA2022★ 26 cited

Detection of companion galaxies around hot dust-obscured hyper-luminous galaxy W0410-0913

M. Ginolfi, E. Piconcelli, L. Zappacosta +18

The phase transition between galaxies and quasars is often identified with the rare population of hyper-luminous, hot dust-obscured galaxies. Galaxy formation models predict these…

astro-ph.GA2022★ 136 cited

JWST NIRCam+NIRSpec: Interstellar medium and stellar populations of young galaxies with rising star formation and evolving gas reservoirs

Sandro Tacchella, Benjamin D. Johnson, Brant E. Robertson +37

We present an interstellar medium and stellar population analysis of three spectroscopically confirmed galaxies in the ERO JWST NIRCam and JWST NIRSpec data of the SMACS J072…

astro-ph.GA2022★ 22 cited

The black hole and host galaxy growth in an isolated QSO observed with ALMA

R. Tripodi, C. Feruglio, F. Fiore +11

The outstanding mass growth of supermassive black holes (SMBHs) at the Reionisation Epoch and how it is related to the concurrent growth of their host galaxies, poses challenges to…

astro-ph.GA2022★ 88 cited

Dual constraints with ALMA: new [O III] 88 m and dust-continuum observations reveal the ISM conditions of luminous LBGs at

Joris Witstok, Renske Smit, Roberto Maiolino +10

We present new [O III] 88 m observations of five bright Lyman-break galaxies spectroscopically confirmed by ALMA through the [C II] 158 m line, unlike…

astro-ph.GA2022★ 83 cited

First Insights into the ISM at with JWST: Possible Physical Implications of a High [O III]/[O III]

Harley Katz, Aayush Saxena, Alex J. Cameron +15

We present a detailed analysis of the rest-frame optical emission line ratios for three spectroscopically confirmed galaxies at . The galaxies were identified in the James W…

astro-ph.GA2022★ 281 cited

The chemical enrichment in the early Universe as probed by JWST via direct metallicity measurements at z~8

M. Curti, F. D'Eugenio, S. Carniani +30

We analyse the chemical properties of three z~8 galaxies behind the galaxy cluster SMACS J0723.3-7327, observed as part of the Early Release Observations programme of the James Web…

astro-ph.IM2022★ 440 cited

The Science Performance of JWST as Characterized in Commissioning

Jane Rigby, Marshall Perrin, Michael McElwain +623

This paper characterizes the actual science performance of the James Webb Space Telescope (JWST), as determined from the six month commissioning period. We summarize the performanc…

astro-ph.GA2022★ 14 cited

The interstellar medium of high-redshift galaxies: Gathering clues from C III] and [C II] lines

Vladan Markov, Stefano Carniani, Livia Vallini +5

A tight relation between [C II] line luminosity and the star formation rate (SFR) has been observed for local galaxies. At high redshift (z > 5), galaxies instead deviate downwards…

astro-ph.GA2022

Feedback effect on the observable properties of AGN

Fabio Vito, Fabio Di Mascia, Simona Gallerani +4

Active galactic nuclei (AGN) feedback has a major impact onto the supermassive black-hole (SMBH) growth, the properties of the host galaxies, and their cosmic evolution. We investi…

astro-ph.GA2022★ 75 cited

Widespread, strong outflows in XQR-30 quasars at the Reionisation epoch

M. Bischetti, C. Feruglio, V. D'Odorico +23

Luminous quasars powered by accretion onto billion solar mass black holes already exist at the epoch of Reionisation, when the Universe was 0.5-1 Gyr old. These objects likely resi…

astro-ph.GA2022★ 21 cited

Enhanced star formation in quasar companions

Tommaso Zana, Simona Gallerani, Stefano Carniani +5

Quasars powered by supermassive black holes (MBH, ) at are predicted to reside in cosmic over-dense regions. However, observations so far could not confi…

astro-ph.GA2022

The ionizing properties of two bright Ly emitters in the BDF reionized bubble at z=7

M. Castellano, L. Pentericci, G. Cupani +17

We investigate the ionizing properties of the pair of bright Ly emitting galaxies BDF521 and BDF2195 at z=7.012 in order to constrain their contribution to the formation of the…

astro-ph.GA2022★ 99 cited

A survey of high- galaxies: SERRA simulations

A. Pallottini, A. Ferrara, S. Gallerani +10

We introduce SERRA, a suite of zoom-in high-resolution () cosmological simulations including non-equilibrium chemistry and on-the-fly radiative transfer. The outpu…