Disentangling the co-evolution of galaxies and supermassive black holes with PRIMA

被引：2

作者：

Bisigello, L. ^{[1
,2
]}

Gruppioni, C. ^{[3
]}

Bolatto, A. ^{[4
]}

Ciesla, L. ^{[5
]}

Pope, A. ^{[6
]}

Armus, L. ^{[7
]}

Smith, J. D. ^{[8
]}

Somerville, R. S. ^{[9
]}

Yung, L. Y. A. ^{[10
]}

Wright, R. J. ^{[11
]}

Bradford, C. M. ^{[13
,14
]}

Glenn, J. ^{[12
]}

Feltre, A. ^{[15
]}

机构：

[1] Ist Radioastron, INAF, Via Piero Gobetti 101, I-40129 Bologna, Italy

[2] Univ Padua, Dipartimento Fis & Astron G Galilei, Via Marzolo 8, I-35131 Padua, Italy

[3] INAF Osservatorio Astrofis & Sci Spazio, Via Gobetti 93-3, I-40129 Bologna, Italy

[4] Univ Maryland, Dept Astron, College Pk, MD 20742 USA

[5] Aix Marseille Univ, CNRS, CNES, LAM, Marseille, France

[6] Univ Massachusetts, Dept Astron, Amherst, MA 01003 USA

[7] CALTECH, IPAC, 1200 E Calif Blvd, Pasadena, CA 91125 USA

[8] Univ Toledo, Ritter Astrophys Res Ctr, Toledo, OH 43606 USA

[9] Flatiron Inst, Ctr Computat Astrophys, 162 5th Ave, New York, NY 10010 USA

[10] Space Telescope Sci Inst, 3700 San Martin Dr, Baltimore, MD 21218 USA

[11] Univ Helsinki, Dept Phys, Gustaf Hallstromin katu 2, Helsinki 00014, Finland

[12] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA

[13] NASA, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA 91011 USA

[14] CALTECH, 1200 Calif Blvd, Pasadena, CA 91125 USA

[15] INAF Osservatorio Astrofisico Arcetri, Largo E Fermi 5, I-50125 Florence, Italy

来源：

ASTRONOMY & ASTROPHYSICS | 2024年 / 689卷

基金：

欧洲研究理事会;

关键词：

surveys; galaxies: active; galaxies: evolution; galaxies: photometry; SPECTRAL ENERGY-DISTRIBUTIONS; QUASAR LUMINOSITY FUNCTION; ACTIVE GALACTIC NUCLEI; ULTRALUMINOUS INFRARED GALAXIES; SPITZER-SPACE-TELESCOPE; FINE-STRUCTURE EMISSION; OBSCURED STAR-FORMATION; SEMIANALYTIC FORECASTS; MOLECULAR OUTFLOWS; STELLAR MASS;

D O I：

10.1051/0004-6361/202450529

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The most active phases of star formation and black hole accretion are strongly affected by dust extinction, making far-infrared (FIR) observations the best way to disentangle and study the co-evolution of galaxies and super massive black holes. The plethora of fine-structure lines and emission features from dust and ionised and neutral atomic and warm molecular gas in the rest-frame mid-infrared (MIR) and FIR provide unmatched diagnostic opportunities to determine the properties of gas and dust, measure gas-phase metallicities, and map cold galactic outflows in even the most obscured galaxies. By combining multi-band photometric surveys with low- and high-resolution FIR spectroscopy, the PRobe far-Infrared Mission for Astrophysics (PRIMA), a 1.8 m diameter, cryogenically cooled FIR observatory currently at the conception stage, will revolutionise the field of galaxy evolution by taking advantage of this IR toolkit to find and study dusty galaxies across galactic time. In this work, we make use of the phenomenological simulation SPRITZ and the Santa Cruz semi-analytical model to describe how a moderately deep multi-band PRIMA photometric survey can easily reach beyond previous IR missions to detect and study galaxies down to 10(11) L-circle dot beyond cosmic noon and at least up to z = 4, even in the absence of gravitational lensing. By decomposing the spectral energy distribution (SED) of these photometrically selected galaxies, we show that PRIMA can be used to accurately measure the relative AGN power, the mass fraction contributed by polycyclic aromatic hydrocarbons (PAHs), and the total IR luminosity. At the same time, spectroscopic follow up with PRIMA will allow us to trace both the star formation and black hole accretion rates (SFRs and BHARs), the gas-phase metallicities, and the mass-outflow rates of cold gas in hundreds to thousands of individual galaxies to z = 2.

引用

页数：16

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