2017
DOI: 10.1017/pasa.2017.46
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Feedback and Feeding in the Context of Galaxy Evolution withSPICA: Direct Characterisation of Molecular Outflows and Inflows

Abstract: A far-infrared observatory such as the SPace Infrared telescope for Cosmology and Astrophysics (SPICA), with its unprecedented spectroscopic sensitivity, would unveil the role of feedback in galaxy evolution during the last ∼ 10 Gyr of the Universe (z = 1.5 − 2), through the use of far-and mid-infrared molecular and ionic fine structure lines that trace outflowing and infalling gas. Outflowing gas is identified in the far-infrared through P-Cygni line shapes and absorption blueshifted wings in molecular lines … Show more

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Cited by 15 publications
(8 citation statements)
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References 146 publications
(290 reference statements)
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“…The line and continuum measurements of strongly lensed galaxies given by George (2015) were corrected using the gravitational magnifications, µ, estimated by Ferkinhoff et al (2014), while those by Gullberg et al (2015) were corrected using the magnification estimates from Hezaveh et al (2013) and Spilker et al (2016), available for 17 out of the 20 sources; for the other three sources we used the median value µ median = 7.4.…”
Section: Correlations Between Continuum and Line Luminositymentioning
confidence: 99%
See 1 more Smart Citation
“…The line and continuum measurements of strongly lensed galaxies given by George (2015) were corrected using the gravitational magnifications, µ, estimated by Ferkinhoff et al (2014), while those by Gullberg et al (2015) were corrected using the magnification estimates from Hezaveh et al (2013) and Spilker et al (2016), available for 17 out of the 20 sources; for the other three sources we used the median value µ median = 7.4.…”
Section: Correlations Between Continuum and Line Luminositymentioning
confidence: 99%
“…George (2015), for all three lines; Brisbin et al(2015)and Farrah et al (2013), for the [O I] 63.18 and [C II] 157.7 µm lines; and Oteo et al (2016), Gullberg et al (2015), Schaerer et al (2015), Yun et al (2015), and Magdis et al…”
mentioning
confidence: 96%
“…These questions, their background science, and how SPICA would help resolve them, are discussed in much more detail in a dedicated series of papers (Spinoglio et al 2017;Fernández-Ontiveros et al 2017;González-Alfonso et al 2017;Gruppioni et al 2017;Kaneda et al 2017;E. Egami et al, in preparation;van der Tak et al 2017;P.…”
Section: The Power Of Infrared Diagnosticsmentioning
confidence: 99%
“…For example, a 2 000-h SAFARI survey will obtain low-resolution (LR; R = 300) spectra for over 1 000 galaxies up to z 4 (Spinoglio et al 2017) while a 600-h SMI survey will identify about 50 000 galaxies in a 10 deg 2 area through R = 50-120 spectroscopy of polycyclic aromatic hydrocarbon (PAH) emission features (Kaneda et al 2017). Such data sets will enormously advance our understanding of galaxy/AGN evolution and will shed light on key science topics such as chemical evolution/metal enrichment (Fernández-Ontiveros et al 2017) and molecular outflows/inflows (González-Alfonso et al 2017). Note that the great power of SPICA mainly resides in such spectroscopic observations, especially in the far-infrared (>100 μm), where Herschel/Spectral and Photometric Imaging Receiver (SPIRE) has already achieved confusion-limited broad-band imaging sensitivities with a 3.5-m telescope.…”
Section: Introductionmentioning
confidence: 99%