Imperial College London
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Dr Clements

Faculty of Natural Sciences, Department of Physics

Reader in Astrophysics
 
 
 
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Contact

 

+44 (0)20 7594 7693d.clements

 
 
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Location

 

1011Blackett LaboratorySouth Kensington Campus

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Summary

 

Publications

Citation

BibTex format

@article{Spinoglio:2017:10.1017/pasa.2017.48,
author = {Spinoglio, L and Alonso-Herrero, A and Armus, L and Baes, M and Bernard-Salas, J and Bianchi, S and Bocchio, M and Bolatto, A and Bradford, C and Braine, J and Carrera, FJ and Ciesla, L and Clements, DL and Dannerbauer, H and Doi, Y and Efstathiou, A and Egami, E and Fernandez-Ontiveros, JA and Ferrara, A and Fischer, J and Franceschini, A and Gallerani, S and Giard, M and Gonzalez-Alfonso, E and Gruppioni, C and Guillard, P and Hatziminaoglou, E and Imanishi, M and Ishihara, D and Isobe, N and Kaneda, H and Kawada, M and Kohno, K and Kwon, J and Madden, S and Malkan, MA and Marassi, S and Matsuhara, H and Matsuura, M and Miniutti, G and Nagamine, K and Nagao, T and Najarro, F and Nakagawa, T and Onaka, T and Oyabu, S and Pallottini, A and Piro, L and Pozzi, F and Rodighiero, G and Roelfsema, P and Sakon, I and Santini, P and Schaerer, D and Schneider, R and Scott, D and Serjeant, S and Shibai, H and Smith, J-DT and Sobacchi, E and Sturm, E and Suzuki, T and Vallini, L and van, der Tak},
doi = {10.1017/pasa.2017.48},
journal = {PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA},
title = {Galaxy Evolution Studies with the SPace IR Telescope for Cosmology and Astrophysics (SPICA): The Power of IR Spectroscopy},
url = {http://dx.doi.org/10.1017/pasa.2017.48},
volume = {34},
year = {2017}
}
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RIS format (EndNote, RefMan)

TY  - JOUR
AB  - IR spectroscopy in the range 12–230 μm with the SPace IR telescope for Cosmology and Astrophysics (SPICA) will reveal the physical processes governing the formation and evolution of galaxies and black holes through cosmic time, bridging the gap between the James Webb Space Telescope and the upcoming Extremely Large Telescopes at shorter wavelengths and the Atacama Large Millimeter Array at longer wavelengths. The SPICA, with its 2.5-m telescope actively cooled to below 8 K, will obtain the first spectroscopic determination, in the mid-IR rest-frame, of both the star-formation rate and black hole accretion rate histories of galaxies, reaching lookback times of 12 Gyr, for large statistically significant samples. Densities, temperatures, radiation fields, and gas-phase metallicities will be measured in dust-obscured galaxies and active galactic nuclei, sampling a large range in mass and luminosity, from faint local dwarf galaxies to luminous quasars in the distant Universe. Active galactic nuclei and starburst feedback and feeding mechanisms in distant galaxies will be uncovered through detailed measurements of molecular and atomic line profiles. The SPICA’s large-area deep spectrophotometric surveys will provide mid-IR spectra and continuum fluxes for unbiased samples of tens of thousands of galaxies, out to redshifts of z ~ 6.
AU  - Spinoglio,L
AU  - Alonso-Herrero,A
AU  - Armus,L
AU  - Baes,M
AU  - Bernard-Salas,J
AU  - Bianchi,S
AU  - Bocchio,M
AU  - Bolatto,A
AU  - Bradford,C
AU  - Braine,J
AU  - Carrera,FJ
AU  - Ciesla,L
AU  - Clements,DL
AU  - Dannerbauer,H
AU  - Doi,Y
AU  - Efstathiou,A
AU  - Egami,E
AU  - Fernandez-Ontiveros,JA
AU  - Ferrara,A
AU  - Fischer,J
AU  - Franceschini,A
AU  - Gallerani,S
AU  - Giard,M
AU  - Gonzalez-Alfonso,E
AU  - Gruppioni,C
AU  - Guillard,P
AU  - Hatziminaoglou,E
AU  - Imanishi,M
AU  - Ishihara,D
AU  - Isobe,N
AU  - Kaneda,H
AU  - Kawada,M
AU  - Kohno,K
AU  - Kwon,J
AU  - Madden,S
AU  - Malkan,MA
AU  - Marassi,S
AU  - Matsuhara,H
AU  - Matsuura,M
AU  - Miniutti,G
AU  - Nagamine,K
AU  - Nagao,T
AU  - Najarro,F
AU  - Nakagawa,T
AU  - Onaka,T
AU  - Oyabu,S
AU  - Pallottini,A
AU  - Piro,L
AU  - Pozzi,F
AU  - Rodighiero,G
AU  - Roelfsema,P
AU  - Sakon,I
AU  - Santini,P
AU  - Schaerer,D
AU  - Schneider,R
AU  - Scott,D
AU  - Serjeant,S
AU  - Shibai,H
AU  - Smith,J-DT
AU  - Sobacchi,E
AU  - Sturm,E
AU  - Suzuki,T
AU  - Vallini,L
AU  - van,der Tak F
AU  - Vignali,C
AU  - Yamada,T
AU  - Wada,T
AU  - Wang,L
DO  - 10.1017/pasa.2017.48
PY  - 2017///
SN  - 1323-3580
TI  - Galaxy Evolution Studies with the SPace IR Telescope for Cosmology and Astrophysics (SPICA): The Power of IR Spectroscopy
T2  - PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA
UR  - http://dx.doi.org/10.1017/pasa.2017.48
UR  - http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000419925000001&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=1ba7043ffcc86c417c072aa74d649202
UR  - http://hdl.handle.net/10044/1/61101
VL  - 34
ER  -
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