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{Gruppioni:2017:10.1017/pasa.2017.49,
author = {Gruppioni, C and Ciesla, L and Hatziminaoglou, E and Pozzi, F and Rodighiero, G and Santini, P and Armus, L and Baes, M and Braine, J and Charmandaris, V and Clements, DL and Christopher, N and Dannerbauer, H and Efstathiou, A and Egami, E and Fernandez-Ontiveros, JA and Fontanot, F and Franceschini, A and Gonzalez-Alfonso, E and Griffin, M and Kaneda, H and Marchetti, L and Monaco, P and Nakagawa, T and Onaka, T and Papadopoulos, A and Pearson, C and Perez-Fournon, I and Perez-Gonzalez, P and Roelfsema, P and Scott, D and Serjeant, S and Spinoglio, L and Vaccari, M and van, der Tak F and Vignali, C and Wang, L and Wada, T},
doi = {10.1017/pasa.2017.49},
journal = {PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA},
title = {Tracing the Evolution of Dust Obscured Star Formation and Accretion Back to the Reionisation Epoch with SPICA},
url = {http://dx.doi.org/10.1017/pasa.2017.49},
volume = {34},
year = {2017}
}
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RIS format (EndNote, RefMan)

TY  - JOUR
AB  - Our current knowledge of star formation and accretion luminosity at high redshift (z > 3–4), as well as the possible connections between them, relies mostly on observations in the rest-frame ultraviolet, which are strongly affected by dust obscuration. Due to the lack of sensitivity of past and current infrared instrumentation, so far it has not been possible to get a glimpse into the early phases of the dust-obscured Universe. Among the next generation of infrared observatories, SPICA, observing in the 12–350 µm range, will be the only facility that can enable us to trace the evolution of the obscured star-formation rate and black-hole accretion rate densities over cosmic time, from the peak of their activity back to the reionisation epoch (i.e., 3 < z  6–7), where its predecessors had severe limitations. Here, we discuss the potential of photometric surveys performed with the SPICA mid-infrared instrument, enabled by the very low level of impact of dust obscuration in a band centred at 34 µm. These unique unbiased photometric surveys that SPICA will perform will fully characterise the evolution of AGNs and star-forming galaxies after reionisation.
AU  - Gruppioni,C
AU  - Ciesla,L
AU  - Hatziminaoglou,E
AU  - Pozzi,F
AU  - Rodighiero,G
AU  - Santini,P
AU  - Armus,L
AU  - Baes,M
AU  - Braine,J
AU  - Charmandaris,V
AU  - Clements,DL
AU  - Christopher,N
AU  - Dannerbauer,H
AU  - Efstathiou,A
AU  - Egami,E
AU  - Fernandez-Ontiveros,JA
AU  - Fontanot,F
AU  - Franceschini,A
AU  - Gonzalez-Alfonso,E
AU  - Griffin,M
AU  - Kaneda,H
AU  - Marchetti,L
AU  - Monaco,P
AU  - Nakagawa,T
AU  - Onaka,T
AU  - Papadopoulos,A
AU  - Pearson,C
AU  - Perez-Fournon,I
AU  - Perez-Gonzalez,P
AU  - Roelfsema,P
AU  - Scott,D
AU  - Serjeant,S
AU  - Spinoglio,L
AU  - Vaccari,M
AU  - van,der Tak F
AU  - Vignali,C
AU  - Wang,L
AU  - Wada,T
DO  - 10.1017/pasa.2017.49
PY  - 2017///
SN  - 1323-3580
TI  - Tracing the Evolution of Dust Obscured Star Formation and Accretion Back to the Reionisation Epoch with SPICA
T2  - PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA
UR  - http://dx.doi.org/10.1017/pasa.2017.49
UR  - http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000415377400001&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=1ba7043ffcc86c417c072aa74d649202
UR  - http://hdl.handle.net/10044/1/61099
VL  - 34
ER  -
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