Exploration of the high-redshift universe enabled by THESEUS

At peak, long-duration gamma-ray bursts are the most luminous sources of electromagnetic radiation known. Since their progenitors are massive stars, they provide a tracer of star formation and star-forming galaxies over the whole of cosmic history. Their bright power-law afterglows provide ideal bac...

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Veröffentlicht in:Exper.Astron 2021-12, Vol.52 (3), p.219-244
Hauptverfasser: Tanvir, N. R., Le Floc’h, E., Christensen, L., Caruana, J., Salvaterra, R., Ghirlanda, G., Ciardi, B., Maio, U., D’Odorico, V., Piedipalumbo, E., Campana, S., Noterdaeme, P., Graziani, L., Amati, L., Bagoly, Z., Balázs, L. G., Basa, S., Behar, E., De Cia, A., Valle, M. Della, De Pasquale, M., Frontera, F., Gomboc, A., Götz, D., Horvath, I., Hudec, R., Mereghetti, S., O’Brien, P. T., Osborne, J. P., Paltani, S., Rosati, P., Sergijenko, O., Stanway, E. R., Szécsi, D., Tot́h, L. V., Urata, Y., Vergani, S., Zane, S.
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container_end_page 244
container_issue 3
container_start_page 219
container_title Exper.Astron
container_volume 52
creator Tanvir, N. R.
Le Floc’h, E.
Christensen, L.
Caruana, J.
Salvaterra, R.
Ghirlanda, G.
Ciardi, B.
Maio, U.
D’Odorico, V.
Piedipalumbo, E.
Campana, S.
Noterdaeme, P.
Graziani, L.
Amati, L.
Bagoly, Z.
Balázs, L. G.
Basa, S.
Behar, E.
De Cia, A.
Valle, M. Della
De Pasquale, M.
Frontera, F.
Gomboc, A.
Götz, D.
Horvath, I.
Hudec, R.
Mereghetti, S.
O’Brien, P. T.
Osborne, J. P.
Paltani, S.
Rosati, P.
Sergijenko, O.
Stanway, E. R.
Szécsi, D.
Tot́h, L. V.
Urata, Y.
Vergani, S.
Zane, S.
description At peak, long-duration gamma-ray bursts are the most luminous sources of electromagnetic radiation known. Since their progenitors are massive stars, they provide a tracer of star formation and star-forming galaxies over the whole of cosmic history. Their bright power-law afterglows provide ideal backlights for absorption studies of the interstellar and intergalactic medium back to the reionization era. The proposed THESEUS mission is designed to detect large samples of GRBs at z > 6 in the 2030s, at a time when supporting observations with major next generation facilities will be possible, thus enabling a range of transformative science. THESEUS will allow us to explore the faint end of the luminosity function of galaxies and the star formation rate density to high redshifts; constrain the progress of re-ionisation beyond z ≳ 6 ; study in detail early chemical enrichment from stellar explosions, including signatures of Population III stars; and potentially characterize the dark energy equation of state at the highest redshifts.
doi_str_mv 10.1007/s10686-021-09778-w
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V.</au><au>Urata, Y.</au><au>Vergani, S.</au><au>Zane, S.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Exploration of the high-redshift universe enabled by THESEUS</atitle><jtitle>Exper.Astron</jtitle><stitle>Exp Astron</stitle><stitle>EXP ASTRON</stitle><date>2021-12-01</date><risdate>2021</risdate><volume>52</volume><issue>3</issue><spage>219</spage><epage>244</epage><pages>219-244</pages><issn>0922-6435</issn><eissn>1572-9508</eissn><abstract>At peak, long-duration gamma-ray bursts are the most luminous sources of electromagnetic radiation known. Since their progenitors are massive stars, they provide a tracer of star formation and star-forming galaxies over the whole of cosmic history. Their bright power-law afterglows provide ideal backlights for absorption studies of the interstellar and intergalactic medium back to the reionization era. The proposed THESEUS mission is designed to detect large samples of GRBs at z &gt; 6 in the 2030s, at a time when supporting observations with major next generation facilities will be possible, thus enabling a range of transformative science. THESEUS will allow us to explore the faint end of the luminosity function of galaxies and the star formation rate density to high redshifts; constrain the progress of re-ionisation beyond z ≳ 6 ; study in detail early chemical enrichment from stellar explosions, including signatures of Population III stars; and potentially characterize the dark energy equation of state at the highest redshifts.</abstract><cop>Dordrecht</cop><pub>Springer Netherlands</pub><doi>10.1007/s10686-021-09778-w</doi><tpages>26</tpages><orcidid>https://orcid.org/0000-0003-3274-6336</orcidid><orcidid>https://orcid.org/0000-0001-7082-6009</orcidid><orcidid>https://orcid.org/0000-0001-5326-880X</orcidid><orcidid>https://orcid.org/0000-0002-0039-3102</orcidid><orcidid>https://orcid.org/0000-0003-3693-3091</orcidid><orcidid>https://orcid.org/0000-0002-9231-1505</orcidid><orcidid>https://orcid.org/0000-0001-5876-9259</orcidid><orcidid>https://orcid.org/0000-0002-9212-7118</orcidid><orcidid>https://orcid.org/0000-0002-6089-0768</orcidid><orcidid>https://orcid.org/0000-0001-6278-1576</orcidid><orcidid>https://orcid.org/0000-0001-8468-4953</orcidid><orcidid>https://orcid.org/0000-0002-9393-8078</orcidid><orcidid>https://orcid.org/0000-0003-2082-1626</orcidid><orcidid>https://orcid.org/0000-0003-3142-5020</orcidid><orcidid>https://orcid.org/0000-0002-5128-1899</orcidid><orcidid>https://orcid.org/0000-0002-5777-1629</orcidid><orcidid>https://orcid.org/0000-0002-7504-7423</orcidid><orcidid>https://orcid.org/0000-0002-8108-9179</orcidid><orcidid>https://orcid.org/0000-0001-9398-4907</orcidid><oa>free_for_read</oa></addata></record>
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identifier ISSN: 0922-6435
ispartof Exper.Astron, 2021-12, Vol.52 (3), p.219-244
issn 0922-6435
1572-9508
language eng
recordid cdi_webofscience_primary_000679280000002
source SpringerNature Journals; Web of Science - Science Citation Index Expanded - 2021<img src="https://exlibris-pub.s3.amazonaws.com/fromwos-v2.jpg" />
subjects Afterglows
Astronomy
Astronomy & Astrophysics
Backlights
Chemistry and Earth Sciences
Computer Science
Dark energy
Electromagnetic radiation
Equations of state
Explosions
Galactic evolution
Gamma ray bursts
Instrumentation and Detectors
Intergalactic media
Interstellar matter
Ionization
Luminosity
Massive stars
Observations and Techniques
Original Article
Physical Sciences
Physics
Physics and Astronomy
Population III stars
Red shift
Science & Technology
Star & galaxy formation
Star formation rate
Statistics for Engineering
title Exploration of the high-redshift universe enabled by THESEUS
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