8 research outputs found
The THESEUS space mission concept: science case, design and expected performances
- Author
- Adami C.
- Amati L.
- Antonelli A.
- Argan A.
- Atteia J.L.
- Attina P.
- Auricchio N.
- Bagoly Z.
- Balazs L.
- Baldazzi G.
- Basa S.
- Basak R.
- Bellutti P.
- Bernardini M. G.
- Bertuccio G.
- Bianco F.
- Blain A.
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- Boer M.
- Botticella M.T.
- Boulade O.
- Bozzo E.
- Braga J.
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- Briggs M.
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- Budtz-Jørgensen C.
- Bulgarelli A.
- Burderi L.
- Butler C.
- Callanan P.
- Camp J.
- Campana R.
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- Campolongo E.
- Capitanio F.
- Capozziello S.
- Caruana J.
- Casella P.
- Castro-Tirado Alberto J.
- Celotti A.
- Cenko B.
- Chardonnet P.
- Chen Y.
- Ciardi B.
- Ciolfi R.
- Colafrancesco S.
- Colpi M.
- Comastri A.
- Connaughton V.
- Contini C.
- Cordier B.
- Covino S.
- Cuby Jean-Gabriel
- D'Avanzo P.
- D'Elia V.
- Dadina M.
- Dainotti M. G.
- De Luca A.
- De Martino D.
- De Pasquale M.
- Del Monte E.
- Della Valle M.
- Dong Y. -W.
- Drago Alessandro
- Ettori S.
- Evangelista Y.
- Feroci M.
- Ferrara A.
- Finelli F.
- Fiorini M.
- Frontera F.
- Fuschino F.
- Fynbo J.
- Gal-Yam Avishay
- Gandhi P.
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- Hafizi M.
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- Zhang B.
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- Zicha J.
- Publication venue
- 'Elsevier BV'
- Publication date
- 03/07/2020
- Field of study
THESEUS is a space mission concept aimed at exploiting Gamma-Ray Bursts for investigating the early Universe and at providing a substantial advancement of multi-messenger and time-domain astrophysics. These goals will be achieved through a unique combination of instruments allowing GRB and X-ray transient detection over a broad field of view (more than 1sr) with 0.5¿1 arcmin localization, an energy band extending from several MeV down to 0.3¿keV and high sensitivity to transient sources in the soft X-ray domain, as well as on-board prompt (few minutes) follow-up with a 0.7¿m class IR telescope with both imaging and spectroscopic capabilities. THESEUS will be perfectly suited for addressing the main open issues in cosmology such as, e.g., star formation rate and metallicity evolution of the inter-stellar and intra-galactic medium up to redshift
10, signatures of Pop III stars, sources and physics of re-ionization, and the faint end of the galaxy luminosity function. In addition, it will provide unprecedented capability to monitor the X-ray variable sky, thus detecting, localizing, and identifying the electromagnetic counterparts to sources of gravitational radiation, which may be routinely detected in the late ¿20s/early ¿30s by next generation facilities like aLIGO/ aVirgo, eLISA, KAGRA, and Einstein Telescope. THESEUS will also provide powerful synergies with the next generation of multi-wavelength observatories (e.g., LSST, ELT, SKA, CTA, ATHENA).© 2018 COSPARS.E. acknowledges the financial support from contracts ASI-INAF 1/009/10/0, NARO15 ASI-INAF 1/037/12/0 and ASI 2015-046-R.0. R.H. acknowledges GACR grant 13-33324S. S.V. research leading to these results has received funding from the European Union's Seventh Framework Programme for research, technological development and demonstration under grant agreement no 606176. D.S. was supported by the Czech grant 1601116S GA CR. Maria Giovanna Dainotti acknowledges funding from the European Union through the Marie Curie Action FP7-PEOPLE-2013-IOF, under grant agreement No. 626267 (>Cosmological Candles>)
NON-UNIONS AFTER FIXATION OF HUMERAL FRACTURES USING HACKETHAL'S BUNDLE NAILING TECHNIQUE
- Author
- Publication venue
- 'FapUNIFESP (SciELO)'
- Publication date
- Field of study
Supplement: "Localization and broadband follow-up of the gravitational-wave transient GW150914" (2016, ApJL, 826, L13)
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- Publication date
- 01/01/2016
- Field of study
This Supplement provides supporting material for Abbott et al. (2016a). We briefly summarize past electromagnetic (EM) follow-up efforts as well as the organization and policy of the current EM follow-up program. We compare the four probability sky maps produced for the gravitational-wave transient GW150914, and provide additional details of the EM follow-up observations that were performed in the different bands
Localization and Broadband Follow-up of the Gravitational-wave Transient GW150914
- Author
- Abbott B. P.
- Abbott R.
- Abbott T. D.
- Abbott T. M. C.
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- Australian Square Kilometer Array Pathfinder (ASKAP) Collaboration
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- Publication venue
- 'American Astronomical Society'
- Publication date
- 28/10/2022
- Field of study
A gravitational-wave (GW) transient was identified in data recorded by
the Advanced Laser Interferometer Gravitational-wave Observatory (LIGO)
detectors on 2015 September 14. The event, initially designated G184098
and later given the name GW150914, is described in detail elsewhere. By
prior arrangement, preliminary estimates of the time, significance, and
sky location of the event were shared with 63 teams of observers
covering radio, optical, near-infrared, X-ray, and gamma-ray wavelengths
with ground- and space-based facilities. In this Letter we describe the
low-latency analysis of the GW data and present the sky localization of
the first observed compact binary merger. We summarize the follow-up
observations reported by 25 teams via private Gamma-ray Coordinates
Network circulars, giving an overview of the participating facilities,
the GW sky localization coverage, the timeline, and depth of the
observations. As this event turned out to be a binary black hole merger,
there is little expectation of a detectable electromagnetic (EM)
signature. Nevertheless, this first broadband campaign to search for a
counterpart of an Advanced LIGO source represents a milestone and
highlights the broad capabilities of the transient astronomy community
and the observing strategies that have been developed to pursue neutron
star binary merger events. Detailed investigations of the EM data and
results of the EM follow-up campaign are being disseminated in papers by
the individual teams.
</p
Localization and broadband follow-up of the gravitational-wave transient GW150914
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- Ćwiek FTPESSTOCA
- Ćwiok M
- Żarnecki AF
- Publication venue
- IOP PUBLISHING LTD
- Publication date
- Field of study
A gravitational-wave transient was identified in data recorded by the Advanced LIGO detectors on 2015 September 14. The event candidate, initially designated G184098 and later given the name GW150914, is described in detail elsewhere. By prior arrangement, preliminary estimates of the time, significance, and sky location of the event were shared with 63 teams of observers covering radio, optical, near-infrared, X-ray, and gamma-ray wavelengths with ground- and space-based facilities. In this Letter we describe the low-latency analysis of the gravitational wave data and present the sky localization of the first observed compact binary merger. We summarize the follow-up observations reported by 25 teams via private Gamma-ray Coordinates Network Circulars, giving an overview of the participating facilities, the gravitational wave sky localization coverage, the timeline and depth of the observations. As this event turned out to be a binary black hole merger, there is little expectation of a detectable electromagnetic signature. Nevertheless, this first broadband campaign to search for a counterpart of an Advanced LIGO source represents a milestone and highlights the broad capabilities of the transient astronomy community and the observing strategies that have been developed to pursue neutron star binary merger events. Detailed investigations of the electromagnetic data and results of the electromagnetic follow-up campaign will be disseminated in the papers of the individual teams
A Decade of GRB Follow-Up by BOOTES in Spain (2003-2013)
- Author
- Castillo-Carrión S.
- Castro-Tirado Alberto J.
- Cunniffe R.
- De La Morena Carretero B.A.
- Fernández-Muñoz R.
- Gorosabel J.
- Guziy S.
- Hudec R.
- Jelínek M.
- Jeong S.
- Kubánek P.
- Mateo Sanguino T.
- Oates S.
- Páta P.
- Pérez-Ramírez D.
- Rabaza O.
- Reglero V.
- Sabau-Graziati L.
- Sánchez-Ramírez R.
- Tello J.C.
- Ugarte Postigo Antonio de
- Vítek S.
- Štrobl J.
- Publication venue
- 'Hindawi Limited'
- Publication date
- 29/06/2018
- Field of study
This article covers ten years of GRB follow-ups by the Spanish BOOTES stations: 71 follow-ups providing 23 detections. Follow-ups by BOOTES-1B from 2005 to 2008 were given in a previous article and are here reviewed and updated, and additional detection data points are included as the former article merely stated their existence. The all-sky cameras CASSANDRA have not yet detected any GRB optical afterglows, but limits are reported where available.The authors appreciate the auspices of INTA, IHSM-UMA/CSIC, and UMA as well as the financial support by the Junta de Andaluca and the Spanish Ministry of Economy and Competitiveness through the Research Projects P07-TIC-03094, P12-TIC2839, AYA2009-14000-C03-01, AYA 2010-39727-C03-01, and AYA-2015-71718-R. Martin Jelinek was supported by the postdoctoral fellowship of the Czech Academy of Sciences. This study was carried out in the framework of the Unidad Asociada IAA-CSIC at the Group of Planetary Science of ETSI-UPV/EHU. This work was supported by the Ikerbasque Foundation for Science. The Czech CVUT FEL team acknowledges the support by GA CR Grant 13-33324S.Peer Reviewe
THE GLOBAL ROBOTIC TELESCOPES INTELLIGENT ARRAY FOR E-SCIENCE (GLORIA)
- Author
- A. F. Zarnecki
- A. González-Rodríguez
- A. J. Castro-Tirado
- C. Linttot
- C. Pérez del Pulgar
- D. Azócar
- E. González
- E. Maureira
- E. O\u2019Boyle
- E. Palazzi
- F. M. Sánchez Moreno
- F. Serena
- G. Beskin
- J. Cabello
- J. Gorosabel
- J. Maza
- J. Strobl
- L. Cuesta
- L. Hanlon
- L. Mankiewicz
- L. Nicastro
- M. A. Pio
- M. C. López-Casado
- M. Jakubek
- M. Jelínek
- M. Malaspina
- M. Prouza
- M. Serra-Ricart
- M. Topinka
- O. Lara-Gil
- P. Janecek
- P. Páta
- P. Sprimont
- R. Cedazo
- R. Cunniffe
- R. Hudec
- R. Simpson
- S. Vitek
- V. F. Muñoz-Martí\u0131nez
- Publication venue
- Universidad Nacional Autónoma de México
- Publication date
- 01/01/2014
- Field of study
G L O R I A e s u n p r o y e c t o w e b - 2 . 0 c o l a b o r a t i v o b a s a d o e n u n a r e d d e t e l e s c o p i o s r o b ́ o t i c o s d e a c c e s o l i b r e q u e e s t ́ a a b i e r t o a l p ́ u b l i c o y e n f o c a d o a l a d i v u l g a c i ́ o n a s t r o n ́ o m i c a y s o b r e t o d o a C i e n c i a C i u d a d a n a
Localization and broadband follow-up of the gravitational-wave transient GW150914
- Author
- Abbott BP
- Abbott R
- Abbott TD
- Abbott TMC
- Abdalla FB
- Abe F
- Abernathy MR
- Acernese F
- Ackermann M
- Ackley K
- Adame JA
- Adams C
- Adams T
- Addesso P
- Adhikari RX
- Adya VB
- Affeldt C
- Agathos M
- Agatsuma K
- Aggarwal N
- Aguiar OD
- Aiello L
- Ain A
- Ajello M
- Ajith P
- Albert A
- Allam S
- Allen B
- Allen WH
- Allison J
- Allocca A
- Altin PA
- Amati L
- Anderson B
- Anderson JP
- Anderson SB
- Anderson WG
- Annis J
- Antonelli LA
- Aptekar RL
- Arai K
- Araya MC
- Arceneaux CC
- Areeda JS
- Armstrong R
- Arnaud N
- Arun KG
- Ascenzi S
- Ashton G
- Ast M
- Aston SM
- Astone P
- Atwood WB
- Aufmuth P
- Aulbert C
- Axelsson M
- Babak S
- Bacon P
- Bader MKM
- Bai J
- Baiardi LC
- Baker PT
- Balanutsa P
- Baldaccini F
- Baldini L
- Ballardin G
- Ballmer SW
- Baltay C
- Banerji M
- Bannister K
- Barayoga JC
- Barbiellini G
- Barclay SE
- Barish BC
- Barker D
- Barlow T
- Barone F
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- Barsuglia M
- Barta D
- Barthelmy S
- Bartlett J
- Bartos I
- Bassiri R
- Basti A
- Bastieri D
- Batch JC
- Baune C
- Bavigadda V
- Bazzan M
- Bazzano A
- Behnke B
- Bejger M
- Bell AS
- Bell CJ
- Bell ME
- Bellazzini R
- Bellm E
- Benacquista M
- Benoit-Lévy A
- Berger BK
- Berger E
- Bergman J
- Bergmann G
- Bernstein RA
- Beroiz M
- Berry CPL
- Bersanetti D
- Bersier DF
- Bertin E
- Bertolini A
- Betzwieser J
- Bhagwat S
- Bhalerao V
- Bhandare R
- Bhat PN
- Bilenko IA
- Billingsley G
- Birch J
- Birney R
- Biscans S
- Bisht A
- Bissaldi E
- Bitossi M
- Biwer C
- Bizouard MA
- Blackburn JK
- Blackburn L
- Blair CD
- Blair DG
- Blair RM
- Blandford RD
- Bloemen S
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- Tyurina N
- Tápai M
- Töyrä D
- Ubertini P
- Uchiyama Y
- Ueno S
- Ugolini D
- Ulaczyk K
- Unnikrishnan CS
- Urban AL
- Usman SA
- Vahlbruch H
- Vajente G
- Valdes G
- Valenti S
- Valle MD
- van Bakel N
- van Beuzekom M
- van den Brand JFJ
- Van Den Broeck C
- van der Schaaf L
- van Heijningen JV
- van Veggel AA
- Vander-Hyde DC
- Vardaro M
- Vass S
- Vasúth M
- Vaulin R
- Vecchio A
- Vedovato G
- Veitch J
- Veitch PJ
- Venkateswara K
- Venters TM
- Veres P
- Verkindt D
- Vetrano F
- Vianello G
- Viceré A
- Vikram V
- Vinciguerra S
- Vine DJ
- Vinet J-Y
- Virgilio AD
- Vitale S
- Vitek S
- Vo T
- Vocca H
- Voronkov MA
- Vorvick C
- Voss D
- Vousden WD
- Vrech R
- Vyatchanin SP
- Wade AR
- Wade LE
- Wade M
- Walker AR
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- Wallace L
- Walsh S
- Wang C
- Wang G
- Wang H
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- Wang X
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- Ward RL
- Warner J
- Was M
- Waters C
- Watson D
- Wayth RB
- Weaver B
- Wechsler RH
- Wei L-W
- Weinert M
- Weinstein AJ
- Weiss R
- Welborn T
- Wen L
- Wester W
- Westphal T
- Wette K
- Weßels P
- Whelan JT
- White DJ
- Whiting BF
- Whiting MT
- Wiersema K
- Wijers RAMJ
- Williams A
- Williams RD
- Williamson AR
- Willis JL
- Willke B
- Willman M
- Wilson-Hodge CA
- Wimmer MH
- Winkler W
- Wipf CC
- Wittel H
- Woan G
- Wolf C
- Wood KS
- Wood M
- Worden J
- Wright DE
- Wright JL
- Wu G
- Yablon J
- Yam W
- Yamamoto H
- Yanagisawa K
- Yancey CC
- Yang S
- Yanny B
- Yap MJ
- Yock PC
- Yoshida M
- Young DR
- Yu H
- Yu H-F
- Yuan F
- Yurkov V
- Yvert M
- Zadrożny A
- Zangrando L
- Zanolin M
- Zaremba M
- Zendri J-P
- Zevin M
- Zhang B-B
- Zhang F
- Zhang L
- Zhang M
- Zhang X
- Zhang Y
- Zhao C
- Zhou M
- Zhou Z
- Zhu S
- Zhu XJ
- Zimmer S
- Zucker ME
- Zuntz J
- Zuraw SE
- Zweizig J
- Ćwiek A
- Ćwiok M
- Żarnecki AF
- Publication venue
- 'American Astronomical Society'
- Publication date
- 01/01/2016
- Field of study
A gravitational-wave (GW) transient was identified in data recorded by the Advanced Laser Interferometer Gravitational-wave Observatory (LIGO) detectors on 2015 September 14. The event, initially designated G184098 and later given the name GW150914, is described in detail elsewhere. By prior arrangement, preliminary estimates of the time, significance, and sky location of the event were shared with 63 teams of observers covering radio, optical, near-infrared, X-ray, and gamma-ray wavelengths with ground- and space-based facilities. In this Letter we describe the low-latency analysis of the GW data and present the sky localization of the first observed compact binary merger. We summarize the follow-up observations reported by 25 teams via private Gamma-ray Coordinates Network circulars, giving an overview of the participating facilities, the GW sky localization coverage, the timeline, and depth of the observations. As this event turned out to be a binary black hole merger, there is little expectation of a detectable electromagnetic (EM) signature. Nevertheless, this first broadband campaign to search for a counterpart of an Advanced LIGO source represents a milestone and highlights the broad capabilities of the transient astronomy community and the observing strategies that have been developed to pursue neutron star binary merger events. Detailed investigations of the EM data and results of the EM follow-up campaign are being disseminated in papers by the individual teams