Výsledky vyhledávání - "A. Nebot Gomez-Moran"

Fink, a new generation of broker for the LSST community

Publikováno v: Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2021, 501 (3), pp.3272-3288. ⟨10.1093/mnras/staa3602⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, 501 (3), pp.3272-3288. ⟨10.1093/mnras/staa3602⟩

Fink is a broker designed to enable science with large time-domain alert streams such as the one from the upcoming Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST). It exhibits traditional astronomy broker features such as automatised

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0e497a731e99bb1567393b76496745d0
https://hal.archives-ouvertes.fr/hal-02966245

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The programme: Accurate masses for double-lined spectroscopic binary components

Autor: Lebreton, Y., Halbwachs, J.-L., Kiefer, F., Arenou, F., Famaey, B., Guillout, P., Ibata, R., Mazeh, T., Nebot Gomez-Moran, A., Pourbaix, D.

Publikováno v: PLATO STESCI WORKshop ii
PLATO STESCI WORKshop ii, May 2018, Milazzo, Italy

International audience; We present the programme: Accurate masses for double-lined spectroscopic binary components that combines spectroscopic and interferometric observations of binary stars which constitute a set of benchmarks for the analysis of t

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::ddb1545f811bb5698c0f271328a038bc
https://univ-rennes.hal.science/hal-02355535

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Infrared outbursts as potential tracers of common envelope events in high-mass X-ray binary formation

Autor: Lidia M. Oskinova, Tomasz Bulik, Ada Nebot Gomez-Moran

Publikováno v: Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2018, 613, pp.L10. ⟨10.1051/0004-6361/201832925⟩
Astron.Astrophys.
Astron.Astrophys., 2018, 613, pp.L10. ⟨10.1051/0004-6361/201832925⟩
Astron.Astrophys., 2018, 613, pp.L10. 〈10.1051/0004-6361/201832925〉

Classic massive binary evolutionary scenarios predict that a transitional common-envelope (CE) phase could be preceded as well as succeeded by the evolutionary stage when a binary consists of a compact object and a massive star, that is, a high-mass

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::70485667e6e5f3df91c91a26730eacb0
https://hal.archives-ouvertes.fr/hal-01815272

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Infrared identification of hard X-ray sources in the Galaxy

Autor: A. Nebot Gomez-Moran, F. Riddick, F. X. Pineau, Christian Motch, Manfred W. Pakull, Francisco J. Carrera

Publikováno v: Digital.CSIC. Repositorio Institucional del CSIC
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The nature of the low- to intermediate-luminosity (LX ∼ 1032–34 erg s−1) source population revealed in hard band (2–10 keV) X-ray surveys of the Galactic plane is poorly understood. To overcome such problem, we cross-correlated the XMM–Newt

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1a6ad9ce99ee96dc5f54ad11712c7c7e
https://doi.org/10.1093/mnras/stv1020

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The programme 'accurate masses for SB2 components'

Autor: Halbwachs, J.-L., Arenou, F., Boffin, H. M. J., Famaey, B., Jorissen, A., Kiefer, F., Le Bouquin, J.-B., Pourbaix, D., Guillout, P., Ibata, R., Lebreton, Y., Mazeh, T., Nebot Gomez-Moran, A., Tal-Or, L.

Publikováno v: SF2A Week
SF2A Week, Jul 2017, Paris, France
SF2A-2017: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics

Accurate stellar masses are requested in order to improve our understanding of stellar interiors, but they are still rather rare. Fortunately, the forthcoming Gaia Mission will provide astrometric measurements permitting the derivation of the orbital

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d502c51dd61bd1e5ea7363e2fd6885bb
https://hal-univ-rennes1.archives-ouvertes.fr/hal-02112623

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Probabilistic multi-catalogue positional cross-match

Autor: A. Nebot Gomez-Moran, Alexey Mints, Simon Rosen, Christian Motch, F. X. Pineau, Françoise Genova, Francisco J. Carrera, A. Ruiz Camunãs, Beatriz Mingo, Laurent Michel, S. Derriere

Publikováno v: Astron.Astrophys.
Astron.Astrophys., 2017, 597, pp.A89. ⟨10.1051/0004-6361/201629219⟩
Astron.Astrophys., 2017, 597, pp.A89. 〈10.1051/0004-6361/201629219〉
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2017, 597, pp.A89. ⟨10.1051/0004-6361/201629219⟩
NASA Astrophysics Data System
Digital.CSIC. Repositorio Institucional del CSIC
instname

[Context]: Catalogue cross-correlation is essential to building large sets of multi-wavelength data, whether it be to study the properties of populations of astrophysical objects or to build reference catalogues (or timeseries) from survey observatio

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::30648ba33544ff7dceb058293ad1b88e
https://hal.archives-ouvertes.fr/hal-01554116

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A Multi-Wavelength View of the XMM-Newton Galactic Plane

Autor: Christian Motch, Ada Nebot Gomez-Moran

Publikováno v: Acta Polytechnica CTU Proceedings, Vol 1, Iss 1, Pp 123-126 (2014)

We present an X-ray survey of the Galactic Plane conducted by the Survey Science Centre of the XMM-Newton satellite. The survey contains more than 1300 X-ray detections at low and intermediate Galactic latitudes and covering 4 deg2 well spread in Gal

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d2fb3bb81c4042ca915b3b009208f022
https://doi.org/10.14311/app.2014.01.0123

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Detached cataclysmic variables are crossing the orbital period gap

Autor: M. R. Schreiber, C. Agurto-Gangas, Boris T. Gänsicke, Alberto Rebassa-Mansergas, Monica Zorotovic, A. Hardy, A. Nebot Gomez-Moran, Steven G. Parsons, Axel Schwope

Publikováno v: Recercat. Dipósit de la Recerca de Catalunya
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Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2016, 457 (4), pp.3867-3877. ⟨10.1093/mnras/stw246⟩
UPCommons. Portal del coneixement obert de la UPC
Universitat Politècnica de Catalunya (UPC)

A central hypothesis in the theory of cataclysmic variable (CV) evolution is the need to explain the observed lack of accreting systems in the ~2-3 h orbital period range, known as the period gap. The standard model, disrupted magnetic braking (DMB),

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e65aa1384c02e939b1d08016015a7c98
http://wrap.warwick.ac.uk/86845/1/WRAP_2016MNRAS.457.3867Z.pdf

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