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Euclid: Superluminous supernovae in the Deep Survey

Subjects: redshift: dependence; [ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]; Astrophysics

  • Source: Astron.Astrophys.Astron.Astrophys., 2018, 609, pp.A83. ⟨10.1051/0004-6361/201731758⟩Repositorio Digital de la Universidad Politécnica de CartagenainstnameNASA

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AGN Feedback and Its Quenching Efficiency

Subjects: active galaxy nuclei; lcsh:Astronomy; High Energy Physics::Lattice

  • Source: Frontiers in Astronomy and Space SciencesFrontiers in Astronomy and Space Sciences, 2017, 4, ⟨10.3389/fspas.2017.00010⟩Frontiers in Astronomy and Space Sciences, Frontiers Media, 2017,

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X-rays from the mode-switching PSR B0943+10

Subjects: Physics; 010504 meteorology & atmospheric sciences; Astrophysics::High Energy Astrophysical Phenomena

  • Source: IAU Symp.IAU Symposium 337IAU Symposium 337, Sep 2017, Jodrell Bank Observatory, United Kingdom. pp.62-65, ⟨10.1017/S1743921317009504⟩Proceedings of the International

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The DR14 APOGEE-TGAS catalogue: Precise chemo-kinematics in the extended solar vicinity

Subjects: Orbital elements; Physics; 010308 nuclear & particles physics

  • Source: Proceedings of the International Astronomical UnionProceedings of the International Astronomical Union, Cambridge University Press (CUP), 2017, 13 (S334), pp.153-157.

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Star Formation Efficiency at Intermediate Redshift

Subjects: Cosmology and Nongalactic Astrophysics (astro-ph.CO); FOS: Physical sciences; Fraction (chemistry)

  • Source: Proceedings of the International Astronomical UnionProceedings of the International Astronomical Union, Volume 292, pp. 303-306, 20132013IAUS..292..303C IAU Symposium 292 (Molecular Gas,

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Variation in the dust spectral index across M33

Subjects: Cosmology and Nongalactic Astrophysics (astro-ph.CO); FOS: Physical sciences; Astrophysics

  • Source: Proceedings IAU Symposium No. 284, 2011, R.J. Tuffs & C.C.Popescu, edsThe Spectral Energy Distribution of GalaxiesThe Spectral Energy Distribution of

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