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Author:
Damiano F. G. Fiorillo, Luca Comisso, Enrico Peretti, Maria Petropoulou, Lorenzo Sironi
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Author:
Maitreya Kundu, Arit Bala, Saugata Barat, Ritaban Chatterjee
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Author:
Iurii Sushch, Pasquale Blasi, Robert Brose
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Title:
Author:
Ivan Agudo, Ioannis Liodakis, Jorge Otero-Santos, Riccardo Middei, Alan Marscher, Svetlana Jorstad, Haocheng Zhang, Hui Li et al.
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Author:
Alberto Antonioni, Michele Re Fiorentin, Eugenio Valdano
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Author:
Hagai Netzer
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Author:
F. Vazza
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Author:
Iuliia Grotova, Arne Rau, Pietro Baldini, Adelle J. Goodwin, Zhu Liu, Andrea Merloni, Mara Salvato, Gemma E. Anderson et al.
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1
(created 2025-05-05T12:33:58Z)
Novel color via stimulation of individual photoreceptors at population scale
https://www.science.org/doi/10.1126/sciadv.adu1052
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Votes: 1
1 month ago Author:
M. Kachelriess, E. Lammert
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Votes: 1
1 month ago Author:
Paul Simeon, Noémie Globus, Kirk S. S. Barrow, Roger Blandford
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Votes: 1
1 month ago Author:
Ryan Plestid, Bei Zhou
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Votes: 1
1 month ago
Title:
Irradiated Pulsar Planets and Companions as 511 keV Positron
Annihilation Line Sources
(View PDF)
Author:
Zachary Metzler, Zorawar Wadiasingh
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Votes: 1
1 month ago Author:
Julian Kuhlmann, Francesca Capel
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Votes: 1
1 month ago
Title:
One Extension to Explain Them All, One Parameter to Minimize $\chi^2$,
One Framework to Bring Them All, and in One Model Bind Them
(View PDF)
Author:
Matteo Forconi, Eleonora DI Valentino
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1 month ago
Title: Three-dimensional maps of the interstellar dust extinction curve within the Milky Way galaxy
Link: https://doi.org/10.1126/science.ado9787
Description: Interstellar dust grains cause extinction (absorption and scattering) of light from background astronomical sources. The spectral shape of the extinction curve depends on the dust composition. We used low-resolution optical spectra to measure the extinction curve of 130 million stars. By inverting these data, we mapped the extinction curve parameter R(V) within the Milky Way in three dimensions and within the Magellanic Clouds in two dimensions. These maps provide improved extinction corrections for astronomical observations. We find that R(V) varies with extinction, consistent with dust grains growing by accretion in low-extinction regions and by coagulation in higher-extinction regions. Star-forming regions have high R(V) values, indicating either preferential destruction of small dust grains or additional supply of large dust grains in those regions.
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Votes: 1
1 month ago Author:
Alexander V. Plavin, Yuri Y. Kovalev, Sergey V. Troitsky
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Votes: 1
1 month ago
Title:
A Massive Black Hole 0.8 kpc from the Host Nucleus Revealed by the
Offset Tidal Disruption Event AT2024tvd
(View PDF)
Author:
Yuhan Yao, Ryan Chornock, Charlotte Ward, Erica Hammerstein, Itai Sfaradi, Raffaella Margutti, Luke Zoltan Kelley, Wenbin Lu et al.
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Votes: 1
2 months ago
Title:
Measurement of Very-high-energy Diffuse Gamma-ray Emissions from the
Galactic Plane with LHAASO-WCDA
(View PDF)
Author:
[LHAASO Collaboration]
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