Results 91 to 100 of about 486 (135)

PLANETARY CANDIDATES OBSERVED BY Kepler. VIII. A FULLY AUTOMATED CATALOG WITH MEASURED COMPLETENESS AND RELIABILITY BASED ON DATA RELEASE 25. [PDF]

Astrophys J Suppl Ser, 2018
Thompson SE, Coughlin JL, Hoffman K, Mullally F, Mullally F, Christiansen JL, Burke CJ, Bryson S, Batalha N, Haas MR, Catanzarite J, Rowe JF, Barentsen G, Caldwell DA, Clarke BD, Jenkins JM, Li J, Latham DW, Lissauer JJ, Mathur S, Morris RL, Seader SE, Smith JC, Klaus TC, Twicken JD, Van Cleve JE, Wohler B, Akeson R, Ciardi DR, Cochran WD, Henze CE, Howell SB, Huber D, Prša A, Ramírez SV, Morton TD, Barclay T, Campbell JR, Chaplin WJ, Charbonneau D, Christensen-Dalsgaard J, Dotson JL, Doyle L, Dunham EW, Dupree AK, Ford EB, Geary JC, Girouard FR, Isaacson H, Kjeldsen H, Quintana EV, Ragozzine D, Shporer A, Aguirre VS, Steffen JH, Still M, Tenenbaum P, Welsh WF, Wolfgang A, Zamudio KA, Koch DG, Borucki WJ.   +61 more
europepmc   +1 more source

Comment on "Bayesian astrostatistics: a backward look to the future" by Tom Loredo, arXiv:1208.3036

, 2012
This short note points out two of the incongruences that I find in the Loredo (2012) comments on Andreon (2012), i.e. on my chapter written for the book "Astrostatistical Challenges for the New Astronomy". First, I find illogic the Loredo decision of putting my chapter among those presenting simple models, because one of the models illustrated in my ...
openaire   +2 more sources

Review of 2D Spectral Image Processing Techniques

The processing of two-dimensional (2D) spectral images constitutes a critical and multifaceted discipline in contemporary astronomical data analysis. As spectroscopic instruments evolve towards higher multiplexing, resolution, and sensitivity, the raw 2D
Bo Qiu, A-Li Luo, Tao Lu, Siqi Liu
core   +1 more source

Straight to the Source: Detecting Aggregate Objects in Astronomical Images with Proper Error Control. [PDF]

J Am Stat Assoc, 2013
Friedenberg DA, Genovese CR.
europepmc   +1 more source

Cloud-Adaptive Observation Replanning with All-Sky Camera Semantic Segmentation at Xinglong Observatory

Nighttime ground-based astronomical observations are often hindered by unpredictable cloud cover, which significantly reduces observing efficiency and complicates manual schedule adjustments.
Cunshi Wang, Ying Wu, Yu Zhang, Yuyang Li, Zhenyang Huang, Chengze Li, Jinhao Fan   +6 more
core   +1 more source

Cosmology from One Galaxy in a Void?

The Astrophysical Journal Letters
Understanding galaxy properties may be the key to unlocking some of the most intriguing mysteries of modern cosmology. Recent work relied on machine learning to extract cosmological constraints on Ω _m using only one galaxy.
Bonny Y. Wang, Alice Pisani
doaj   +1 more source

Exploring the Model Dependence of MCMC-based 21 cm Power Spectrum Parameter Constraints

The Astrophysical Journal
Detection and analysis of the cosmic 21 cm signal of neutral hydrogen has long been considered the most promising route towards exploration of the Epoch of Reionization (EoR).
A. Berklas, J. C. Pober
doaj   +1 more source

ASTROSTATISTICS, COSMIC INFORMATION, AND THE TESTABILITY OF THE THEORY OF OBJECTIVITY: a critical–propositional analysis of the white paper Astrostatistics in Canada, by Eadie et al., in dialogue with the modal axioms, phenomenic elements, Inducer Effects, cosmogonic theorem, and cosmological Eras of TO

This article presents a critical–propositional analysis of the white paper Astrostatistics in Canada by Eadie et al. (2019), published on Zenodo under DOI https://doi.org/10.5281/zenodo.3756019, with Pauline Barmby among its coauthors, in dialogue with the Theory of Objectivity (TO).
Cabannas, Vidamor, Silva, Denivaldo
openaire   +2 more sources

Editorial: Frontiers in astronomy and space sciences: a decade of discovery and advancement-10th anniversary conference

Frontiers in Astronomy and Space Sciences
Julio Navarro, Alberto G. Fairén, Alberto G. Fairén, Didier Fraix-Burnet, Steve B. Howell, Paola Marziani, Cristina Puzzarini, Miriam Rengel   +7 more
doaj   +1 more source

Time Contour Plots

, 2020
This new SAS ® tool is two-dimensional color chart for visualizing changes in a population or system over time. Data for one point in time appear as a thin horizontal band of color.
David J Corliss
core