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Deep learning in astronomy: a tutorial perspective
Astronomy is a branch of science that covers the study and analysis of all extraterrestrial
objects and their phenomena. The study brings together the aspects of mathematics …
objects and their phenomena. The study brings together the aspects of mathematics …
A stellar spectral flux library: 1150–25000 Å
AJ Pickles - Publications of the Astronomical Society of the Pacific, 1998 - iopscience.iop.org
ABSTRACT A stellar spectral flux library of wide spectral coverage and an example of its
application are presented. The new library consists of 131 flux‐calibrated spectra …
application are presented. The new library consists of 131 flux‐calibrated spectra …
Circular polarization in star-formation regions: Implications for biomolecular homochirality
J Bailey, A Chrysostomou, JH Hough, TM Gledhill… - Science, 1998 - science.org
Strong infrared circular polarization resulting from dust scattering in reflection nebulae in the
Orion OMC-1 star-formation region has been observed. Circular polarization at shorter …
Orion OMC-1 star-formation region has been observed. Circular polarization at shorter …
[كتاب][B] Dust in the galactic environment
DCB Whittet - 2018 - taylorfrancis.com
Dust is a ubiquitous feature of the cosmos, im**ing directly or indirectly on most fields of
modern astronomy and astrophysics. Dust in the Galactic Environment, Second Edition …
modern astronomy and astrophysics. Dust in the Galactic Environment, Second Edition …
Astronomical sources of circularly polarized light and the origin of homochirality
J Bailey - Origins of Life and Evolution of the Biosphere, 2001 - Springer
Possible astronomical sources of ultraviolet circularly polarized light (UVCPL) which might
be responsible for enantiomeric selection in interstellarorganic molecules are considered …
be responsible for enantiomeric selection in interstellarorganic molecules are considered …
[HTML][HTML] B (e)-supergiants of the Magellanic Clouds
FJ Zickgraf, B Wolf, O Stahl, C Leitherer… - … vol. 163, no. 1-2, July …, 1986 - adsabs.harvard.edu
Spectroscopic and photometric observations at the satellite UV, visual, and infrared
wavelengths of 8 Magellanic Clouds dusty B [e]-supergiants are discussed. In spite of their …
wavelengths of 8 Magellanic Clouds dusty B [e]-supergiants are discussed. In spite of their …
Powerful model for the point source sky: Far-ultraviolet and enhanced midinfrared performance
M Cohen - Astronomical Journal (ISSN 0004-6256), vol. 107 …, 1994 - adsabs.harvard.edu
I report further developments of the Wainscoat et al.(1992) model originally created for the
point source infrared sky. The already detailed and realistic representation of the Galaxy …
point source infrared sky. The already detailed and realistic representation of the Galaxy …
In-flight calibration of the Cassini imaging science sub-system cameras
R West, B Knowles, E Birath, S Charnoz… - Planetary and Space …, 2010 - Elsevier
We describe in-flight calibration of the Cassini Imaging Science Sub-system narrow-and
wide-angle cameras using data from 2004 to 2009. We report on the photometric …
wide-angle cameras using data from 2004 to 2009. We report on the photometric …
[HTML][HTML] Orbital elements of S stars-Revisiting the evolutionary status of S stars
A Jorissen, M Mayor - … and Astrophysics (ISSN 0004-6361), vol …, 1992 - adsabs.harvard.edu
The hypothesis of an evolutionary link between barium stars and the non-Mira S stars is
discussed. The hypothesis of an evolutionary link between the barium stars and the non …
discussed. The hypothesis of an evolutionary link between the barium stars and the non …
SAO 244567-A post-AGB star which has turned into a planetary nebula within the last 40 years
M Parthasarathy, P Garcia-Lario, SR Pottasch… - 1993 - prints.iiap.res.in
SAO 244567 (Hen 1357= CPD-59 deg 6926= IRAS 17119-5926) is an IRAS source with far
infrared colors and flux distribution similar to those of planetary nebulae. The IUE ultraviolet …
infrared colors and flux distribution similar to those of planetary nebulae. The IUE ultraviolet …