L. M. Howes - Concepedia

Concepedia

Author

L. M. Howes

Lund University ORCID

Also Known As

Fusillo, N. Gentile, Howes, L., Howes, L. M., Howes, Louise Margaret, L M Howes, L. Howes, L. M. Howes, Louise Howes, Louise M. Howes

23

Publications

1.1K

Citations

13

H-Index

15

Concepts

All Affiliations

Lund University Australian National University Uppsala University Centre National de la Recherche Scientifique University of Cambridge

LM

About

L. M. Howes is an author at Lund University specializing in photometry, engineering, and astrophysics.

Top Concepts

#	Concept	H-Index	Publications	Citations
1	Engineering	4	4	523
2	Natural Sciences	1	1	33
3	Physics	1	1	33
4	Space Sciences	1	1	311
5	Astrodynamics	1	1	33

L. M. Howes

×

13

Publications

1.1K

Citations

13

H-Index

	Year	Citations
4MOST: Project overview and information for the First Call for Proposals Roelof S. de Jong, Oscar Agertz, James Aird, Swinburne Research Bank (Swinburne University of Technology) EngineeringProject ManagementSpace OpticSatellite InstrumentationActive Optics	2019	311
Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars T. Bensby, S. Feltzing, Andrew Gould, Astronomy and Astrophysics	2017	184
Extremely metal-poor stars from the cosmic dawn in the bulge of the Milky Way L. M. Howes, Andrew R. Casey, M. Asplund, Nature Cosmic AbundancePhotometryEngineeringBlack Hole PhysicsStellar Structure	2015	111
The EMBLA survey – metal-poor stars in the Galactic bulge L. M. Howes, M. Asplund, Stefan Keller, Monthly Notices of the Royal Astronomical Society	2016	99
On the metallicity dependance of the [Y/Mg] – age relation for solar type stars S. Feltzing, L. M. Howes, P. J. McMillan, Monthly Notices of the Royal Astronomical Society Letters	2016	77
The Gaia-ESO Survey: the most metal-poor stars in the Galactic bulge L. M. Howes, M. Asplund, Andrew R. Casey, Monthly Notices of the Royal Astronomical Society Bulge StarsCosmic AbundancePhotometryAaomega SpectroscopyEngineering	2014	68
Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars. VI. Age and abundance structure of the stellar populations in the central sub-kpc of the Milky Way T. Bensby, S. Feltzing, Andrew Gould, arXiv (Cornell University)	2017	66
The<i>Gaia</i>-ESO Survey: the selection function of the Milky Way field stars E. Stonkuté, S. E. Koposov, L. M. Howes, Monthly Notices of the Royal Astronomical Society	2016	37
Estimating stellar ages and metallicities from parallaxes and broadband photometry: successes and shortcomings L. M. Howes, L. Lindegren, S. Feltzing, Astronomy and Astrophysics Cosmic AbundanceGalaxy FormationPhotometryEngineeringPhysics	2018	33
Using the multi-object adaptive optics demonstrator RAVEN to observe metal-poor stars in and towards the Galactic Centre Masen Lamb, Kim A. Venn, David R. Andersen, Monthly Notices of the Royal Astronomical Society	2016	22

Page 1