Física de la Tierra y Astrofísica
Departament
National Optical Astronomy Observatory
Tucson, Estados UnidosPublicacions en col·laboració amb investigadors/es de National Optical Astronomy Observatory (12)
2022
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First Sagittarius A* Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole in the Center of the Milky Way
Astrophysical Journal Letters, Vol. 930, Núm. 2
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First Sagittarius A* Event Horizon Telescope Results. II. EHT and Multiwavelength Observations, Data Processing, and Calibration
Astrophysical Journal Letters, Vol. 930, Núm. 2
2019
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The CANDELS/SHARDS Multiwavelength Catalog in GOODS-N: Photometry, Photometric Redshifts, Stellar Masses, Emission-line Fluxes, and Star Formation Rates
Astrophysical Journal, Supplement Series, Vol. 243, Núm. 2
2018
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The Astropy Project: Building an Open-science Project and Status of the v2.0 Core Package
Astronomical Journal, Vol. 156, Núm. 3
2015
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Learning from FITS: Limitations in use in modern astronomical research
Astronomy and Computing, Vol. 12, pp. 133-145
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Worldwide variations in artificial skyglow
Scientific Reports, Vol. 5, pp. 8409
2010
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The HST/ACS Coma cluster survey. II. data description and source catalogs
Astrophysical Journal, Supplement Series, Vol. 191, Núm. 1, pp. 143-159
2009
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Comparison of hα and UV star formation rates in the local volume: Systematic discrepancies for dwarf galaxies
Astrophysical Journal, Vol. 706, Núm. 1, pp. 599-613
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Evidence for intermediate-age stellar populations in early-type galaxies from K-band spectroscopy
Astrophysical Journal, Vol. 705, Núm. 2 PART 2
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Evolution of red-sequence cluster galaxies from redshift 0.8 to 0.4: ages, metallicities, and morphologies
Astronomy and Astrophysics, Vol. 499, Núm. 1, pp. 47-68
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Stellar population study in early-type galaxies: An approach from the K band
Proceedings of the International Astronomical Union
2008
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The hubble space telescope advanced camera for surveys Coma Cluster survey. I. Survey objectives and design
Astrophysical Journal, Supplement Series, Vol. 176, Núm. 2, pp. 424-437