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Your search keyword '"Balona, Luis"' showing total 6 results
Start Over Author "Balona, Luis" Publication Type Conference Materials
6 results on '"Balona, Luis"'

1. PySALT: the SALT science pipeline

Author

Crawford, Steven M., primary, Still, Martin, additional, Schellart, Pim, additional, Balona, Luis, additional, Buckley, David A. H., additional, Dugmore, Garith, additional, Gulbis, Amanda A. S., additional, Kniazev, Alexei, additional, Kotze, Marissa, additional, Loaring, Nicola, additional, Nordsieck, Kenneth H., additional, Pickering, Timothy E., additional, Potter, Stephen, additional, Romero Colmenero, Encarni, additional, Vaisanen, Petri, additional, Williams, Theodore, additional, and Zietsman, Ewald, additional

Published
2010
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3. The image quality of the Southern African Large Telescope (SALT)

Author

O'Donoghue, Darragh E., primary, Atad-Ettedgui, Eli, additional, Balona, Luis, additional, Bigelow, Bruce C., additional, Booth, John A., additional, Botha, Lucian, additional, Brink, Janus D., additional, Buckley, David A. H., additional, Charles, Phil, additional, Christians, Alrin, additional, Clemens, J. Christopher, additional, Crause, Lisa A., additional, Crawford, Steven M., additional, Evans, Geoffrey P., additional, Gajjar, Hitesh, additional, Hashimoto, Yas, additional, Hendricks, Malcolm, additional, Kniazev, Alexei, additional, Koeslag, Anthony R., additional, Koorts, Willie P., additional, Kriel, Herman J., additional, Loaring, Nicola S., additional, Love, Jonathan, additional, Marang, Fred, additional, Metcalfe, Douglas, additional, Meyer, Brennan, additional, O'Connor, James, additional, du Plessis, Charl A., additional, Ramsey, Lawrence W., additional, Romero-Colmenero, Encarni, additional, Sass, Craig, additional, Scholtz, Johann C., additional, Sefako, Ramotholo, additional, Siyengo, Sandisa, additional, Still, Martin, additional, Strydom, Ockert J., additional, Swat, Arkadiusz, additional, Du Toit, Johann F., additional, Vaisanen, Petri, additional, Wells, Martyn, additional, and Worters, Hannah, additional

Published
2008
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4. High-speed SALT instrument CCD detectors

Author

O'Donoghue, Darragh, primary, Balona, Luis A., additional, Carter, Dave B., additional, Evans, Geoff P., additional, Fourie, Piet, additional, Koorts, Willie P., additional, O'Connor, James, additional, Osman, Faranah, additional, Petersen, Chantal, additional, and Steyn, Hendrik, additional

Published
2004
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5. The image quality of the Southern African Large Telescope (SALT).

Author

O'Donoghue, Darragh E., Atad-Ettedgui, Eli, Balona, Luis, Bigelow, Bruce C., Booth, John A., Botha, Lucian, Brink, Janus D., Buckley, David A. H., Charles, Phil, Christians, Alrin, Clemens, J. Christopher, Crause, Lisa A., Crawford, Steven M., Evans, Geoffrey P., Gajjar, Hitesh, Hashimoto, Yas, Hendricks, Malcolm, Kniazev, Alexei, Koeslag, Anthony R., and Koorts, Willie P.

Published
2008
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6. Metal-Rich SX Phe Stars in the Kepler Field.

Author

Nemec, James M., Balona, Luis A., Kinemuchi, Karen, Murphy, Simon J., Young-Beom Jeon, Kurtz, Donald W., and Pigulski, Andrzej

Subjects
HIGH resolution spectroscopy, ASTRONOMICAL observations, ASTRONOMICAL photometry, RADIAL velocity of stars
Abstract

High-resolution spectroscopic observations have been made for 32 of the 34 candidate SX Phe stars identified in the Kepler field by Balona & Nemec (2012). All available long-and short-cadence Q0-Q17 Kepler photometry has been analyzed for the 34 candidates. Radial velocities (RVs), space motions (U, V, W), projected rotation velocities (υ sin i), spectral types, and atmospheric characteristics (Teff, log g, [M/H], υmic, etc.) were derived from ~ 160 spectra taken with the ESPaDOnS spectrograph on the Canada-France-Hawaii 3.6-m telescope and with the ARCES spectrograph on the Apache Point Observatory 3.5-m telescope. Two thirds of the stars are fast rotators with υ sin i > 50 km/s, including four stars with υ sin i > 200 km/s. Three of the stars have (negative) RVs > 250 km/s and retrograde space motions, and seven stars have total space motions > 400 km/s. All the spectroscopically measured SX Phe candidates have positions in a Toomre diagram that are consistent with being bona fide halo and thick-disk stars. Although several stars show a marked metal weakness, the mean [Fe/H] of the sample is near 0.0 dex (σ ~ 0.25 dex), which is considerably more metal-rich than is normally expected for a sample of Pop. II stars. Observed pulsation frequency modulations and optical time delays suggest that at least eight of the SX Phe stars are in binary systems, some of which show significant RV variations. Six of the time-delay binaries have secondary masses ranging from 0.05 to 0.70 M☉ and orbital periods in the range 9 to 1570 days. Another star appears to be an ellipsoidal variable with a 2.3-day orbital period; and two other systems have orbital periods longer than the ~ 4-year sampling interval of the Kepler data. [ABSTRACT FROM AUTHOR]

Published
2015
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