Hostname: page-component-cd9895bd7-lnqnp Total loading time: 0 Render date: 2024-12-23T10:32:05.504Z Has data issue: false hasContentIssue false

Flux Calibration Issues

Published online by Cambridge University Press:  01 December 2006

Andrew J. Pickles*
Affiliation:
Caltech, 1200 E. California Blvd., Pasadena, CA 91225, USA email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Recent stellar spectral libraries have sought higher resolution and the accurate determination of specific optical spectral indeces as stellar population indicators. But the value of accurate flux comparisons over wide wavelength regions should still be emphasized, particularly as more and better spectro-photometric data for composite populations becomes available.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2007

References

Bagnuolo, S., Jehin, E., Ledoux, C., Cabanac, R., Melo, C. & Gilmozzi, R. 2003, ESO Messenger 114, 10Google Scholar
Bessell, M. S. 2005, Ann. Rev. 43, 293Google Scholar
Bruzual, G. & Charlot, S. 2003, MNRAS 344, 1000CrossRefGoogle Scholar
Cenarro, A.J., Peletier, R.F., Sánchez-Blázquez, P, Selam, S.O., Toloba, E., Cardiel, N., Falcón-Barroso, J, Gorgas, J., Jiménez-Vicente, J. & Vazdekis, A. 2007, MNRAS 374, 664CrossRefGoogle Scholar
Cohen, M., Walker, R. G., Carter, B, Hammersley, P., Kidger, M. & Noguchi, K. 1999, A J, 117, 1864CrossRefGoogle Scholar
Cushing, M. C., Vacca, W. D. R & ayner, J. T. 2004, PASP 116, 362CrossRefGoogle Scholar
Gregg, M. D., Silva, D., Rayner, J., Valdes, F., Worthey, G., Pickles, A., Rose, J. A., Vacca, W. & Carney, B. 2004, BAAS 36, 1496Google Scholar
Hamuy, M., Walker, A. R., Suntzeff, N. B., Gigoux, P., Heathcote, S. R. & Phillips, M. M. 1992 PASP 104, 533CrossRefGoogle Scholar
Hamuy, M., Suntzeff, N. B., Heathcote, S. R., Walker, A. R., Gigoux, P. & Phillips, M. M. 1994 PASP 106, 566CrossRefGoogle Scholar
Lançon, A. & Wood, P. R. 2000, A&AS 146, 217Google Scholar
Le Borgne, J.-F., Bruzual, G., Pelló, R., Lançon, A., Rocca-Volmerange, B., Sanahuja, B., Schaerer, D., Soubiran, C. & Vílchez-Gómez, R. 2003, A&A 402, 433LGoogle Scholar
Le Borgne, D., Rocca-Volmerange, B., Prugniel, P., Lançon, A., Fioc, M. & Soubiran, C. 2004, A&A 425, 881Google Scholar
Maíz Apellániz, J. 2006, ApJ 131, 1184CrossRefGoogle Scholar
Mermilliod, J.-C., Mermilliod, M. & Hauck, B. 1997, A&AS 124, 349Google Scholar
Munari, U., Sordo, R., Castelli, F. & Zwitter, T. 2005 A&A 442, 1127Google Scholar
Pickles, A. J. 1998, PASP 110, 863CrossRefGoogle Scholar
Prugniel, Ph., & Soubiran, C. 2001, A&A 369, 1048Google Scholar
Prugniel, Ph., & Soubiran, C. 2004, astro.ph 0409214Google Scholar
Rayner, J. T, Toomey, D. W., Onaka, P. M., Denault, A. J., Stahlberger, W. E., Vacca, W. D., Cushing, M. C. & Wang, S. 2003, PASP 115, 362CrossRefGoogle Scholar
Sánchez-Blázquez, P., Peletier, R.F., Jiménez-Vicente, J., Cardiel, N., Cenarro, A. J., Falcón-Barroso, J., Gorgas, J., Selam, S. & Vazdekis, A. 2006, MNRAS 371, 703CrossRefGoogle Scholar
Vacca, W. D., Cushing, M. C. & Rayner, J. T 2003, PASP 115, 389CrossRefGoogle Scholar
Valdes, F., Gupta, R., Rose, J. A., Singh, H. P. & Bell, D. J. 2004, ApJS 152, 251CrossRefGoogle Scholar