8 results
An older, more quiescent universe from panchromatic SED fitting of the 3D-HST survey
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- Journal:
- Proceedings of the International Astronomical Union / Volume 15 / Issue S352 / June 2019
- Published online by Cambridge University Press:
- 04 June 2020, pp. 99-102
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- June 2019
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Probing Galactic Outskirts with Dragonfly
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- Journal:
- Proceedings of the International Astronomical Union / Volume 11 / Issue S321 / March 2016
- Published online by Cambridge University Press:
- 21 March 2017, pp. 137-146
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- March 2016
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Hα Equivalent Widths from the 3D-HST survey: evolution with redshift and dependence on stellar mass†
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- Journal:
- Proceedings of the International Astronomical Union / Volume 8 / Issue S295 / August 2012
- Published online by Cambridge University Press:
- 17 July 2013, p. 91
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- August 2012
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Which Galaxy Property Best Predicts Quiescence?
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- Journal:
- Proceedings of the International Astronomical Union / Volume 8 / Issue S295 / August 2012
- Published online by Cambridge University Press:
- 17 July 2013, p. 177
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- August 2012
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What drives the star formation in early-type galaxies at late epochs? - the case for minor mergers
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- Journal:
- Proceedings of the International Astronomical Union / Volume 5 / Issue S262 / August 2009
- Published online by Cambridge University Press:
- 13 April 2010, pp. 168-171
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- August 2009
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E+A galaxies in intermediate redshift clusters
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- Journal:
- Proceedings of the International Astronomical Union / Volume 2004 / Issue IAUC195 / March 2004
- Published online by Cambridge University Press:
- 06 October 2004, pp. 483-487
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- March 2004
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Measuring the Evolution of the Mass-to-Light Ratio from z = 0 to z = 0.6 from the Fundamental Plane
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- Journal:
- Symposium - International Astronomical Union / Volume 186 / 1999
- Published online by Cambridge University Press:
- 25 May 2016, pp. 447-457
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- 1999
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Measuring the Evolution of the M/L ratio from the Fundamental Plane in Cl 0024+16 at z=0.39
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- Journal:
- Symposium - International Astronomical Union / Volume 171 / 1996
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- 25 May 2016, pp. 233-240
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- 1996
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