Near-infrared luminosity function of galaxies in distant clusters

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Near-infrared luminosity function of galaxies in distant clusters

Near-infrared luminosity function of galaxies in distant clusters

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SED fitt<strong>in</strong>g with 9 passbands from B to 4.5μ<br />

B VR i z J K 3.6 4.5<br />

B VR i z J K 3.6 4.5<br />

VLT/FORS HST/ACS VLT/ISAAC Spitzer/IRAC

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EAA_ws1314_V14_summary.pdf

Vorlesung

6.1. Spektrallinien

Künstlicher Stern über dem Calar Alto (Teil 2)

Max-Planck-Institut für Astronomie - Jahresbericht 2007

Max-Planck-Institut für Astronomie - Jahresbericht 2009

Annual Report 2010

thesis pdf, 3MB

L4 Star formation Part III

Where lies the Peak of the Brown Dwarf Binary Separation ...

Sterrewacht Leiden - FTP Directory Listing

Annual Report 2011 Max Planck Institute for Astronomy

Trapezoidal Rule Integration

Science Case

SED fitt<strong>in</strong>g with 9 passbands from B to 4.5μ B VR i z J K 3.6 4.5 B VR i z J K 3.6 4.5 VLT/FORS HST/ACS VLT/ISAAC Spitzer/IRAC

Massive <strong>galaxies</strong> with old stars i-z CM @ z=1.24 Blakeslee et al. 2003 redshifts from R. Demarco (PhD Thesis)

Page 1 and 2: Near-infrared luminosity function o
Page 3 and 4: Distant Galaxy Clusters We studied
Page 5 and 6: RDCS J1252+2927 @ z=1.24(Rosati et
Page 7 and 8: The Lynx supercluster 2 galaxy clus
Page 9 and 10: The K-band luminosity function at z
Page 11 and 12: The K-band luminosity function at z
Page 13 and 14: The K * redshift evolution up to re
Page 15: The stellar mass function of cluste
Page 19: Conclusions - The evolution of the