... JWST . ... The formation and evolution of galaxies I: the deep imaging survey(s) by Simon Lilly, Mike Fall, Massimo Stiavelli, Piero Madau, Avi Loeb, Jon Gardner, Marcia Rieke . ... The formation and evolution of galaxies IV: the relation between galaxy evolution and AGN by Simon Lilly, Mike Fall, Massimo Stiavelli, Piero Madau, Avi Loeb, Jon Gardner, Marcia Rieke, Robert Fosbury . ... The evolution of the cosmic supernova rates (revised April 1999) by Piero Madau, Robert Kirshner, Andrea Ferrara . ...
... Complex astrophysical phenomena could now be studied spectroscopically: the X-ray absorption line forest intrinsic to Seyfert galaxies; the interaction between AGN jets and intracluster media; hot winds of starburst galaxies; stellar coronal plasmas; the charge -exchange emission of Mars' exosphere; the X-ray irradiation of protoplanetary disks; and the myst erious flat-topped spectral line shapes of O star winds. ... We estimate that Gen-X will be able to detect and resolve 20, 000 stars in NGC...
THE ASTRONOMICAL JOURNAL, 116 : 1009 х1038, 1998 September ( 1998. The American Astronomical Society. All rights reserved. Printed in U.S.A. OBSERVATIONAL EVIDENCE FROM SUPERNOVAE FOR AN ACCELERATING UNIVERSE AND A COSMOLOGICAL CONSTANT ADAM G. RIESS,1 ALEXEI PETER M. GARNAVICH,2 B. LEIBUNDGUT,6 M. R. V. FILIPPENKO,1 PETER CHALLIS,2 ALEJANDRO CLOCCHIATTI,3 ALAN DIERCKS,4 RON L. GILLILAND,5 CRAIG J. HOGAN,4 SAURABH JHA,2 ROBERT P. KIRSHNER,2 M. PHILLIPS,7 DAVID REISS,4 BRIAN P. SCHMIDT,8,9 ROBERT A.
ST-ECF Instrument Science Report WFC3-2009-17 WFC3 SMOV proposal 11552: Calibration of the G141 grism H. Kuntschner, H. Bushouse, M. KЭmmel, J. R. Walsh October 16, 2009 A BSTR A C T Based on the SMOV observations, the performance of the WFC3 near-IR grism G141 has been assessed. ... Figure 2: Image of the G141 grism exposure (iab908s4q_flt.fits). ... 12 2 ST-ECF Technical Instrument Report WFC3-2009-17 Figure 5: Linear fit for the wavelength solution of the G141 grism. ...
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CORES OR CUSPS IN ELLIPTICAL GALAXIES: LUMINOSITY OR ENVIRONMENT? ... The low lumi nosity disky galaxies have `hard' cores with a steep slope in the luminosity profile at small radii, whereas the luminous galaxies have `soft' cores with flat profiles at small radii (e.g. Faber et al. ... Coma Cluster cores In the gas/stellar continuum paradigm, one would expect that in the outer parts of a cluster it is more likely that the last merger was gaseous than in its central regions. ...