[no subject]

["Ming F. Gu" <mfgu@stanford.edu>]

Dear Conference organizor,
I have two abstract to submit as attached. The registration form is 
included below.
Thanks.

Registration form
--------------------------------------------------------------------------------
Last name: Gu
First name: Ming
Middle name/initial: F.
Affiliation: Stanford University
Street Address: 382 Via Pueblo, Varian 334. 
City: Stanford
State: CA
Postal Code: 94305
Country: USA
Tel: 650-723-1775
Fax: 650-926-8908
E mail: mfgu@stanford.edu
Citizenship*: P.R. China
Abstract title:
1. Laboratory Measurement and Theoretical Modeling of K-shell X-ray Lines
   from Inner-shell Excited and Ionized Ions of Oxygen
2. Laboratory Survey of Fe L-shell X-ray Emission Lines between 7 and 11~{\AA}
Special requirements:


=======================
 Ming Feng Gu
 Stanford University
 650-723-1775
 mfgu@stanford.edu
=======================
\documentclass{article}

\begin{document}

\title{Laboratory Measurement and Theoretical Modeling of K-shell X-ray Lines       
   from Inner-shell Excited and Ionized Ions of Oxygen}

\author{
Ming Feng Gu$^1$ \and
Mike Schmidt$^{2,3}$ \and
Peter Beiersdorfer$^2$ \and
Hui Chen$^2$ \and
Daniel B. Thorn$^2$ \and
Elmar Tr\"{a}bert$^{2,4}$ \and
Ehud Behar$^5$ \and
Steven M. Kahn$^1$
}
\maketitle

\begin{abstract}
We present high resolution laboratory spectra of K-shell X-ray lines from
inner-shell excited and ionized ions of oxygen, obtained with a reflection
grating spectrometer on the electron beam ion trap (EBIT-I) at the Lawrence
Livermore National Laboratory. Only with a multi-ion model including all major
atomic collisional and radiative processes, are we able to identify the
observed K-shell transitions of oxygen ions from O III to O VI. The
wavelengths and associated
errors for some of the strongest transitions are given, taking into
account both the experimental and modeling uncertainties. The present data
should be useful in identifying the absorption features present in
astrophysical sources, such as active galactic nuclei and X-ray
binaries. They are also useful in providing benchmarks for the testing of
theoretical atomic structure calculations.

The work at Lawrence Livermore National Laboratory was performed under
the auspices of the Department of Energy under Contract No. W-7405-Eng-48
and was supported by the National Aeronautics and Space
Administration under work order W19,878 issued by the Space
Astrophysics Research and Analysis Program. M.F.G and S.M.K acknowledge the
support by the NASA grant NAG5-5419.
E.T. acknowledges travel support from the German Research Association (DFG).
E.B. was supported by grant No. 2002111 from the United States Israel
Binational Foundation.
\end{abstract}

\noindent
$^{1}$Kavli Institute for Particle Astrophysics and Cosmology,
and \\ Department of Physics, Stanford University, CA 94305, USA\\
$^{2}$High Temperature and Astrophysics Division,\\ Lawrence
Livermore National Laboratory, Livermore, CA 94550-9234, USA\\
$^{3}$Technische Universit\"{a}t Dresden, Germany\\
$^{4}$Ruhr-Universit\"{a}t Bochum, Germany\\
$^{5}$Department of Physics, Technion, Haifa 32000, Israel\\

\end{document}
\documentclass{article}

\begin{document}

\title{Laboratory Survey of Fe L-shell X-ray Emission Lines between 7 and 11~{\AA}}

\author{
Ming Feng Gu$^1$ \and
Hui Chen$^2$ \and
Peter Beiersdorfer$^2$ \and
Greg V. Brown$^2$ \and
Daniel B. Thorn$^2$ \and
Steven M. Kahn$^1$
}
\maketitle
\begin{abstract}
We present a comprehensive survey of Fe L-shell X-ray lines between 7 and
11~{\AA} using the electron beam ion trap at the Lawrence Livermore National
Laboratory. A set of flat crystal spectrometers are used to measure the
wavelengths of all significant Fe emission lines in the 7--11~{\AA} range,
most of them being transitions from high $n$ (up to $n=10$) configurations to
the $n=2$ shell. The identification and assignment of transitions are made
with the help of detailed theoretical modeling using the Flexible Atomic
Code. The present work is an extension of Brown et~al. (2002, ApJ 140, 589)
where Fe lines above 10.6~{\AA} are measured and identified. The combination
of the previous and the present work provides the most extensive and accurate
laboratory X-ray line list for Fe L-shell ions to date.

The work at Lawrence Livermore National Laboratory was performed under
the auspices of the Department of Energy under Contract No. W-7405-Eng-48
and was supported by the National Aeronautics and Space
Administration under work order W19,878 issued by the Space
Astrophysics Research and Analysis Program. M.F.G and S.M.K acknowledge the
support by the NASA grant NAG5-5419.
\end{abstract}

\noindent
$^{1}$Kavli Institute for Particle Astrophysics and Cosmology,
and \\ Department of Physics, Stanford University, CA 94305, USA\\
$^{2}$High Temperature and Astrophysics Division,\\ Lawrence
Livermore National Laboratory, Livermore, CA 94550-9234, USA\\

\end{document}