Next: Generation from Ground Calibration Up: EMOS_REDIST Previous: EMOS_REDIST Contents . The redistribution parameters for the MOS cameras. ... Attributes: . None. Columns: . ... The central CCD of each MOS detector has developed a patch where the energy resolution is worse than the average. ... The energy bounds of PHA channels. ... The energy bounds of the PI channels, used to determine the equivalent energies of spectral channels in the redistribution matrix construction. ...

... Classes . ... casa . casa::Poisson . ... Poisson distribution. ... Poisson ( RNG *gen, Double mean=0.0) . Construct a random number generator for a Poisson distribution. virtual . ... mean () const . ... These function allow you to manipulate the parameters (mean) described above through the base class. virtual Vector < Double > . ... The second argument defines the parameters for this distribution as described in the synopsis. virtual casa::Poisson::~Poisson . ... Double casa::Poisson::mean . ...

... Up: Proposal Processing . ... ESO is prototyping a distributed ``Phase II'' system that will allow astronomers to prepare their observations at their home institutions, while maintaining a central repository for all observation data. ... ESO is developing a Phase II Proposal Preparation system (P2PP) to collect detailed scientific programme descriptions, in the form of observation blocks (OB). ... ESO's Phase II Proposal Preparation system is an integral part of the VLT Data Flow System (DFS). ...

... Science . ... Science Users Information > Science Activities > PhD Thesis Topics offered by ESO Faculty Members > Thesis Topic: Next generation Fornax Cluster surveys . ... Data Handling and Products . ... Science Data Products Forum . ... An international team, with Dr. Hilker as Co-PI, has started to gather wide-field optical and infrared imaging data as well as spectroscopic data on the whole extent of the Fornax cluster, mainly based on observations with ESO telescopes (VLT, VST, VISTA). ...

RPS2 Proposal Submission Software: Testing and Distribution of Periodically Updated Software Robert E. Douglas, Jr. PRESTO/SST Space Telescope Science Institute 3700 San Martin Drive Baltimore, MD 21218 Phone: (410) 338-4497 Fax: (410) 338-1592 Email: rdouglas@stsci.edu In 1995, the Space Telescope Science Institute (STScI) introduced RPS2 (Remote Proposal Submission 2nd Generation). RPS2 is used by Hubble Space Telescope (HST) proposers to prepare their detailed observation descriptions. ...

. Main Page . Related Pages . Classes . Files . Class List . Class Hierarchy . Class Members . #include < dustmodel.h > . List of all members. double . alpha . double . acutlarge . double . beta . double . at . double . C . Silicate dust size-distribution parameters . The documentation for this struct was generated from the following file: . dustmodel.h . Generated on Fri Jul 11 07:32:08 2008 for DUST by 1.5.5

... Galaxies 99 Cosmic background with model of cloudy interstellar medium Yu. ... Figure 1: Averaged spectrum of the cosmic background I f in frequency range 0.25 200 MHz for the Galactic poles. ... First interpretation of the cosmic noise background spectrum at broad band frequency range 0.25 200 MHz with a model of the cloudy interstellar medium ISM is presented here. ... Synthesized background spectra I f for regions of the Galactic poles at the frequency range 0.25 200 MHz is presented in Fig. ...