WebPIMMS MM

A Mission Count Rate Simulator
Powered by PIMMS v3.9k

See the WebPIMMS User Guide or the PIMMS User Guide for help with WebPIMMS.

Convert From:	Into:

Input Energy Range (low-high):	keV	Units
	Angstroms
Output Energy Range (low-high):	keV	Units
	Angstroms

Source: Flux / Count Rate	(erg/cm²/s)
Source: Flux / Count Rate	(counts/s)	Redshift	Galactic nH (cm¯²)

Base Model	Intrinsic nH (cm¯²)	Photon index / keV	OR Enter Additional Raymond Smith Models
+ Model 2	Intrinsic nH (cm¯²)	Photon index / keV	Normalization Relative to Base Model	Energy at which the models are normalized (keV)
+ Model 3	Intrinsic nH (cm¯²)	Photon index / keV	Normalization Relative to Base Model	Energy at which the models are normalized (keV)
+ Gaussian: No Yes		Line Center Energy (keV)	Physical Width (keV)	Equivalent Width Relative to Base Mode (eV)

Note: The following parameters are mission dependent

CHANDRA: Frame time (s)
CHANDRA ACIS pile-up calculation only

Go to the standard WebPIMMS web interface.

For help in the use of WebPIMMS, see the WebPIMMS User Guide or the PIMMS User Guide

WebPIMMS is a Web version of the PIMMS (v3.9j) tool. PIMMS was developed by Koji Mukai at the HEASARC. The first Web version was developed at the SAX Data Center. The SAX PIMMS package was ported to and modified for the HEASARC Web site by Michael Arida.

This file was last modified on Thursday, 15-Oct-2009 18:03:46 BST

For feedback or questions on WebPIMMS, please contact Michael Arida. arida@milkyway.gsfc.nasa.gov

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