From lpd@head-cfa.harvard.edu Fri Oct 3 10:46:21 1997 Return-Path: Received: from space.mit.edu (space [18.75.0.10]) by wiwaxia.mit.edu with SMTP id KAA11962 for ; Fri, 3 Oct 1997 10:46:21 -0400 (EDT) Received: from head-cfa (head-cfa.harvard.edu) by space.mit.edu AA19380; Fri, 3 Oct 97 10:46:16 EDT Received: from cfa271 by head-cfa (SMI-8.6/SMI-SVR4) id KAA02371; Fri, 3 Oct 1997 10:46:02 -0400 Message-Id: <199710031446.KAA02371@head-cfa> To: dd@head-cfa.harvard.edu Date: Fri, 03 Oct 1997 10:46:02 -0400 From: Larry David Status: R Content-Length: 36876 ------- Forwarded Message Return-Path: Received: from beida by head-cfa (SMI-8.6/SMI-SVR4) id KAA01982; Fri, 3 Oct 1997 10:38:07 -0400 Received: by beida (SMI-8.6/SMI-SVR4) id KAA02359; Fri, 3 Oct 1997 10:38:06 -0400 Date: Fri, 3 Oct 1997 10:38:06 -0400 From: zhao@beida (Ping Zhao) Message-Id: <199710031438.KAA02359@beida> To: lpd@beida X-UIDL: 96f0a89d0826700435f5b81ec955b1f7 Status: U HRMA On-orbit On-axis Effective Area Coating: 97.25% bulk Ir Energy Shell 1 Shell 3 Shell 4 Shell 6 HRMA (keV) (cm2) (cm2) (cm2) (cm2) (cm2) - --------------------------------------------------------------------- - --------------------------------------------------------------------- ------- End of Forwarded Message From lpd@cfa271.harvard.edu Fri Oct 3 10:46:10 1997 Return-Path: Received: from space.mit.edu (space [18.75.0.10]) by wiwaxia.mit.edu with SMTP id KAA11957 for ; Fri, 3 Oct 1997 10:46:09 -0400 (EDT) Received: from head-cfa (head-cfa.harvard.edu) by space.mit.edu AA19363; Fri, 3 Oct 97 10:46:02 EDT Received: from cfa271 by head-cfa (SMI-8.6/SMI-SVR4) id KAA02359; Fri, 3 Oct 1997 10:45:55 -0400 Received: by cfa271 (SMI-8.6/SMI-SVR4) id KAA07191; Fri, 3 Oct 1997 10:45:48 -0400 Date: Fri, 3 Oct 1997 10:45:48 -0400 From: lpd@cfa271.harvard.edu (Larry David) Message-Id: <199710031445.KAA07191@cfa271> To: dd@cfa271.harvard.edu Subject: HRMA effective area Status: R Content-Length: 430 Hi Dan, I'm forwarding the latest calculations of the HRMA effective area to you in the next email. These are the same numbers used in the SIN and are based on raytrace simulations by Ping Zhao. Note - the simulated effective areas still disagree with XRCF measurements at the 10% level. Below 2keV Henke coefficients are used, while above 2 keV synchrotron measurements are used to determine the optical coeficients. Larry