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dc.contributor.authorMcClintock, Jeffrey E.
dc.contributor.authorSteiner, James F.
dc.contributor.authorGrinberg, Victoria
dc.contributor.authorGarcia, Javier A.
dc.contributor.authorRemillard, Ronald A
dc.date.accessioned2015-02-18T16:44:35Z
dc.date.available2015-02-18T16:44:35Z
dc.date.issued2014-09
dc.date.submitted2014-04
dc.identifier.issn1538-4357
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1721.1/94589
dc.description.abstractWe fitted all of the several hundred RXTE PCA spectra of the Crab individually to a simple power-law model; the total number of counts in the composite spectrum is >10[superscript 9]. We then used the spectrum of residuals to derive a calibration tool, called pcacorr, that we apply to large samples of spectra for GX 339-4, H1743-322, and XTE J1550-564. Application of the tool improved the quality of all the fits, and the improvement is dramatic for spectra with [> over ~] 10[superscript 7] counts. The Crab residual spectrum is somewhat different for each of the five Proportional Counter Array (PCA) detectors, but it was relatively stable over the course of the mission. We recommend that pcacorr be routinely applied to spectra with [> over ~] 10[superscript 6] counts and that one include a systematic error of 0.1%, rather than the 0.5-1% value that has customarily been used. We expect that application of the tool will result in an increase in sensitivity of the PCA to faint spectral features by up to an order of magnitude.en_US
dc.language.isoen_US
dc.publisherIOP Publishingen_US
dc.relation.isversionofhttp://dx.doi.org/10.1088/0004-637x/794/1/73en_US
dc.rightsArticle is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.en_US
dc.sourceAmerican Astronomical Societyen_US
dc.titleAN EMPIRICAL METHOD FOR IMPROVING THE QUALITY OF RXTE PCA SPECTRAen_US
dc.typeArticleen_US
dc.identifier.citationGarcia, Javier A. et al. “AN EMPIRICAL METHOD FOR IMPROVING THE QUALITY OF RXTE PCA SPECTRA.” The Astrophysical Journal 794.1 (2014): 73. © 2014 The American Astronomical Societyen_US
dc.contributor.departmentMIT Kavli Institute for Astrophysics and Space Researchen_US
dc.contributor.mitauthorRemillard, Ronald Alanen_US
dc.contributor.mitauthorGrinberg, Victoriaen_US
dc.relation.journalThe Astrophysical Journalen_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dspace.orderedauthorsGarcia, Javier A.; McClintock, Jeffrey E.; Steiner, James F.; Remillard, Ronald A.; Grinberg, Victoriaen_US
dc.identifier.orcidhttps://orcid.org/0000-0003-2538-0188
mit.licensePUBLISHER_POLICYen_US
mit.metadata.statusComplete


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