xte.mit.edu

MIT X-Ray Timing Explorer Project

The X-Ray Timing Explorer Project. At 8:48 EST Saturday December 30, 1995. Analysis and Instrument Status. The X-ray Timing Explorer. A NASA mission originally scheduled. For launch in August 1995, is designed to facilitate the study of time variability in the emission of X-ray sources with moderate spectral resolution. Time scales from microseconds to months are covered in an instantaneous spectral range from 2 to 250 keV. It is designed for a required life time of two years, a goal of five years. Will ...

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MIT X-Ray Timing Explorer Project | xte.mit.edu Reviews

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The X-Ray Timing Explorer Project. At 8:48 EST Saturday December 30, 1995. Analysis and Instrument Status. The X-ray Timing Explorer. A NASA mission originally scheduled. For launch in August 1995, is designed to facilitate the study of time variability in the emission of X-ray sources with moderate spectral resolution. Time scales from microseconds to months are covered in an instantaneous spectral range from 2 to 250 keV. It is designed for a required life time of two years, a goal of five years. Will ...

<META> KEYWORDS

1 xte was launched

2 asm light curves

3 one day averages

4 source activity

5 source list

6 main page

7 at the nasa

8 technical information

9 engineering data

10 updated periodically

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xte was launched,asm light curves,one day averages,source activity,source list,main page,at the nasa,technical information,engineering data,updated periodically,documents about xte,an html version,the flight documents,staff,scientists,ed morgan,wei cui

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MIT X-Ray Timing Explorer Project | xte.mit.edu Reviews

https://xte.mit.edu

The X-Ray Timing Explorer Project. At 8:48 EST Saturday December 30, 1995. Analysis and Instrument Status. The X-ray Timing Explorer. A NASA mission originally scheduled. For launch in August 1995, is designed to facilitate the study of time variability in the emission of X-ray sources with moderate spectral resolution. Time scales from microseconds to months are covered in an instantaneous spectral range from 2 to 250 keV. It is designed for a required life time of two years, a goal of five years. Will ...

INTERNAL PAGES

xte.mit.edu

1

ASM STATUS

http://xte.mit.edu/asm_status.html

Analysis and Instrument Status Source Activity. ASM Status Report for 27 April, 1996. Dramatic variability from the galactic binary ("microquasar") 1915 10 was noted in the ASM data. This was the first ASM TOO which led to PCU observations that are rich in temporal variability. Results will be reported at the HEAD meeting by Greiner, Morgan, and Remillard. ASM Status Report for 30 August, 1996. Analysis Status (enlarged source catalog and improved light curves). The light curves currently posted "through...

2

ASM Light Curves Overview

http://xte.mit.edu/asmlc/ASM.html

3

ASM Light Curves

http://xte.mit.edu/asmlc/One-Day.html

Quick-look results provided by the ASM/RXTE team. Web page design and software coding by Derek Fox. Data solutions currently run through Week 831 (continuous coverage from 2/20/96 to 12/31/2011). Sources are listed in order of increasing right ascension. Plots show the most recent year's data, but the data files are Mission-complete. Reduced chi-square of the fit 1.4, except for Sco X-1 4.0. Number of sources in the field of view 40. Earth angle 75 degrees. Exposure time 30 seconds.

4

ASM source list

http://xte.mit.edu/asmlc/ptplot/lightcurves/sources.html

The ASM Light Curves Page. If you do not have a Java and JavaScript enabled browser then you will not be able to view the light curves of these sources. Algol, Beta Per, x0304 407. Aqlx1, V133Aq1, x1908 005. Cenx3, x1119-603, V779Cen. Cirx1, BR Cir, x1516-569. Crab, x0531 219, CM Tau. Cygx1, HDE226868, V1357Cyg, x1956 350. Cygx2, V1341Cyg, x2141 380. Cygx3, V1521Cyg, x2030 407. Dmuma, BD 61°1211, x1052 607. Gammacas, HD144, x0053 604. Gkper, x0327 437. Gx1 4, V2116 Oph, x1728-247. Gx13 1, x1811-171.

5

ASM Announcements

http://xte.mit.edu/xte_anno.html

Source Activity Data Extraction. 1 Crab = 74 SSC cts/sec. Weeks 736-743 results (2010 March 5 - April 29). LSV 4417 - an outburst was seen from MJD 55285 to MJD 55303 with a weak flux of 100 mcrab near MJD 55292. 3C 129 - showed significant emission for 10 to 15 days following (about) MJD 55290; the peak flux was 50 mcrab. X0512-401 - possibly was as strong as 25 mcrab for a few days. X0535 262 - was in outburst from MJD 55275 to MJD 55310; the peak flux was about 330 mcrab. Mkn 421 - 50 mcrab. Week 731 ...

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space.mit.edu

RXTE | MIT Kavli Institute for Astrophysics and Space Research

http://space.mit.edu/instrumentation/rxte

MIT KAVLI INSTITUTE FOR ASTROPHYSICS AND SPACE RESEARCH. Job Opportunities and Fellowships. Tools for MKI Community. The MIT Kavli Institute paves the way for new developments in space- and ground-based astrophysics. Our faculty, research staff, and students develop technology and instrumentation with a focus on an engineering and technical core. We are comprised of the MIT Department of Physics. MIT School of Engineering. MIT EAPS (Earth, Atmospheric and Planetary Sciences). Neutron Stars and Black Holes.

space-dev.mit.edu

RXTE | MIT Kavli Institute for Astrophysics and Space Research

http://space-dev.mit.edu/instrumentation/rxte

MIT KAVLI INSTITUTE FOR ASTROPHYSICS AND SPACE RESEARCH. Job Opportunities and Fellowships. Tools for MKI Community. The MIT Kavli Institute paves the way for new developments in space- and ground-based astrophysics. Our faculty, research staff, and students develop technology and instrumentation with a focus on an engineering and technical core. We are comprised of the MIT Department of Physics. MIT School of Engineering. MIT EAPS (Earth, Atmospheric and Planetary Sciences). Neutron Stars and Black Holes.

space-live.mit.edu

RXTE | MIT Kavli Institute for Astrophysics and Space Research

http://space-live.mit.edu/instrumentation/rxte

MIT KAVLI INSTITUTE FOR ASTROPHYSICS AND SPACE RESEARCH. Job Opportunities and Fellowships. Tools for MKI Community. The MIT Kavli Institute paves the way for new developments in space- and ground-based astrophysics. Our faculty, research staff, and students develop technology and instrumentation with a focus on an engineering and technical core. We are comprised of the MIT Department of Physics. MIT School of Engineering. MIT EAPS (Earth, Atmospheric and Planetary Sciences). Neutron Stars and Black Holes.

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MIT X-Ray Timing Explorer Project

The X-Ray Timing Explorer Project. At 8:48 EST Saturday December 30, 1995. Analysis and Instrument Status. The X-ray Timing Explorer. A NASA mission originally scheduled. For launch in August 1995, is designed to facilitate the study of time variability in the emission of X-ray sources with moderate spectral resolution. Time scales from microseconds to months are covered in an instantaneous spectral range from 2 to 250 keV. It is designed for a required life time of two years, a goal of five years. Will ...

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