Blanco, Philip R. - Center for Astrophysics & Space Sciences, University of California at San Diego

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• TABLE 1. Observation dates, livetimes (s), and background subtracted count rates (counts s 01 ) for the 4 ROSAT HRI observations of N49.
• THE ASTROPHYSICAL JOURNAL, 562 499507, 2001 November 20 ( 2001. The American Astronomical Society. All rights reserved. Printed in U.S.A.
• The Astrophysical Journal, 511:L21L24, 1999 January 20 1999. The American Astronomical Society. All rights reserved. Printed in U.S.A.
• FIG. 3. Total power spectrum from both RX 05256604 (left) and a simulated pulsar (right) for periods from 7:58:5 s. The power spectra represents the sum of
• accepted for publication in Astrophysical Journal (Letters) H I absorption toward the nucleus of the
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• The Astrophysical Journal, 554:L33--L36, 2001 June 10 # 2001. The American Astronomical Society. All rights reserved. Printed in U.S.A.
• The Astrophysical Journal, 502:L129--L132, 1998 August 1 q 1998. The American Astronomical Society. All rights reserved. Printed in U.S.A.
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• square wave characterized by a broad duty cycle (0:5), an initial period of 8 s, and a period derivative of
• The Astrophysical Journal, 521:L49--L53, 1999 August 10 # 1999. The American Astronomical Society. All rights reserved. Printed in U.S.A.
• The Astrophysical Journal, 520:L107L110, 1999 August 1 1999. The American Astronomical Society. All rights reserved. Printed in U.S.A.
• H I ABSORPTION TOWARD THE NUCLEUS OF THE POWERFUL RADIO GALAXY CYGNUS A: EVIDENCE FOR AN ATOMIC OBSCURING TORUS?
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• Astron. Astrophys. 341, 141--150 (1999) ASTRONOMY ASTROPHYSICS
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• THE CONTINUOUS HARD XRAY IMAGER FOR ASTROPHYSICS Richard E. Rothschild, James L. Matteson, William A. Heindl, and Laurence E. Peterson
• Astron. Astrophys. 342, 736744 (1999) ASTROPHYSICS
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• EVIDENCE OF XRAY SYNCHROTRON EMISSION FROM ELECTRONS ACCELERATED TO 40 TeV IN THE SUPERNOVA REMNANT CASSIOPEIA A
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• The Astrophysical Journal, 489:L51--L54, 1997 November 1 q 1997. The American Astronomical Society. All rights reserved. Printed in U.S.A.
• The High Energy XRay Timing Experiment P. R. Blanco, R. E. Rothschild & the HEXTE team.
• RXTE OBSERVATIONS OF A NEW XRAY TRANSIENT: GRS 1737231 WEI CUI, 1 W. A. HEINDL, 2 J. H. SWANK, 3 D. M. SMITH, 4 E. H. MORGAN, 1 R. REMILLARD, 1 AND F. E. MARSHALL 3
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• A&A 371, 858864 (2001) DOI: 10.1051/0004-6361:20010438
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• PASJ: Publ. Astron. Soc. Japan 48, 389--394 (1996) Detection of Hard Xray Emission in Mkn 463
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• Nonlinear Elasticity, Proteinquakes and the Energy Landscapes of Functional Transitions in Proteins
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• The Astrophysical Journal, 502:L129L132, 1998 August 1 1998. The American Astronomical Society. All rights reserved. Printed in U.S.A.
• HEXTE Feasibility of Observations P. R. Blanco & the HEXTE team
• (pblanco@ucsd.edu) (dgruber@ucsd.edu)
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• RXTE OBSERVATIONS OF A NEW X-RAY TRANSIENT: GRS 1737 31 WEI CUI,1 W. A. HEINDL,2 J. H. SWANK,3 D. M. SMITH,4 E. H. MORGAN,1 R. REMILLARD,1 AND F. E. MARSHALL3
• THE ASTROPHYSICAL JOURNAL, 563 229238, 2001 December 10 ( 2001. The American Astronomical Society. All rights reserved. Printed in U.S.A.
• FIG. 2. 6100 A(left) and OIII (right) images of N49 with the smoothed Xray con tours and bestfit error circle of RX 05256604 overplotted.
• The Astrophysical Journal, 519:L165--L168, 1999 July 10 # 1999. The American Astronomical Society. All rights reserved. Printed in U.S.A.
• FIG. 1. Smoothed image of N49 obtained with the ROSAT High Resolution Im ager. The image was obtained from 4 observations, with a total of 50000 s of
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