Search Results - "Bult, P. M"

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  1. 1

    NICER-NuSTAR Observations of the Neutron Star Low-mass X-Ray Binary 4U 1735-44 by Ludlam, R. M., Cackett, E. M., García, J. A., Miller, J. M., Bult, P. M., Strohmayer, T. E., Guillot, S., Jaisawal, G. K., Malacaria, C., Fabian, A. C., Markwardt, C. B.

    Published in The Astrophysical journal (01-05-2020)
    “…We report on the first simultaneous Neutron Star Interior Composition Explore (NICER) and Nuclear Spectroscopic Telescope Array (NuSTAR) observations of the…”
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    Journal Article
  2. 2

    NICER Discovers mHz Oscillations in the "Clocked" Burster GS 1826−238 by Strohmayer, T. E., Gendreau, K. C., Altamirano, D., Arzoumanian, Z., Bult, P. M., Chakrabarty, D., Chenevez, J., Guillot, S., Guver, T., Homan, J., Jaisawal, G. K., Keek, L., Mahmoodifar, S., Miller, J. M., Ozel, F.

    Published in The Astrophysical journal (20-09-2018)
    “…We report the discovery with the Neutron Star Interior Composition Explorer (NICER) of mHz X-ray brightness oscillations from the "clocked burster" GS…”
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    Journal Article
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    NICER-NuSTAR Observations of the Neutron Star Low-Mass X-ray Binary 4U 1735-44 by Ludlam, R. M, Cackett, E. M, García, J. A, Miller, J. M, Bult, P. M, Strohmayer, T. E, Guillot, S, Jaisawal, G. K, Malacaria, C, Fabian, A. C, Markwardt, C. B

    Published 14-04-2020
    “…We report on the first simultaneous $NICER$ and $NuSTAR$ observations of the neutron star (NS) low-mass X-ray binary 4U 1735$-$44, obtained in 2018 August. The…”
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    Journal Article
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    A NICER Spectrum of MAXI J1535-571: Near-Maximal Black Hole Spin and Potential Disk Warping by Miller, J. M, Gendreau, K, Ludlam, R. M, Fabian, A. C, Altamirano, D, Arzoumanian, Z, Bult, P. M, Cackett, E. M, Homan, J, Kara, E, Neilsen, J, Remillard, R. A, Tombesi, F

    Published 11-06-2018
    “…We report on a NICER observation of the Galactic X-ray binary and stellar-mass black hole candidate, MAXI J1535-571. The source was likely observed in an…”
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    Journal Article
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    NuSTAR and NICER reveal IGR J17591-2342 as a new accreting millisecond X-ray pulsar by Sanna, A, Ferrigno, C, Ray, P. S, Ducci, L, Jaisawal, G. K, Enoto, T, Bozzo, E, Altamirano, D, Di Salvo, T, Strohmayer, T. E, Papitto, A, Riggio, A, Burderi, L, Bult, P. M, Bogdanov, S, Gambino, A. F, Marino, A, Iaria, R, Arzoumanian, Z, Chakrabarty, D, Gendreau, K. C, Guillot, S, Markwardt, C. B, Wolff, M. T

    Published 30-08-2018
    “…A&A 617, L8 (2018) We report on the discovery by the Nuclear Spectroscopic Telescope Array (NuSTAR) and the Neutron Star Interior Composition Explorer (NICER)…”
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    Journal Article
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    Detection of Reflection Features in the Neutron Star Low-Mass X-ray Binary Serpens X-1 with NICER by Ludlam, R. M, Miller, J. M, Arzoumanian, Z, Bult, P. M, Cackett, E. M, Chakrabarty, D, Dauser, T, Enoto, T, Fabian, A. C, Garcia, J. A, Gendreau, K. C, Guillot, S, Homan, J, Jaisawal, G. K, Keek, L, La Marr, B, Malacaria, C, Markwardt, C. B, Steiner, J. F, Strohmayer, T. E

    Published 02-05-2018
    “…We present Neutron Star Interior Composition Explorer (NICER) observations of the neutron star low-mass X-ray binary Serpens X-1 during the early mission phase…”
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    Journal Article
  10. 10

    Modelling the ice band towards HD 29647 by van de Bult, C. E. P. M., Mayo Greenberg, J.

    “…Calculations have been made on a core–mantle–mantle grain model whose outer mantle consists of dirty ice material accreted in a molecular cloud. The…”
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    Photochemical reactions in interstellar grains photolysis of CO, NH3, and H2O by Agarwal, V K, Schutte, W, Greenberg, J M, Ferris, J P, Briggs, R, Connor, S, Van de Bult, C P, Baas, F

    “…A simulation of the organic layer accreted onto interstellar dust particles was prepared by slow deposition of a CO:NH2:H2O gas mixture on an Al block at 10 K,…”
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    Ice in the Taurus molecular cloud: modelling of the 3-µm profile by van de Bult, C. E. P. M., Greenberg, J. Mayo, Whittet, D. C. B.

    “…Detailed calculations of the absorption by interstellar core–mantle particles with mantles of different compositions are compared with observations of the 3 µm…”
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    Journal Article
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