Search Results - "Bachetti, Matteo"

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    Stingray: A Modern Python Library for Spectral Timing by Huppenkothen, Daniela, Bachetti, Matteo, Stevens, Abigail L., Migliari, Simone, Balm, Paul, Hammad, Omar, Khan, Usman Mahmood, Mishra, Himanshu, Rashid, Haroon, Sharma, Swapnil, Ribeiro, Evandro Martinez, Blanco, Ricardo Valles

    Published in The Astrophysical journal (10-08-2019)
    “…This paper describes the design and implementation of stingray, a library in Python built to perform time series analysis and related tasks on astronomical…”
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    PINT: A Modern Software Package for Pulsar Timing by Luo, Jing, Ransom, Scott, Demorest, Paul, Ray, Paul S., Archibald, Anne, Kerr, Matthew, Jennings, Ross J., Bachetti, Matteo, van Haasteren, Rutger, Champagne, Chloe A., Colen, Jonathan, Phillips, Camryn, Zimmerman, Josef, Stovall, Kevin, Lam, Michael T., Jenet, Fredrick A.

    Published in The Astrophysical journal (01-04-2021)
    “…Abstract Over the past few decades, the measurement precision of some pulsar timing experiments has advanced from ∼10 μ s to ∼10 ns, revealing many subtle…”
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    Spectral and Timing Analysis of NuSTAR and Swift/XRT Observations of the X-Ray Transient MAXI J0637–430 by Lazar, Hadar, Tomsick, John A., Pike, Sean N., Bachetti, Matteo, Buisson, Douglas J. K., Connors, Riley M. T., Fabian, Andrew C., Fuerst, Felix, García, Javier A., Hare, Jeremy, Jiang, Jiachen, Shaw, Aarran W., Walton, Dominic J.

    Published in The Astrophysical journal (01-11-2021)
    “…Abstract We present results for the first observed outburst from the transient X-ray binary source MAXI J0637–430. This study is based on eight observations…”
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    Return to the Forgotten Ultraluminous X-Ray Source: A Broadband NICER+NuSTAR Study of NGC 4190 ULX-1 by Earnshaw, Hannah P., Bachetti, Matteo, Brightman, Murray, Fürst, Felix, Harrison, Fiona A., Middleton, Matthew, Ludlam, Renee, Pike, Sean N., Stern, Daniel, Walton, Dominic J.

    Published in The Astrophysical journal (18-06-2024)
    “…We observed the nearby and relatively understudied ultraluminous X-ray source (ULX) NGC 4190 ULX-1 jointly with Neutron Star Interior Composition Explorer…”
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    Timing Calibration of the NuSTAR X-Ray Telescope by Bachetti, Matteo, Markwardt, Craig B., Grefenstette, Brian W., Gotthelf, Eric V., Kuiper, Lucien, Barret, Didier, Cook, W. Rick, Davis, Andrew, Fürst, Felix, Forster, Karl, Harrison, Fiona A., Madsen, Kristin K., Miyasaka, Hiromasa, Roberts, Bryce, Tomsick, John A., Walton, Dominic J.

    Published in The Astrophysical journal (01-02-2021)
    “…The Nuclear Spectroscopic Telescope Array (NuSTAR) mission is the first focusing X-ray telescope in the hard X-ray (3-79 keV) band. Among the phenomena that…”
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    The Slowest Spinning X-Ray Pulsar in an Extragalactic Globular Cluster by Zolotukhin, Ivan Yu, Bachetti, Matteo, Sartore, Nicola, Chilingarian, Igor V., Webb, Natalie A.

    Published in The Astrophysical journal (20-04-2017)
    “…Neutron stars are thought to be born rapidly rotating and then exhibit a phase of rotation-powered pulsations as they slow down to 1-10 s periods. The…”
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    A multi-wavelength pipeline for pulsar searches by Pilia, Maura, Trois, Alessio, Bachetti, Matteo, Pellizzoni, Alberto, Atzeni, Giuseppe, Egron, Elise, Iacolina, Maria Noemi, Loru, Sara, Poddighe, Antonio, Vacca, Valentina

    “…Pulsar studies in the recent years have shown, more than others, to have benefited from a multi-wavelength approach. The INAF-Astronomical Observatory in…”
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    Accurate X-ray timing in the presence of systematic biases with simulation-based inference by Huppenkothen, Daniela, Bachetti, Matteo

    “…ABSTRACT Because many of our X-ray telescopes are optimized towards observing faint sources, observations of bright sources like X-ray binaries in outburst are…”
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    Hard X-Ray Flares and Spectral Variability in NGC 4395 ULX1 by Ghosh, Tanuman, Rana, Vikram, Bachetti, Matteo

    Published in The Astrophysical journal (01-10-2022)
    “…Abstract We report the detection of flaring events in NGC 4395 ULX1, a nearby ultraluminous X-ray source (ULX), for the first time, using recent XMM-Newton…”
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