Search Results - "D’Agostino, Joshua J"

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  1. 1

    The effects of diffuse ionized gas and spatial resolution on metallicity gradients: TYPHOON two-dimensional spectrophotometry of M83 by Poetrodjojo, Henry, D’Agostino, Joshua J, Groves, Brent, Kewley, Lisa, Ho, I-Ting, Rich, Jeff, Madore, Barry F, Seibert, Mark

    “…Abstract We present a systematic study of the diffuse ionized gas (DIG) in M83 and its effects on the measurement of metallicity gradients at varying…”
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    Journal Article
  2. 2

    A new diagnostic to separate line emission from star formation, shocks, and AGNs simultaneously in IFU data by D'Agostino, Joshua J, Kewley, Lisa J, Groves, Brent A, Medling, Anne, Dopita, Michael A, Thomas, Adam D

    “…ABSTRACT In the optical spectra of galaxies, methods for the separation of line emission arising from star formation and an additional hard component, such as…”
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    Journal Article
  3. 3

    Comparison of Theoretical Starburst Photoionization Models for Optical Diagnostics by D'Agostino, Joshua J., Kewley, Lisa J., Groves, Brent, Byler, Nell, Sutherland, Ralph S., Nicholls, David, Leitherer, Claus, Stanway, Elizabeth R.

    Published in The Astrophysical journal (10-06-2019)
    “…We study and compare different examples of stellar evolutionary synthesis input parameters used to produce photoionization model grids using the MAPPINGS V…”
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    Journal Article
  4. 4
  5. 5

    Separating line emission from star formation, shocks, and AGN ionization in NGC 1068 by D’Agostino, Joshua J, Kewley, Lisa J, Groves, Brent A, Medling, Anne M, Di Teodoro, Enrico, Dopita, Michael A, Thomas, Adam D, Sutherland, Ralph S, Garcia-Burillo, Santiago

    “…ABSTRACT In the optical spectra of galaxies, the separation of line emission from gas ionized by star formation and an active galactic nucleus (AGN), or by…”
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    Journal Article
  6. 6

    Comparison of Theoretical Starburst Photoionisation Models for Optical Diagnostics by D'Agostino, Joshua J, Kewley, Lisa J, Groves, Brent, Byler, Nell, Sutherland, Ralph S, Nicholls, David, Leitherer, Claus, Stanway, Elizabeth R

    Published 07-06-2019
    “…We study and compare different examples of stellar evolutionary synthesis input parameters used to produce photoionisation model grids using the MAPPINGS V…”
    Get full text
    Journal Article
  7. 7

    A New Diagnostic to Separate Line Emission from Star Formation, Shocks, and AGN Simultaneously in IFU Data by D'Agostino, Joshua J, Kewley, Lisa J, Groves, Brent A, Medling, Anne, Dopita, Michael A, Thomas, Adam D

    Published 26-02-2019
    “…In the optical spectra of galaxies, methods for the separation of line emission arising from star formation and an additional hard component, such as shocks or…”
    Get full text
    Journal Article
  8. 8

    The Effects of Diffuse Ionized Gas and Spatial Resolution on Metallicity Gradients: TYPHOON Two-Dimensional Spectrophotometry of M83 by Poetrodjojo, Henry, D'Agostino, Joshua J, Groves, Brent, Kewley, Lisa, Ho, I-Ting, Rich, Jeff, Madore, Barry F, Seibert, Mark

    Published 08-05-2019
    “…We present a systematic study of the diffuse ionized gas (DIG) in M83 and its effects on the measurement of metallicity gradients at varying resolution scales…”
    Get full text
    Journal Article
  9. 9

    Starburst-AGN mixing: TYPHOON observations of NGC 1365, NGC 1068, and the effect of spatial resolution on the AGN fraction by D'Agostino, Joshua J, Poetrodjojo, Henry, Ho, I-Ting, Groves, Brent, Kewley, Lisa, Madore, Barry F, Rich, Jeff, Seibert, Mark

    Published 31-07-2018
    “…We demonstrate a robust method of resolving the star-formation and AGN contributions to emission lines using two very well known AGN systems: NGC 1365, and NGC…”
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    Journal Article
  10. 10

    Separating Line Emission from Star Formation, Shocks, and AGN Ionisation in NGC 1068 by D'Agostino, Joshua J, Kewley, Lisa J, Groves, Brent A, Medling, Anne M, Di Teodoro, Enrico, Dopita, Michael A, Thomas, Adam D, Sutherland, Ralph S, Garcia-Burillo, Santiago

    Published 19-06-2019
    “…In the optical spectra of galaxies, the separation of line emission from gas ionised by star formation and an AGN, or by star formation and shocks, are very…”
    Get full text
    Journal Article