A dataset provided by the European Space Agency

Name: X-ray Timing Observations of NGC 5408 X-1: Pinning Down the Mass
Published: 2009-02-07T00:00:00Z

Proposal ID	050075
Title	X-ray Timing Observations of NGC 5408 X-1: Pinning Down the Mass
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0500750101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0500750201
DOI	https://doi.org/10.5270/esa-6x2rb1s
Principal Investigator, PI	Dr Tod Strohmayer
Abstract	We propose EPIC observations of the ultraluminous X-ray source (ULX) in NGC 5408. Our AO4 pointing has revealed a wealth of new timing properties in this object. We have found the first quasiperiodic oscillation (at 20 mHz)and power spectral break in this source. The power spectrum in the hard X-rayband shows a classic flat-topped.. noise with a break in the power law veryclose to the 20 mHz QPO. These timing signatures allow the first estimates ofthe mass of the ULX based on comparisons with similar features observed inGalactic black hole systems accreting at high rates.
Publications	The linear rms-flux relation in an ultraluminous X-ray source \|Heil, L. M., Vaughan, S., \| MNRAS \| 405-86 \| 2010 \| 2010MNRAS.405L..86H \| http://ui.adsabs.harvard.edu/#abs/2010MNRAS.405L..86H The scaling of X-ray variability with luminosity in ultra-luminous X-ray sources \|Gonzalez-Martin, O., Papadakis, I., et al. \| A&A \| 526-132 \| 2011 \| 2011A&A...526A.132G \| http://ui.adsabs.harvard.edu/#abs/2011A&A...526A.132G Evidence for an Intermediate-mass Black Hole in NGC 5408 X-1 \|Strohmayer, Tod E., Mushotzky, Richard F., \| ApJ \| 703-1386 \| 2009 \| 2009ApJ...703.1386S \| http://ui.adsabs.harvard.edu/#abs/2009ApJ...703.1386S Unlocking the nature of ultraluminous X-ray sources using their X-ray spectra \|Gladstone, J. C., Roberts, T. P., \| AN \| 332-345 \| 2011 \| 2011AN....332..345G \| http://ui.adsabs.harvard.edu/#abs/2011AN....332..345G Does NGC 5408 X-1 really contain an intermediate-mass black hole? \|Middleton, M. J., Roberts, T. P., et al. \| AN \| 332-388 \| 2011 \| 2011AN....332..388M \| http://ui.adsabs.harvard.edu/#abs/2011AN....332..388M Challenging times: a re-analysis of NGC 5408 X-1 \|Middleton, M. J., Roberts, T. P., et al. \| MNRAS \| 411-644 \| 2011 \| 2011MNRAS.411..644M \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.411..644M An All-Sky Atlas of Radio/X-ray Associations \|Flesch, E., \| PASA \| 27-283 \| 2010 \| 2010PASA...27..283F \| http://ui.adsabs.harvard.edu/#abs/2010PASA...27..283F A Multi-epoch Timing and Spectral Study of the Ultraluminous X-Ray NGC 5408 X-1 with XMM-Newton \|Dheeraj, Pasham R., Strohmayer, Tod E., \| ApJ \| 753-139 \| 2012 \| 2012ApJ...753..139D \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...753..139D Exospheric solar wind charge exchange as seen by XMM-Newton \|Carter, J. A., Semba, S., \| AN \| 333-313 \| 2012 \| 2012AN....333..313C \| http://ui.adsabs.harvard.edu/#abs/2012AN....333..313C Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog \|Lin, Dacheng, Webb, Natalie A., \| ApJ \| 756-27 \| 2012 \| 2012ApJ...756...27L \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...756...27L The ultraluminous state revisited: fractional variability and spectral shape as diagnostics of super-Eddington accretion \|Sutton, Andrew D., Roberts, Timothy P., \| MNRAS \| 435-1758 \| 2013 \| 2013MNRAS.435.1758S \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.435.1758S The Local Environment of Ultraluminous X-Ray Sources Viewed by XMM-Newton.s Optical Monitor \|Berghea, C. T., Dudik, R. P., et al. \| ApJ \| 776-100 \| 2013 \| 2013ApJ...776..100B \| http://ui.adsabs.harvard.edu/#abs/2013ApJ...776..100B X-ray variability and energy spectra from NGC 5408 X-1 with XMM-Newton \|Caballero-Garcia, M. D., Belloni, T. M., \| MNRAS \| 435-2665 \| 2013 \| 2013MNRAS.435.2665C \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.435.2665C Time lags in the ultraluminous X-ray source NGC 5408 X-1: implications for the black hole mass \|De Marco, B., Ponti, G., et al. \| MNRAS \| 436-3782 \| 2013 \| 2013MNRAS.436.3782D \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.436.3782D Revisiting Putative Cool Accretion Disks in Ultraluminous X-Ray Sources \|Miller, J. M., Walton, D. J., et al. \| ApJ \| 776-36 \| 2013 \| 2013ApJ...776L..36M \| http://ui.adsabs.harvard.edu/#abs/2013ApJ...776L..36M Broad absorption features in wind-dominated ultraluminous X-ray sources? \|Middleton, Matthew J., Walton, Dominic J., et al. \| MNRAS \| 438-51 \| 2014 \| 2014MNRAS.438L..51M \| http://ui.adsabs.harvard.edu/#abs/2014MNRAS.438L..51M Ultraluminous X-ray sources: a deeper insight into their spectral evolution \|Pintore, Fabio, Zampieri, Luca, et al. \| MNRAS \| 439-3461 \| 2014 \| 2014MNRAS.439.3461P \| http://ui.adsabs.harvard.edu/#abs/2014MNRAS.439.3461P Automatic Classification of Time-variable X-Ray Sources \|Lo, Kitty K., Farrell, Sean, et al. \| ApJ \| 786-20 \| 2014 \| 2014ApJ...786...20L \| http://ui.adsabs.harvard.edu/#abs/2014ApJ...786...20L The diversity of quasars unified by accretion and orientation \|Shen, Yue, Ho, Luis C., \| Natur \| 513-210 \| 2014 \| 2014Natur.513..210S \| http://ui.adsabs.harvard.edu/#abs/2014Natur.513..210S On the black hole masses in ultra-luminous X-ray sources \|Zhou, Xin-Lin, \| NewA \| 37-1 \| 2015 \| 2015NewA...37....1Z \| http://ui.adsabs.harvard.edu/#abs/2015NewA...37....1Z Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift \|Yershov, V. N., \| Ap&SS \| 354-97 \| 2014 \| 2014Ap&SS.354...97Y \| http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y A spectral-timing model for ULXs in the supercritical regime \|Middleton, Matthew J., Heil, Lucy, et al. \| MNRAS \| 447-3243 \| 2015 \| 2015MNRAS.447.3243M \| http://ui.adsabs.harvard.edu/#abs/2015MNRAS.447.3243M X-ray time lags and non-linear variability in the ultraluminous X-ray sources NGC 5408 X-1 and NGC 6946 X-1 \|Hernandez-Garcia, L., Vaughan, S., et al. \| MNRAS \| 453-2877 \| 2015 \| 2015MNRAS.453.2877H \| http://ui.adsabs.harvard.edu/#abs/2015MNRAS.453.2877H Resolved atomic lines reveal outflows in two ultraluminous X-ray sources \|Pinto, Ciro, Middleton, Matthew J., \| Natur \| 533-64 \| 2016 \| 2016Natur.533...64P \| http://ui.adsabs.harvard.edu/#abs/2016Natur.533...64P The Rotation of the Hot Gas around the Milky Way \|Hodges-Kluck, Edmund J., Miller, Matthew J., \| ApJ \| 822-21 \| 2016 \| 2016ApJ...822...21H \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...822...21H The Million Optical - Radio/X-ray Associations (MORX) Catalogue \|Flesch, Eric W., \| PASA \| 33-52 \| 2016 \| 2016PASA...33...52F \| http://ui.adsabs.harvard.edu/#abs/2016PASA...33...52F The thin and medium filters of the EPIC camera on-board XMM-Newton: measured performance after more than 15 years of operation \|Barbera, Marco, Gastaldello, Fabio, et al. \| ExA \| 42-179 \| 2016 \| 2016ExA....42..179B \| http://ui.adsabs.harvard.edu/#abs/2016ExA....42..179B Analysis of Quasi-periodic Oscillations and Time Lag in Ultraluminous X-Ray Sources with XMM-Newton \|Li, Zi-Jian, Xiao, Guang-Cheng, et al. \| ApJ \| 839-19 \| 2017 \| 2017ApJ...839...19L \| http://ui.adsabs.harvard.edu/#abs/2017ApJ...839...19L Ultrafast outflows in ultraluminous X-ray sources \|Pinto, C., Fabian, A., et al. \| AN \| 338-234 \| 2017 \| 2017AN....338..234P \| http://ui.adsabs.harvard.edu/#abs/2017AN....338..234P A new, clean catalogue of extragalactic non-nuclear X-ray sources in nearby galaxies \|Earnshaw, H. P., Roberts, T. P., et al. \| MNRAS \| 483-5554 \| 2019 \| 2019MNRAS.483.5554E \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.483.5554E Ultraluminous X-ray sources with flat-topped noise and QPO \|Atapin, Kirill, Fabrika, Sergei, \| MNRAS \| 486-2766 \| 2019 \| 2019MNRAS.486.2766A \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.486.2766A A Multi-epoch Timing and Spectral Study of the Ultraluminous X-Ray NGC 5408 X-1 with XMM-Newton \|Pasham, Dheeraj R., Strohmayer, Tod E., \| ApJ \| 753-139 \| 2012 \| 2012ApJ...753..139P \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...753..139P Thermal stability of winds driven by radiation pressure in super-Eddington accretion discs \|Pinto, C., Mehdipour, M., et al. \| MNRAS \| 491-5702 \| 2020 \| 2020MNRAS.491.5702P \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.491.5702P Linking Soft Excess in Ultraluminous X-Ray Sources with Optically Thick Wind Driven by Supercritical Accretion \|Qiu, Yanli, Feng, Hua, \| ApJ \| 906-36 \| 2021 \| 2021ApJ...906...36Q \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...906...36Q Classification of 4XMM-DR9 sources by machine learning \|Zhang, Yanxia, Zhao, Yongheng, \| MNRAS \| 503-5263 \| 2021 \| 2021MNRAS.503.5263Z \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5263Z X-ray reverberation models of the disc wind in ultraluminous X-ray source NGC 5408 X-1 \|Luangtip, W., Chainakun, P., et al. \| MNRAS \| 507-6094 \| 2021 \| 2021MNRAS.507.6094L \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.507.6094L Ionized emission and absorption in a large sample of ultraluminous X-ray sources \|Kosec, P., Pinto, C., et al. \| MNRAS \| 508-3569 \| 2021 \| 2021MNRAS.508.3569K \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.508.3569K The impact of precession on the observed population of ULXs \|Khan, Norman, Middleton, Matthew J., et al. \| MNRAS \| 509-2493 \| 2022 \| 2022MNRAS.509.2493K \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.509.2493K The Redshift Evolution of Ultraluminous X-Ray Sources out to z 0.5: Comparison with X-Ray Binary Populations and Contribution to the Cosmic X-Ray Background \|Scott Barrows, R., Comerford, Julia M., et al. \| ApJ \| 932-27 \| 2022 \| 2022ApJ...932...27S \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...932...27S Winds in ultraluminous X\\u2011ray sources: New challenges \|Pinto, C., Kosec, P., \| AN \| 344-20220134 \| 2023 \| 2023AN....34420134P \| http://ui.adsabs.harvard.edu/#abs/2023AN....34420134P Unveiling the accretion scenario of BH-ULXs using XMM-Newton observations \|Majumder, Seshadri, Das, Santabrata, et al. \| MNRAS \| 526-2086 \| 2023 \| 2023MNRAS.526.2086M \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.526.2086M The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII, O VIII, and Fe L-shell Transitions \|Pan, Zeyang, Qu, Zhijie, et al. \| ApJS \| 271-62 \| 2024 \| 2024ApJS..271...62P \| http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P Robust constraints on feebly interacting particles using XMM-Newton \|Luque, Pedro De la Torre, Balaji, Shyam, \| PhRvD \| 109-L101305 \| 2024 \| 2024PhRvD.109j1305L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j1305L Multimessenger search for electrophilic feebly interacting particles from supernovae \|Luque, Pedro De la Torre, Balaji, Shyam, \| PhRvD \| 109-103028 \| 2024 \| 2024PhRvD.109j3028L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j3028L Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints \|De la Torre Luque, Pedro, Balaji, Shyam, \| ApJ \| 968-46 \| 2024 \| 2024ApJ...968...46D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...968...46D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2008-01-13T17:42:44Z/2008-01-15T03:13:41Z
Version	17.56_20190403_1200
Mission Description	The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations. Since Earths atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis.
Creator Contact	https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk
Date Published	2009-02-07T00:00:00Z
Keywords	"NGC 5408", "quasiperiodic oscillation", "power spectrum", "power law", "power spectral break", "ngc 5408", "x ray", "EPIC", "ngc 5408 x", "mhz qpo", "hard xray band"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Tod Strohmayer, 2009, 'X-ray Timing Observations of NGC 5408 X-1: Pinning Down the Mass', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-6x2rb1s