A dataset provided by the European Space Agency

Name: Monitoring the ultraluminous X-ray sources in the nearby galaxy NGC 1313
Published: 2006-02-25T00:00:00Z

Proposal ID	020523
Title	Monitoring the ultraluminous X-ray sources in the nearby galaxy NGC 1313
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0205230201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0205230301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0205230401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0205230501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0205230601
DOI	https://doi.org/10.5270/esa-9br152s
Principal Investigator, PI	Dr IAN SMITH
Abstract	XMM-Newton has revolutionized the study of X-ray sources in nearby galaxies suchas NGC 1313, a barred spiral galaxy that is 3.7 Mpc away. This contains twoultraluminous X-ray sources, and SN 1978K, the first supernova remnantrecognized from its X-ray flux. NGC 1313 is close enough that XMM-Newton canperform detailed simultaneous spectroscopic and timing studies of all of them.In Cycle 2, we were awarded time to perform 7 Priority A observations as thefirst stage in a long-term program of monitoring the known sources, searchingfor new transients, and determining the diffuse emission component. Here we willcontinue this campaign by performing 4 more pointings of 10 ksec to study thesources on time scales ranging from seconds to months.
Publications	Spectral variability of ultraluminous X-ray sources \|Kajava, Jari J. E., Poutanen, Juri, \| MNRAS \| 398-1450 \| 2009 \| 2009MNRAS.398.1450K \| http://ui.adsabs.harvard.edu/#abs/2009MNRAS.398.1450K The XMM-Newton serendipitous survey. V. The Second XMM-Newton serendipitous source catalogue \|Watson, M. G., Schroder, A. C., et al. \| A&A \| 493-339 \| 2009 \| 2009A&A...493..339W \| http://ui.adsabs.harvard.edu/#abs/2009A&A...493..339W Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras \|Mateos, S., Saxton, R. D., et al. \| A&A \| 496-879 \| 2009 \| 2009A&A...496..879M \| http://ui.adsabs.harvard.edu/#abs/2009A&A...496..879M X-ray spectral states and metallicity in the ultraluminous X-ray sources NGC 1313 X-1 and X-2 \|Pintore, Fabio, Zampieri, Luca, \| MNRAS \| 420-1107 \| 2012 \| 2012MNRAS.420.1107P \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.420.1107P The XMM Cluster Survey: optical analysis methodology and the first data release \|Mehrtens, Nicola, Romer, A. Kathy, et al. \| MNRAS \| 423-1024 \| 2012 \| 2012MNRAS.423.1024M \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423.1024M Spectral State Transitions of the Ultraluminous X-Ray Sources X-1 and X-2 in NGC 1313 \|Feng, Hua, Kaaret, Philip, \| ApJ \| 650-75 \| 2006 \| 2006ApJ...650L..75F \| http://ui.adsabs.harvard.edu/#abs/2006ApJ...650L..75F XMM-Newton discovery of transient X-ray pulsar in NGC 1313 \|Trudolyubov, S. P., \| MNRAS \| 387-36 \| 2008 \| 2008MNRAS.387L..36T \| http://ui.adsabs.harvard.edu/#abs/2008MNRAS.387L..36T 2XMM ultraluminous X-ray source candidates in nearby galaxies \|Walton, D. J., Roberts, T. P., et al. \| MNRAS \| 416-1844 \| 2011 \| 2011MNRAS.416.1844W \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.416.1844W Spectral Evolution of NGC 1313 X-2: Evidence against the Cool Disk Model \|Feng, Hua, Kaaret, Philip, \| ApJ \| 660-113 \| 2007 \| 2007ApJ...660L.113F \| http://ui.adsabs.harvard.edu/#abs/2007ApJ...660L.113F Multiwavelength Monitoring of the Unusual Ultraluminous Supernova SN 1978K in NGC 1313 and the Search for an Associated Gamma-Ray Burst \|Smith, I. A., Ryder, S. D., et al. \| ApJ \| 669-1130 \| 2007 \| 2007ApJ...669.1130S \| http://ui.adsabs.harvard.edu/#abs/2007ApJ...669.1130S The X-Ray Spectral Evolution in X-Ray Binaries and Its Application to Constrain the Black Hole Mass of Ultraluminous X-Ray Sources \|Wu, Qingwen, Gu, Minfeng, \| ApJ \| 682-212 \| 2008 \| 2008ApJ...682..212W \| http://ui.adsabs.harvard.edu/#abs/2008ApJ...682..212W Six years of XMM-Newton observations of NGC 1313 X-1 and X-2 \|Pintore, F., Zampieri, L., \| AN \| 332-337 \| 2011 \| 2011AN....332..337P \| http://ui.adsabs.harvard.edu/#abs/2011AN....332..337P A large catalogue of ultraluminous X-ray source candidates in nearby galaxies \|Walton, D. J., Gladstone, J. C., et al. \| AN \| 332-354 \| 2011 \| 2011AN....332..354W \| http://ui.adsabs.harvard.edu/#abs/2011AN....332..354W 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 The XMM Cluster Survey: X-ray analysis methodology \|Lloyd-Davies, E. J., Romer, A. Kathy, et al. \| MNRAS \| 418-14 \| 2011 \| 2011MNRAS.418...14L \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.418...14L 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 The cosmological analysis of X-ray cluster surveys - II. Application of the CR-HR method to the XMM archive \|Clerc, N., Sadibekova, T., et al. \| MNRAS \| 423-3561 \| 2012 \| 2012MNRAS.423.3561C \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423.3561C 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 An XMM-Newton Survey of the Soft X-Ray Background. II. An All-Sky Catalog of Diffuse O VII and O VIII Emission Intensities \|Henley, David B., Shelton, Robin L., \| ApJS \| 202-14 \| 2012 \| 2012ApJS..202...14H \| http://ui.adsabs.harvard.edu/#abs/2012ApJS..202...14H Searching for massive outflows in Holmberg IX X-1 and NGC 1313 X-1: the iron K band \|Walton, D. J., Miller, J. M., et al. \| MNRAS \| 426-473 \| 2012 \| 2012MNRAS.426..473W \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.426..473W A systematic cross-search for radio/infrared counterparts of XMM- Newton sources \|Combi, J. A., Albacete Colombo, J. F., et al. \| Ap&SS \| 331-53 \| 2011 \| 2011Ap&SS.331...53C \| http://ui.adsabs.harvard.edu/#abs/2011Ap&SS.331...53C 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 Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog: Objects of Special Interest \|Lin, Dacheng, Webb, Natalie A., \| ApJ \| 780-39 \| 2014 \| 2014ApJ...780...39L \| http://ui.adsabs.harvard.edu/#abs/2014ApJ...780...39L 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 Super-Eddington Accretion in the Ultraluminous X-Ray Source NGC 1313 X-2: An Ephemeral Feast \|Weng, Shan-Shan, Zhang, Shuang-Nan, \| ApJ \| 780-147 \| 2014 \| 2014ApJ...780..147W \| http://ui.adsabs.harvard.edu/#abs/2014ApJ...780..147W 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 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 Irradiated, colour-temperature-corrected accretion discs in ultraluminous X-ray sources \|Sutton, Andrew D., Done, Chris, \| MNRAS \| 444-2415 \| 2014 \| 2014MNRAS.444.2415S \| http://ui.adsabs.harvard.edu/#abs/2014MNRAS.444.2415S 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 Sunyaev-Zel.dovich effect or not? Detecting the main foreground effect of most galaxy clusters \|Xiao, Weike, Chen, Chen, et al. \| MNRAS \| 432-41 \| 2013 \| 2013MNRAS.432L..41X \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.432L..41X Evidence for High-frequency QPOs with a 3:2 Frequency Ratio from a 5000 Solar Mass Black Hole \|Pasham, Dheeraj R., Cenko, S. Bradley, et al. \| ApJ \| 811-11 \| 2015 \| 2015ApJ...811L..11P \| http://ui.adsabs.harvard.edu/#abs/2015ApJ...811L..11P Diagnosing the accretion flow in ultraluminous X-ray sources using soft X-ray atomic features \|Middleton, Matthew J., Walton, Dominic J., et al. \| MNRAS \| 454-3134 \| 2015 \| 2015MNRAS.454.3134M \| http://ui.adsabs.harvard.edu/#abs/2015MNRAS.454.3134M The Interaction of the Fermi Bubbles with the Milky Way.s Hot Gas Halo \|Miller, Matthew J., Bregman, Joel N., \| ApJ \| 829-9 \| 2016 \| 2016ApJ...829....9M \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...829....9M SPIDERS: the spectroscopic follow-up of X-ray selected clusters of galaxies in SDSS-IV \|Clerc, N., Merloni, A., et al. \| MNRAS \| 463-4490 \| 2016 \| 2016MNRAS.463.4490C \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.463.4490C 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 X-ray decay of the ultraluminous supernova SN 1978K in NGC 1313 \|Zhao, Hai-Hui, Weng, Shan-Shan, \| MNRAS \| 468-1551 \| 2017 \| 2017MNRAS.468.1551Z \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.468.1551Z 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 Anisotropy of the galaxy cluster X-ray luminosity-temperature relation \|Migkas, Konstantinos, Reiprich, Thomas H., \| A&A \| 611-50 \| 2018 \| 2018A&A...611A..50M \| http://ui.adsabs.harvard.edu/#abs/2018A&A...611A..50M Recurrent Outbursts Revealed in 3XMM J031820.8-663034 \|Zhao, Hai-Hui, Weng, Shan-Shan, \| ApJ \| 859-106 \| 2018 \| 2018ApJ...859..106Z \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...859..106Z The XMM Cluster Survey: Present status and latest results \|Viana, P. T. P., Mehrtens, N., et al. \| AN \| 334-462 \| 2013 \| 2013AN....334..462V \| http://ui.adsabs.harvard.edu/#abs/2013AN....334..462V 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 Testing emergent gravity on galaxy cluster scales \|Tamosiunas, Andrius, Bacon, David, et al. \| JCAP \| 5-53 \| 2019 \| 2019JCAP...05..053T \| http://ui.adsabs.harvard.edu/#abs/2019JCAP...05..053T Chandra Follow-up of the SDSS DR8 Redmapper Catalog Using the MATCha Pipeline \|Hollowood, Devon L., Jeltema, Tesla, et al. \| ApJS \| 244-22 \| 2019 \| 2019ApJS..244...22H \| http://ui.adsabs.harvard.edu/#abs/2019ApJS..244...22H A new possible accretion scenario for ultra-luminous X-ray sources \|Kobayashi, Shogo B., Nakazawa, K., \| MNRAS \| 489-366 \| 2019 \| 2019MNRAS.489..366K \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.489..366K 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 Stellar mass as a galaxy cluster mass proxy: application to the Dark Energy Survey redMaPPer clusters \|Palmese, A., Annis, J., et al. \| MNRAS \| 493-4591 \| 2020 \| 2020MNRAS.493.4591P \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.493.4591P X-ray properties of the X-CLASS-redMaPPer galaxy cluster sample: the luminosity-temperature relation \|Molham, Mona, Clerc, Nicolas, et al. \| MNRAS \| 494-161 \| 2020 \| 2020MNRAS.494..161M \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.494..161M Multiwavelength classification of X-ray selected galaxy cluster candidates using convolutional neural networks \|Kosiba, Matej, Lieu, Maggie, et al. \| MNRAS \| 496-4141 \| 2020 \| 2020MNRAS.496.4141K \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.496.4141K SPIDERS: overview of the X-ray galaxy cluster follow-up and the final spectroscopic data release \|Clerc, N., Kirkpatrick, C. C., et al. \| MNRAS \| 497-3976 \| 2020 \| 2020MNRAS.497.3976C \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.497.3976C An X-Ray- and SZ-bright Diffuse Source toward M31: A Local Hot Bridge \|Qu, Zhijie, Huang, Rui, et al. \| ApJ \| 907-14 \| 2021 \| 2021ApJ...907...14Q \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...907...14Q 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 Broadband X-ray spectral variability of the pulsing ULX NGC 1313 X-2 \|Robba, A., Pinto, C., et al. \| A&A \| 652-118 \| 2021 \| 2021A&A...652A.118R \| http://ui.adsabs.harvard.edu/#abs/2021A&A...652A.118R 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 Solar Cycle Temporal Variation of the Solar Wind Charge Exchange X-Ray Lines \|Qu, Zhijie, Koutroumpa, Dimitra, et al. \| ApJ \| 930-21 \| 2022 \| 2022ApJ...930...21Q \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...930...21Q 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 Propeller states in locally supercritical ULXs \|Middleton, M., G\\u00farpide, A., \| MNRAS \| 519-2224 \| 2023 \| 2023MNRAS.519.2224M \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.519.2224M 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	2004-05-01T21:28:43Z/2005-02-07T15:33:48Z
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	2006-02-25T00:00:00Z
Keywords	"supernova remnant recognized", "xray sources", "XMM", "xray flux", "time scales ranging", "diffuse emission component", "NGC 1313", "nearby galaxy", "ultraluminous xray sources", "XMM-Newton", "barred spiral galaxy", "ngc 1313", "term program", "xmm newton"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr IAN SMITH, 2006, 'Monitoring the ultraluminous X-ray sources in the nearby galaxy NGC 1313', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-9br152s