A dataset provided by the European Space Agency

Name 065465
Title NGC 4190-ULX1: The nearest unstudied ultraluminous X-ray source
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0654650101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0654650201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0654650301

DOI 10.5270/esa-8ygcrze
Author Mr Floyd Jackson
Description Although it ranks amongst the nearest (at d ~ 3 Mpc) and brightest (flux ~ 4e-12 erg-cm^2-s) ULXs, NGC 4190-ULX1 has not yet been studied in the modern era of X-ray astronomy. Here we propose two 25-ks XMM-Newton observations to provide a first detailed view of it.s X-ray properties. We will investigate the specific characteristics of the X-ray spectral and temporal data of the source, and contrast them with other low-luminosity (~10^39 erg-s) ULXs to provide new insights into this hitherto neglected class of objects.
Publication 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 ,
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 ,
Irradiated, colour-temperature-corrected accretion discs in ultraluminous X-ray sources . Sutton, Andrew D., Done, Chris, . MNRAS . 444-2415 . 2014 . 2014MNRAS.444.2415S ,
XMM-Newton publication statistics . Ness, J.-U., Parmar, A. N., et all. . AN . 335-210 . 2014 . 2014AN....335..210N ,
Ensemble X-ray variability of active galactic nuclei. II. Excess variance and updated structure function . Vagnetti, F., Middei, R., et all. . A&A . 593-55 . 2016 . 2016A&A...593A..55V ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
ULX spectra revisited: Accreting, highly magnetized neutron stars as the engines of ultraluminous X-ray sources . Koliopanos, Filippos, Vasilopoulos, Georgios, et all. . A&A . 608-47 . 2017 . 2017A&A...608A..47K ,
Searching for outflows in ultraluminous X-ray sources through high-resolution X-ray spectroscopy . Kosec, P., Pinto, C., et all. . MNRAS . 473-5680 . 2018 . ...,
A new, clean catalogue of extragalactic non-nuclear X-ray sources in nearby galaxies . Earnshaw, H. P., Roberts, T. P., et all. . MNRAS . 483-5554 . 2019 . 2019MNRAS.483.5554E ,
A new possible accretion scenario for ultra-luminous X-ray sources . Kobayashi, Shogo B., Nakazawa, K., . MNRAS . 489-366 . 2019 . 2019MNRAS.489..366K ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2010-06-06T12:08:27Z/2010-11-25T07:11:27Z
Version 17.56_20190403_1200
Mission Description The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's 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 Earth's 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 2011-12-16T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2011-12-16T00:00:00Z, 065465, 17.56_20190403_1200. https://doi.org/10.5270/esa-8ygcrze