A dataset provided by the European Space Agency

Name 015028
Title Coordinated broadband monitoring of variable X-ray sources in NGC 1313
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0150280101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0150280201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0150280301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0150280401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0150280501
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0150280601
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0150280701
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0150281101

DOI 10.5270/esa-l4smpop
Author Dr Ian Smith
Description We propose co-ordinated broadband monitoring of the ultraluminous X-ray sources (ULXs) in the nearby spiral galaxy NGC 1313. We request 10 pointings of 10 ksec each, distributed over a period of 6 weeks, with XMM-Newton EPIC pn as the primary science instrument. These will be co-ordinated with simultaneous ground-based observations. The science goals of our program are to investigate the multiwavelength spectra and the short- and long-term variability of various sources in NGC 1313, in particular the far off-center source X-2, which will be used to unveil the nature of ULXs. As a by-product of our study, we will provide additional data to the on-going monitoring of SN 1978K.
Publication X-Ray and Optical Variability of the Ultraluminous X-Ray Source NGC 1313 X-2 . Mucciarelli, P., Zampieri, L., et all. . ApJ . 658-999 . 2007 . 2007ApJ...658..999M ,
Spectral variability of ultraluminous X-ray sources . Kajava, Jari J. E., Poutanen, Juri, . MNRAS . 398-1450 . 2009 . 2009MNRAS.398.1450K ,
The XMM-Newton serendipitous survey. V. The Second XMM-Newton serendipitous source catalogue . Watson, M. G., Schroder, A. C., et all. . A&A . 493-339 . 2009 . 2009A&A...493..339W ,
Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras . Mateos, S., Saxton, R. D., et all. . A&A . 496-879 . 2009 . 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 ,
The XMM Cluster Survey: optical analysis methodology and the first data release . Mehrtens, Nicola, Romer, A. Kathy, et all. . MNRAS . 423-1024 . 2012 . 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 ,
XMM-Newton discovery of transient X-ray pulsar in NGC 1313 . Trudolyubov, S. P., . MNRAS . 387-36 . 2008 . 2008MNRAS.387L..36T ,
2XMM ultr...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2003-11-25T00:50:59Z/2004-01-17T02:08:01Z
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 2005-02-05T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2005-02-05T00:00:00Z, 015028, 17.56_20190403_1200. https://doi.org/10.5270/esa-l4smpop