Name | 040641 |
Title | Understanding the nature of Seyfert 2 Galaxy VV 780 - IC4518 |
URL | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0406410101 |
DOI | https://doi.org/10.5270/esa-wd6gl0s |
Author | European Space Agency |
Description | We discovered hard X-ray emission from Seyfert 2 galaxy VV 780 with INTEGRAL. VV 780 is an interacting galaxy pair at an early stage of merger. Its soft X-ray properties point to an highly obscured AGN. The sample of early merger Sy2s that are observed in X-rays is limited and they may hold important clues to understand the onset of starburst and AGN activity. We request one XMM-Newton observation of this source, first to verify that the X-ray emitting object in the ISGRI error circle is VV 780. We will also obtain the spectral parameters of the source in soft X-rays with XMM-Newton. Along with the simultaneous RXTE observation (submitted AO-11), the overall spectrum will enable us to classify this object, and provide information about the nature of hard and soft X-ray emission. |
Publication | No observations found associated with the current proposal |
Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
Temporal Coverage | 2006-08-15T09:16:41Z/2006-08-15T16:16:54Z |
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 | 2007-09-12T00:00:00Z |
Publisher And Registrant | European Space Agency |
Credit Guidelines | European Space Agency, 2007, Understanding The Nature Of Seyfert 2 Galaxy Vv 780 - Ic4518, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-wd6gl0s |