A dataset provided by the European Space Agency

Name: SN 2001ci: A type Ic supernova in NGC 3079
Published: 2004-11-01T00:00:00Z
License: https://creativecommons.org/licenses/by-nc/3.0/igo

Proposal ID	014776
Title	SN 2001ci: A type Ic supernova in NGC 3079
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0147760101
DOI	https://doi.org/10.5270/esa-tx1qhie
Principal Investigator, PI	Dr Wolfgang Pietsch
Abstract	We propose a 45 ks XMM-Newton EPIC observation of SN 2001ci, a type Icsupernova (SN) that exploded around April 20, 2001 about 25 north of thenucleus of NGC 3079. While type II SNe have been established as X-rayemitters in nearby galaxies by Einstein and ROSAT detections, only one SNtype Ic, SN 1994I was detected. SN 2001ci is selected for its type and therelatively small distance for XMM-Newton follow-up observations. AnXMM-Newton observation of NGC 3079 by us shortly before the SN explosion isan additional benefit. For a better understanding of the shock wavesinteracting with the circumstellar matter around type Ic SNe X-raylightcurves and spectra are urgently needed.
Publications	A revision of the X-ray absorption nature of BALQSOs \|Streblyanska A. Barcons X. et al. \| A&A \| 515-2 \| 2010 \| 2010A&A...515A...2S \| http://ui.adsabs.harvard.edu/#abs/2010A&A...515A...2S 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 The X-ray Energy Dependence of the Relation Between Optical and X-ray Emission in Quasars \|Young M. Elvis M. \| ApJ \| 708-1388 \| 2010 \| 2010ApJ...708.1388Y \| http://ui.adsabs.harvard.edu/#abs/2010ApJ...708.1388Y An Extremely Luminous Panchromatic Outburst from the Nucleus of a Distant Galaxy \|Levan A. J. Tanvir N. 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Melu00e9ndez M. et al. \| MNRAS \| 508-4902 \| 2021 \| 2021MNRAS.508.4902V \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.508.4902V 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 X-ray emission from a rapidly accreting narrow-line Seyfert 1 galaxy at z = 6.56 \|Wolf J. 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Marcum Pamela M. et al. \| ApJ \| 967-169 \| 2024 \| 2024ApJ...967..169B \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...967..169B 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 Probing the inner Galactic halo with blue horizontal-branch stars. Gaia DR3-based catalogue with atmospheric and stellar parameters \|Culpan R. Dorsch M. et al. \| A&A \| 685-A134 \| 2024 \| 2024A&A...685A.134C \| http://ui.adsabs.harvard.edu/#abs/2024A&A...685A.134C Extinction and AGN over host galaxy contrast effects on the optical spectroscopic classification of AGN \|Barquu00edn-Gonzu00e1lez L. Mateos S. et al. \| A&A \| 687-A159 \| 2024 \| 2024A&A...687A.159B \| http://ui.adsabs.harvard.edu/#abs/2024A&A...687A.159B Search for Young Stellar Objects within 4XMM-DR13 Using CatBoost and SPE \|Ma Xiangyao Zhang Yanxia et al. \| AJ \| 168-210 \| 2024 \| 2024AJ....168..210M \| http://ui.adsabs.harvard.edu/#abs/2024AJ....168..210M New 511 keV Line Data Provide Strongest sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 973-L6 \| 2024 \| 2024ApJ...973L...6D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...973L...6D
Instrument	EPN, RGS1, OM, RGS2, EMOS1, EMOS2
Temporal Coverage	2003-10-14T03:03:50Z/2003-10-14T15:23:50Z
Version	21.51_20241115_1113
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	2004-11-01T00:00:00Z
Last Update	2026-06-19
Keywords	"xmm newton epic", "EPIC", "ngc 3079", "onlysupernovatype ic", "nearby galaxy", "rosat detections", "XMM", "type ii sne", "xmm newton", "shock waves interacting", "circumstellar matter", "type ic supernova", "XMM-Newton", "additional benefit", "sn 2001ci", "NGC 3079", "xray emitters", "ROSAT"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Wolfgang Pietsch, 2004, 'SN 2001ci: A type Ic supernova in NGC 3079', 21.51_20241115_1113, European Space Agency, https://doi.org/10.5270/esa-tx1qhie
Rights	Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.