P
P. M. Rodriguez-Pascual
Researcher at European University of Madrid
Publications - 3
Citations - 83
P. M. Rodriguez-Pascual is an academic researcher from European University of Madrid. The author has contributed to research in topics: Quasar & Active galactic nucleus. The author has an hindex of 2, co-authored 3 publications receiving 80 citations.
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Journal ArticleDOI
Monitoring of the optical and 2.5-11.7 mu m spectrum and mid-IR imaging of the Seyfert 1 galaxy Mrk 279 with ISO
Maria Santos-Lleo,J. Clavel,Benjamin L. Schulz,Bruno Altieri,P. Barr,Danielle Alloin,Perry Berlind,R. Bertram,R. Bertram,D. M. Crenshaw,Rick Edelson,Uriel Giveon,Keith Horne,John P. Huchra,Shai Kaspi,Gerard A. Kriss,Julian H. Krolik,M. A. Malkan,Yu. F. Malkov,Hagai Netzer,P. T. O'Brien,Bradley M. Peterson,Richard W. Pogge,V. I. Pronik,B.-C. Qian,Gail A. Reichert,P. M. Rodriguez-Pascual,S. G. Sergeev,J. Tao,Susan Tokarz,R. M. Wagner,R. M. Wagner,Willem Wamsteker,Belinda Jane Wilkes +33 more
TL;DR: In this article, mid-infrared images of the Seyfert 1 galaxy Mrk 279 obtained with the ISO satellite are presented together with the results of a one-year monitoring campaign of the 2.5-11.7 mum spectrum.
Journal ArticleDOI
XMM-Newton observation of the deep minimum state of PG 2112+059 - A spectrum dominated by reflection from the accretion disk?
Norbert Schartel,P. M. Rodriguez-Pascual,M. Santos-Lleo,Lucía Ballo,J. Clavel,Matteo Guainazzi,Elena Jiménez-Bailón,Elena Jiménez-Bailón,Enrico Piconcelli +8 more
TL;DR: In this paper, the physical conditions of the absorber and the broad iron line of the X-ray weak quasar PG 2112+059 in greater detail than in previous studies were investigated.
Journal ArticleDOI
XMM-Newton observation of the deep minimum state of PG 2112+059: A spectrum dominated by reflection from the accretion disk?
Norbert Schartel,P. M. Rodriguez-Pascual,M. Santos-Lleo,Lucía Ballo,J. Clavel,Matteo Guainazzi,Elena Jiménez-Bailón,Elena Jiménez-Bailón,Enrico Piconcelli +8 more
TL;DR: In this paper, a 75ks XMM-Newton observation of PG 2112+059 performed in November 2005 and compare it with a 15k XMM Newton observation taken in May 2003 was analyzed.