Energy scaling of soft-x-ray high harmonics driven by a loosely-focused TW-scale mid-infrared pulse

Author(s):  
Kotaro Nishimura ◽  
Yuxi Fu ◽  
Akira Suda ◽  
Katsumi Midorikawa ◽  
Eiji J. Takahashi
2003 ◽  
Vol 257 (1-2) ◽  
pp. 42-50 ◽  
Author(s):  
G. Hoffmann ◽  
H.J. Schimper ◽  
C. Schwender ◽  
N. Herhammer ◽  
G.F. West ◽  
...  

2006 ◽  
Vol 642 (1) ◽  
pp. 126-139 ◽  
Author(s):  
P. Barmby ◽  
A. Alonso‐Herrero ◽  
J. L. Donley ◽  
E. Egami ◽  
G. G. Fazio ◽  
...  
Keyword(s):  

2004 ◽  
Vol 418 (2) ◽  
pp. 465-473 ◽  
Author(s):  
D. Lutz ◽  
R. Maiolino ◽  
H. W. W. Spoon ◽  
A. F. M. Moorwood

2013 ◽  
Vol 434 (1) ◽  
pp. 639-651 ◽  
Author(s):  
P. Shalima ◽  
V. Jithesh ◽  
K. Jeena ◽  
R. Misra ◽  
S. Ravindranath ◽  
...  
Keyword(s):  

1989 ◽  
Vol 22 (4) ◽  
pp. 363-371 ◽  
Author(s):  
R. Somashekar ◽  
I. H. Hall ◽  
P. D. Carr

Methods which determine the number and disorder of lattice planes in a crystal from the Fourier cosine coefficients of the intensity profile of an X-ray reflection use only the low harmonics and require that the coefficients be normalized so that the zero harmonic is unity. Experimentally, the profiles can only be recorded over a smaller range of scattering angle than required by the theory, and it is necessary to subtract background, which is likely to be estimated with considerable error, before determining the coefficients. It is shown that with polymer fibres this causes serious errors in the normalization, and in the values of those low harmonics used in the size and disorder determination, and prevents reliable values being obtained. Methods which avoid normalization and use only high harmonics are needed. It is shown that disorder may be obtained in such a way, but not size, for which low-order normalized coefficients are essential. A method of extrapolation is described and tested which enables the accurate high harmonics to be used to improve the estimates of the low ones. Whilst this will yield more reliable values of crystal size than are obtainable from existing methods, the accuracy depends entirely on the validity of the extrapolation, which cannot be tested in many cases of interest.


2019 ◽  
Vol 622 ◽  
pp. A29 ◽  
Author(s):  
Chandreyee Maitra ◽  
Frank Haberl ◽  
Valentin D. Ivanov ◽  
Maria-Rosa L. Cioni ◽  
Jacco Th. van Loon

Context. Finding active galactic nuclei (AGN) behind the Magellanic Clouds (MCs) is difficult because of the high stellar density in these fields. Although the first AGN behind the Small Magellanic Cloud (SMC) were reported in the 1980s, it is only recently that the number of AGN known behind the SMC has increased by several orders of magnitude. Aims. The mid-infrared colour selection technique has proven to be an efficient means of identifying AGN, especially obscured sources. The X-ray regime is complementary in this regard and we use XMM-Newton observations to support the identification of AGN behind the SMC. Methods. We present a catalogue of AGN behind the SMC by correlating an updated X-ray point-source catalogue from our XMM-Newton survey of the SMC with previously identified AGN from the literature as well as a list of candidates obtained from the ALLWISE mid-infrared colour-selection criterion. We studied the properties of the sample with respect to their redshifts, luminosities, and X-ray spectral characteristics. We also identified the near-infrared counterpart of the sources from the VISTA observations. Results. The redshift and luminosity distributions of the sample (where known) indicate that we detect sources ranging from nearby Seyfert galaxies to distant and obscured quasars. The X-ray hardness ratios are compatible with those typically expected for AGN, and the VISTA colours and variability are also consistent with AGN. A positive correlation was observed between the integrated X-ray flux (0.2–12 keV) and the ALLWISE and VISTA magnitudes. We further present a sample of new candidate AGN and candidates for obscured AGN. Together these make an interesting subset for further follow-up studies. An initial spectroscopic follow-up of 6 out of the 81 new candidates showed that all six sources are active galaxies, although two have narrow emission lines.


2007 ◽  
Vol 376 (1) ◽  
pp. 416-434 ◽  
Author(s):  
G. Rodighiero ◽  
C. Gruppioni ◽  
F. Civano ◽  
A. Comastri ◽  
A. Franceschini ◽  
...  

2008 ◽  
Vol 680 (1) ◽  
pp. 130-142 ◽  
Author(s):  
Carolin N. Cardamone ◽  
C. Megan Urry ◽  
Maaike Damen ◽  
Pieter van Dokkum ◽  
Ezequiel Treister ◽  
...  

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