Search for a Near‐Infrared Counterpart to the Cassiopeia A X‐Ray Point Source

2001 ◽  
Vol 558 (1) ◽  
pp. 270-275 ◽  
Author(s):  
D. L. Kaplan ◽  
S. R. Kulkarni ◽  
S. S. Murray
2018 ◽  
Vol 620 ◽  
pp. A12 ◽  
Author(s):  
L. Chiappetti ◽  
S. Fotopoulou ◽  
C. Lidman ◽  
L. Faccioli ◽  
F. Pacaud ◽  
...  

We present the version of the point source catalogue of the XXL Survey that was used, in part, in the first series of XXL papers. In this paper we release, in our database in Milan and at CDS: (i) the X-ray source catalogue with 26 056 objects in two areas of 25 deg2 with a flux limit (at 3σ) of ~10−15 erg s−1 cm−2 in [0.5–2] keV, and ~ 3 × 10−15 erg s−1 cm−2 in [2–10] keV, yielding a 90% completeness limit of 5.8 × 10−15 and 3.8 × 10−14 respectively;(ii) the associated multiwavelength catalogues with candidate counterparts of the X-ray sources in the infrared, near-infrared, optical, and ultraviolet (plus spectroscopic redshift when available); and (iii) a catalogue of spectroscopic redshifts recently obtained in the southern XXL area. We also present the basic properties of the X-ray point sources and their counterparts. Other catalogues described in the second series of XXL papers will be released contextually, and will constitute the second XXLdata release.


2001 ◽  
Vol 547 (1) ◽  
pp. L41-L44 ◽  
Author(s):  
M. A. McLaughlin ◽  
J. M. Cordes ◽  
A. A. Deshpande ◽  
B. M. Gaensler ◽  
T. H. Hankins ◽  
...  

2001 ◽  
Vol 548 (2) ◽  
pp. 800-810 ◽  
Author(s):  
Deepto Chakrabarty ◽  
Michael J. Pivovaroff ◽  
Lars E. Hernquist ◽  
Jeremy S. Heyl ◽  
Ramesh Narayan
Keyword(s):  
X Ray ◽  

1986 ◽  
Vol 116 ◽  
pp. 229-230
Author(s):  
D. J. Stickland ◽  
C. Lloyd ◽  
A. J. Willis

The recent study by Caillault et al. (1985) has shown the emission-line star AS 431 (= WR 147) to be a strong X-ray source and moderately strong radio emitter. Combining optical, near-infrared and radio data, they deduced that its mass loss rate was ∼ 4 × 10−4 M⊙yr−1, an order of magnitude greater than is normal for WR stars. They also suggested that it would show up in the IRAS survey and that such data would help to elucidate whether its extreme reddening had a significant circumstellar component. To investigate this possibility and to study the general properties of the object, we have raided the IRAS Point Source Catalogue.


Author(s):  
D. A. Carpenter ◽  
Ning Gao ◽  
G. J. Havrilla

A monolithic, polycapillary, x-ray optic was adapted to a laboratory-based x-ray microprobe to evaluate the potential of the optic for x-ray micro fluorescence analysis. The polycapillary was capable of collecting x-rays over a 6 degree angle from a point source and focusing them to a spot approximately 40 µm diameter. The high intensities expected from this capillary should be useful for determining and mapping minor to trace elements in materials. Fig. 1 shows a sketch of the capillary with important dimensions.The microprobe had previously been used with straight and with tapered monocapillaries. Alignment of the monocapillaries with the focal spot was accomplished by electromagnetically scanning the focal spot over the beveled anode. With the polycapillary it was also necessary to manually adjust the distance between the focal spot and the polycapillary.The focal distance and focal spot diameter of the polycapillary were determined from a series of edge scans.


2012 ◽  
Vol 746 (1) ◽  
pp. L10 ◽  
Author(s):  
Joshua C. Dolence ◽  
Charles F. Gammie ◽  
Hotaka Shiokawa ◽  
Scott C. Noble

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