1. MHZ-325 - Munthouders 32,5mm - zelfklevend(per 50, 250, 500 of 1000)
Beschrijving. Zelfklevende munthouders gemaakt van de juiste, milieuvriendelijke grondstoffen zodat uw munt(en) op geen enkele manier wordt aangetast.
Type: Zelfklevend Diameter venster: 32,5 mm

2. 325 MHz Short Range Radio Service - HFUnderground
10 apr 2024 · 325 MHz band, Narrow band FM, NFM, NBFM and FSK. 12.5 kHz channel spacing. 2.5 watt maximum transmitter power output. 325.000 MHz to 325.4875 MHz UHF band.
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3. Band 315 – 325 kHz – Detail of Frequency Band
This web application is created for efficient access to information on the radio spectrum. Provided information and data are simplified presentation of a series ...
The CTU´s application named Utilisation of Radio Spectrum provides an overview of conditions set by the CTU for particular frequency bands, radiocommunication services and applicaions. Radio Spectrum Utilisation Plan stems is based on the Frequency Band Allocation Plan (National Table of Frequency Allocation).
4. 325 MHz Wireless, RF Saw Filter - Anatech Electronics
More Information. Center Frequency, 325.3 MHz. Dimensions, 3.8 x 3.8 x 1.4 mm. Power Handling, 10 dBm. Style, SMT. Band Width, 6.6 MHz.
325 MHz Wireless, RF Saw Filter

5. Unusual increase in the 325 MHz flux density of PSR B0655+64
We report on the detection of a large amplification of the flux density of PSR B0655+64 at 325 MHz (a factor of similar to 43) that lasted about one hour.
We report on the detection of a large amplification of the flux density of PSR B0655+64 at 325 MHz (a factor of similar to 43) that lasted about one hour. To the best of our knowledge such a large amplification has not been reported before. The phenomenon is restricted to a very narrow bandwidth (50 % decorrelation half-width of 3.6 +/- 0.4 MHz). The decorrelation bandwidth and characteristic time scale of the variation are in agreement with the values expected for diffractive interstellar scintillation. However, the observed amplification of the flux density of PSR B0655+64 is rather large. The observations suggest that amplifications of a factor up to 8 are not uncommon for PSR 0655+64 at 92 cm. The extreme flux density amplification of PSR 0655+64 might be explained in terms of caustics. We consider it unlikely that this event can be explained by intrinsic variability.
6. A.H. Systems FCC-4 Tuned Dipole Antenna 325 MHz – 1 GHz
Specifications ; Frequency Range. 325 MHz - 1000 MHz ; Balun Loss. <0.5 dB ; Maximum Continuous Power. 60 Watts ; Impedance. 50 Ohm ; Length. 9.0 in.
A.H. Systems FCC-4 Tuned Dipole Antenna 325 MHz – 1 GHz A.H. Systems
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7. High Frequency Tuned Dipole Antenna DA1G-FCC, 325 MHz to 1 ...
Dimensions: Length 9 in. Frequency Range: 325 MHz - 1000 MHz; Gain: 0 to 2 dBi; Impedance: 50 Ohms nominal; Maximum Continuous Power: 60 Watts ...
High Frequency Tuned Dipole Antenna DA1G-FCC, 325 MHz to 1 GHz, CISPR 16-1-5, 60 Watts . The EMC Shop is the only online store for EMC test equipment and accessories.

8. What is the expected behavior with a UserClk higher than 325 MHz in a ...
13 jun 2023 · What is the expected behavior with a UserClk higher than 325 MHz in a design using TX Buffer Bypass (GTH Transciever, Kintex UltraScale ...
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9. Lumped LC Low Pass Filter, DC - 325 MHz, 50Ω | SALF-325+ | Mini-Circuits
Mini-Circuits is a global leader in the design and manufacturing of RF, IF, and microwave components from DC to 86GHz.

10. 325-MHz observations of the ELAIS-N1 field using the Giant ...
We present observations of the European Large-Area ISO Survey-North 1 (ELAIS-N1) at 325 MHz using the Giant Metrewave Radio Telescope (GMRT), with the ultimate ...
Abstract. We present observations of the European Large-Area ISO Survey-North 1 (ELAIS-N1) at 325 MHz using the Giant Metrewave Radio Telescope (GMRT), wit

11. 100-325 MHz, Bidirectional Sensor (DB8885AD350) - dbSpectra
We manufacture Land Mobile Radio, Public Safety, and Wireless/Cellular equipment. All products are proudly designed and manufactured in the USA. dbSpectra is ...
dbSpectra DB8885AD350 PDF: Spec Sheet for 100-325 MHz, Bidirectional Sensor (DB8885AD350)

12. VLA XMM Large Scale Structure Field 325-MHz Source Catalog - HEASARC
For the phase calibration of the radio data, the authors used standard self-calibration at 325 MHz and field-base calibration at 74 MHz. Polyhedron-based ...
The XMM Large Scale Structure survey (XMM-LSS) is an X-ray survey aimed at studying the large scale structure of the Universe. The XMM-LSS field (centered at RA (J2000) = 02h 24m 00.27s, Dec (J2000) = -04o 09' 47.6") is currently being followed up using observations across a wide range of wavelengths, and in their paper the authors present the observational results of a low frequency radio survey of the XMM-LSS field using the Very Large Array at 74 and 325 MHz. This survey will map out the locations of the extragalactic radio sources relative to the large scale structure as traced by the X-ray emission. This is of particular interest because radio galaxies and radio-loud AGN show strong and complex interactions with their small and larger scale environment, and different classes of radio galaxies are suggested to lie at different places with respect to the large scale structure.
13. the 325 MHz radio luminosity function of AGN and star-forming galaxies ...
In this paper, we present a measurement of the evolution of radio-loud AGN and SF galaxies to z = 0.5, by matching a catalogue of radio sources measured at a ...
Abstract. Measurement of the evolution of both active galactic nuclei (AGN) and star-formation in galaxies underpins our understanding of galaxy evolution

14. What is the expected behavior with a UserClk higher than 325 MHz ...
What is the expected behavior with a UserClk higher than 325 MHz in a design using TX Buffer Bypass (GTH Transciever, Kintex UltraScale FPGA)? Is it ...
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15. [PDF] First Measurements on the 325 MHz Superconducting CH Cavity
Abstract. At the Institute for Applied Physics (IAP), Frankfurt. University, a superconducting 325 MHz CH-Cavity has been designed and built.
16. Com-Power LI-325 10 kHz - 400 MHz LISN for RTCA DO-160 / MIL-STD ...
The Com-Power LI-325 Line Impedance Stabilization Network (LISN) provides the necessary measurement platform for performing power line conducted emissions ...
Order the Com-Power LI-325 10 kHz - 400 MHz LISN for RTCA DO-160 / MIL-STD 461D. The EMC Shop offers new, used, rentals and leases for EMC test equipment & accessories

17. the 325 MHz radio luminosity function of AGN and star-forming galaxies
Galaxy And Mass Assembly (GAMA): the 325 MHz radio luminosity function of AGN and star-forming galaxies. Prescott, M.; Mauch, T.; Jarvis, M.J.; McAlpine, ...
Measurement of the evolution of both active galactic nuclei (AGN) and star-formation in galaxies underpins our understanding of galaxy evolution over cosmi...
18. A study of the Lockman Hole Region at 325 MHz - arXiv
11 mei 2020 · Title:Characterizing EoR foregrounds: A study of the Lockman Hole Region at 325 MHz ... Abstract:One of the key science goals for the most ...
One of the key science goals for the most sensitive telescopes, both current and upcoming, is the detection of the redshifted 21-cm signal from the Cosmic Dawn and Epoch of Reionization. The success of detection relies on accurate foreground modeling for their removal from data sets. This paper presents the characterization of astrophysical sources in the Lockman Hole region. Using 325 MHz data obtained from the GMRT, a $6^\circ \times 6^\circ$ mosaiced map is produced with an RMS reaching 50 $μ$Jy $\mathrm{beam}^{-1}$. A source catalog containing 6186 sources is created, and the Euclidean normalized differential source counts have been derived from it, consistent with previous observations as well as simulations. A detailed comparison of the source catalog is also made with previous findings - at both lower and higher frequencies. The angular power spectrum (APS) of the diffuse Galactic synchrotron emission is determined for three different galactic latitudes using the Tapered Gridded Estimator. The values of the APS lie between $\sim$1 mK$^2$ to $\sim$100 mK$^2$. Fitting a power law of the form $A\ell^{-β}$ gives values of $A$ and $β$ varying across the latitudes considered. This paper demonstrates, for the first time, the variation of the power-law index for diffuse emission at very high galactic locations. It follows the same trend that is seen at locations near the galactic plane, thus emphasizing the need for low-frequency observations for developing better models of th...

19. Galaxy And Mass Assembly (GAMA): the 325 MHz radio luminosity ...
Measurement of the evolution of both active galactic nuclei (AGN) and star-formation in galaxies underpins our understanding of galaxy evolution over cosmic ...
Measurement of the evolution of both active galactic nuclei (AGN) and star-formation in galaxies underpins our understanding of galaxy evolution over cosmic time. Radio continuum observations can provide key information on these two processes, in particular via the mechanical feedback produced by radio jets in AGN, and via an unbiased dust-independent measurement of star formation rates. In this paper, we determine radio luminosity functions at 325 MHz for a sample of AGN and star-forming galaxies by matching a 138 deg2 radio survey conducted with the Giant Metrewave Radio Telescope, with optical imaging and redshifts from the Galaxy And Mass Assembly survey. We find that the radio luminosity function at 325 MHz for star-forming galaxies closely follows that measured at 1.4 GHz. By fitting the AGN radio luminosity function out to z = 0.5 as a double power law, and parametrizing the evolution as Φ ∝ (1 + z)k, we find evolution parameters of k = 0.92 ± 0.95 assuming pure density evolution and k = 2.13 ± 1.96 assuming pure luminosity evolution. We find that the Low Excitation Radio Galaxies are the dominant population in space density at lower luminosities. Comparing our 325 MHz observations with radio continuum imaging at 1.4 GHz, we determine separate radio luminosity functions for steep- and flat-spectrum AGN, and show that the beamed population of flat-spectrum sources in our sample can be shifted in number density and luminosity to coincide with the un...
20. [PDF] AR201178 - Ampleon
26 jan 2021 · CW Signal performance over 325-352 MHz ... The presented demo is tuned for the frequency range: 325-352MHz. Figure 1 Demo Front view. Page 4 ...
21. Cygnus survey with the Giant Metrewave Radio Telescope at 325 ...
We surveyed the central ∼15 sq deg of the Cygnus constellation at the 325 and 610 MHz bands with angular resolutions and sensitivities of 10″ and 6″, and 0.5 ...
Astronomy & Astrophysics (A&A) is an international journal which publishes papers on all aspects of astronomy and astrophysics
22. TV-2 Tuned Dipole Antenna - 325 MHz - 1000 MHz - RF Globalnet
The TV-2 is a tuned dipole antenna from AH Systems that operates within the 325 MHz to 1000 MHz frequency range.
The TV-2 is a tuned dipole antenna from A.H. Systems that operates within the 325 MHz to 1000 MHz frequency range.

23. Design and development of efficient and compact 20 kW 325 MHz solid ...
3 mei 2024 · The salient features of this SSA include power density of 12.7 kW/m3, AC to RF efficiency of 54.8% at 20 kW, and guaranteed output of 20 kW with ...
An efficient and compact, 20 kW solid-state power amplifier (SSA) at 325 MHz has been designed and developed in-house, using single stage combining. It comprise
