Integration time for short broad band clicks in echolocating FM-bats (Eptesicus fuscus)

1996 ◽  
Vol 178 (2) ◽  
Author(s):  
A. Surlykke ◽  
O. Bojesen
1988 ◽  
Author(s):  
James A. Simmons ◽  
Edward G. Freedman ◽  
Scott B. Stevenson ◽  
Lynda Chen ◽  
Timothy J. Wohlgemant

1987 ◽  
Vol 117 ◽  
pp. 216-217
Author(s):  
S. van den Bergh ◽  
C. J. Pritchet

Recently we have obtained both Hα + [NII] and broad-band red exposures of a number of galaxies with an RCA 320 × 512 CCD at the prime-focus of the 3.6 m CFH Telescope. Figure 1 shows the difference between Hα and red exposures (each with a total integration time of 60 min) of M87 = NGC4486.


2003 ◽  
Vol 12 (4) ◽  
Author(s):  
Erik Høg

AbstractGaia will obtain multi-color photometry for astrometric and astrophysical purposes. A photometry in five broad bands and with high angular resolution will be obtained after every astrometric observation of a star, especially for the sake of correcting slight astrometric chromaticity errors of the optical system. A separate smaller telescope will obtain photometry in eleven passbands of medium width designed to serve the astrophysical analysis of the mission results. The medium-band photometry (MBP) has less angular resolution, but much longer effective integration time than the broad-band photometry (BBP).


1989 ◽  
Vol 86 (4) ◽  
pp. 1318-1332 ◽  
Author(s):  
James A. Simmons ◽  
Edward G. Freedman ◽  
Scott B. Stevenson ◽  
Lynda Chen ◽  
Timothy J. Wohlgenant

2012 ◽  
Vol 8 (S290) ◽  
pp. 133-136
Author(s):  
Paul A. Mason ◽  
Edward L. Robinson ◽  
Sebastian Gomez ◽  
Emmanuel Gonzalez ◽  
Isaac D. Lopez ◽  
...  

AbstractHigh speed photometry of several accreting binaries was obtained using the McDonald Observatory 2.1m telescope and ARGOS CCD photometer. A broad-band filter (BVR) was used in order to maximize flux and maintain a short (1-10s) integration time on faint targets. Such observations obtained over several years allow for variability study over time scales covering many orders of magnitude. Observations and analysis for several binaries are summarized.


2010 ◽  
Vol 3 (4) ◽  
pp. 3803-3849 ◽  
Author(s):  
J. C. Gómez Martín ◽  
J. Blahins ◽  
U. Gross ◽  
T. Ingham ◽  
A. Goddard ◽  
...  

Abstract. We demonstrate a new instrument for in situ detection of atmospheric iodine atoms and molecules based on atomic and molecular resonance and off-resonance ultraviolet fluorescence excited by lamp emission. The instrument combines the robustness, light weight, low power consumption and efficient excitation of radio-frequency discharge light sources with the high sensitivity of the photon counting technique. Calibration of I2 fluorescence is achieved via quantitative detection of the molecule by incoherent broad band cavity-enhanced absorption spectroscopy. Atomic iodine fluorescence signal is calibrated by controlled broad band photolysis of known I2 concentrations in the visible spectral range at atmospheric pressure. The instrument has been optimised in laboratory experiments to reach detection limits of 1.2 pptv for I atoms and 20 pptv for I2, for S/N=1 and 10 min of integration time. The ROFLEX system has been deployed in a field campaign in Northern Spain, representing the first concurrent observation of ambient mixing ratios of iodine atoms and molecules in the 1–350 pptv range.


1997 ◽  
Vol 51 (6) ◽  
pp. 849-855 ◽  
Author(s):  
Praveen C. Kumar ◽  
Joseph A. Wehrmeyer

An experimental system to investigate the feasibility of using laser Raman spectroscopy to detect stack gas pollutants is described. With spontaneous Raman spectroscopy, one unit is capable of measuring all gas species simultaneously and, when applied to a continuous emissions monitoring (CEM) system, could both simplify it and improve reliability. Minimum detectabilities with the use of this weak light scattering process were determined for the three primary pollutants from coal-based power plants: carbon monoxide (CO), sulfur dioxide (SO2), and nitric oxide (NO). A frequency-doubled, pulsed Nd:YAG laser was used to excite the test gas held in a sample cell. A charge-coupled device connected to a spectrometer was used as the detection system, providing complete spectral information. A set of experiments was carried out for different concentrations of the three test gas species. With a 200-s integration time, the following minimum detectability limits were obtained: 100 ppm for SO2, 250 ppm for CO, and 250 ppm for NO. A mixture of all three pollutants in a base of N2 was made to simulate typical stack gas mixtures. Baseline strength and associated shot noise are more severe when gas mixtures are being analyzed. One possible explanation is the broad-band fluorescence of NO2, perhaps produced photolytically. System modifications to improve minimum detectabilities are discussed.


2011 ◽  
Vol 4 (1) ◽  
pp. 29-45 ◽  
Author(s):  
J. C. Gómez Martín ◽  
J. Blahins ◽  
U. Gross ◽  
T. Ingham ◽  
A. Goddard ◽  
...  

Abstract. We demonstrate a new instrument for in situ detection of atmospheric iodine atoms and molecules based on atomic and molecular resonance and off-resonance ultraviolet fluorescence excited by lamp emission. The instrument combines the robustness, light weight, low power consumption and efficient excitation of radio-frequency discharge light sources with the high sensitivity of the photon counting technique. Calibration of I2 fluorescence is achieved via quantitative detection of the molecule by Incoherent Broad Band Cavity-enhanced Absorption Spectroscopy. Atomic iodine fluorescence signal is calibrated by controlled broad band photolysis of known I2 concentrations in the visible spectral range at atmospheric pressure. The instrument has been optimised in laboratory experiments to reach detection limits of 1.2 pptv for I atoms and 13 pptv for I2, for S/N = 1 and 10 min of integration time. The ROFLEX system has been deployed in a field campaign in northern Spain, representing the first concurrent observation of ambient mixing ratios of iodine atoms and molecules in the 1–350 pptv range.


1999 ◽  
Vol 173 ◽  
pp. 309-314 ◽  
Author(s):  
T. Fukushima

AbstractBy using the stability condition and general formulas developed by Fukushima (1998 = Paper I) we discovered that, just as in the case of the explicit symmetric multistep methods (Quinlan and Tremaine, 1990), when integrating orbital motions of celestial bodies, the implicit symmetric multistep methods used in the predictor-corrector manner lead to integration errors in position which grow linearly with the integration time if the stepsizes adopted are sufficiently small and if the number of corrections is sufficiently large, say two or three. We confirmed also that the symmetric methods (explicit or implicit) would produce the stepsize-dependent instabilities/resonances, which was discovered by A. Toomre in 1991 and confirmed by G.D. Quinlan for some high order explicit methods. Although the implicit methods require twice or more computational time for the same stepsize than the explicit symmetric ones do, they seem to be preferable since they reduce these undesirable features significantly.


Author(s):  
Burton B. Silver ◽  
Theodore Lawwill

Dutch-belted 1 to 2.5 kg anesthetized rabbits were exposed to either xenon or argon laser light administered in a broad band, designed to cover large areas of the retina. For laser exposure, the pupil was dilated with atropine sulfate 1% and pheny lephrine 10%. All of the laser generated power was within a band centered at 5145.0 Anstroms. Established threshold for 4 hour exposures to laser irradiation are in the order of 25-35 microwatts/cm2. Animals examined for ultrastructural changes received 4 hour threshold doses. These animals exhibited ERG, opthalmascopic, and histological changes consistent with threshold damage.One month following exposure the rabbits were killed with pentobarbitol. The eyes were immediately enucleated and dissected while bathed in 3% phosphate buffered gluteraldehyde.


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