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9 results for “Neides”
High-level Data Products for NEID Solar Observations (January 1, 2021 - June 30, 2024)
<p>High-level data products derived from Sun-as-a-star observations by the NEID Solar Telescope at WIYN Observatory, spanning January 1, 2021 through June 30, 2024. We identify 117,060 observations which are unlikely to be significantly affected by weather, hardware or major calibration issues. This repository provides several high-level data products to the community to aid in the interpretation and inter comparisons of NEID solar observations. These include individual radial velocities (RV) measurements from the Penn State Research Pipeline, RVs binned over solar oscillation timescales, and daily-binned RVs, activity indicators, and cross correlation functions, as well as estimated corrections for differential extinction and the apparent solar rotation velocity. For additional information, see the manscript, "Earths within Reach: Evaluation of Strategies for Mitigating Solar Variability using 3.5 years of NEID Sun-as-a-Star Observations". </p>
Revisiting ε Eridani with NEID: Line Parameter Data Cube
<p>This repository contains the data cube (an <a href="https://xarray.dev/">xarray</a> DataArray) used in Jiang et al. 2023 <i>Revisiting ε Eridani with NEID: Identifying New Activity-Sensitive Lines in a Young K Dwarf Star</i> (in press). The cube contains all line parameters (centroid, depth, FWHM, and integrated flux) for each line in the compiled line list over 32 NEID observations of ε Eridani spanning a six-month period from September 2021 to February 2022, as well as the measured RV and activity indices for each observation. For information on how the line parameters are measured, see the paper.</p>
High-quality NEID Solar Observations (January 2021 - June 2022)
<p>NExScI archives all NEID Solar observations at <a href="https://neid.ipac.caltech.edu/search_solar.php">https://neid.ipac.caltech.edu/search_solar.php</a>. NEID takes data even during inclement weather, and the official <a href="https://neid.ipac.caltech.edu/docs/NEID-DRP/index.html">NEID Data Reduction Pipeline</a> does not differentiate between those taken in excellent or poor observing conditions. This CSV file contains a list of all NEID Solar observations from January 1, 2021 to June 13, 2022, identifies which are currently believed to be of high-quality, and provides diagnostic information used (so users can easily adapting the selection criterion for their needs).</p> <p><strong>Columns:</strong></p> <p>filename: Name of file as provided by NExScI</p> <p>bjd: Barycentric Julian Date</p> <p>mask: true for observations considered of high quality; false for observations suspected to be low quality; See selection criterion specified below</p> <p>pyrflux_mean: mean flux observed by pyrheliometer during exposure</p> <p>pyrflux_rms: root mean square deviation from mean of flux observed by pyrheliometer during exposure</p> <p>expmeter_mean: mean of exposure meter during exposure (summed over wavelength channels)</p> <p>expmeter_rms: root mean square deviation from mean of exposure meter during exposure (summed over wavelength channels)</p> <p>airmass: airmass of sun a time of observation</p> <p>hour_angle: hour angle of sun at time of observation</p> <p>driftfun: value of DRIFTFUN copied from FITS header of filename</p> <p>wavecal: value of WAVECAL copied from FITS header of filename</p> <p>expmeter_mean_blue: mean of exposure meter during exposure (summed over bluest third of wavelength channels)</p> <p>expmeter_mean_green: mean of exposure meter during exposure (summed over middle third of wavelength channels)</p> <p>expmeter_mean_red: mean of exposure meter during exposure (summed over reddest third of wavelength channels)</p> <p> </p> <p>Selection criteria for setting mask to true:</p> <p>1. Require E_VER from fits file matches v1.1.* (Data processed with common minor version of NEID DRP)</p> <p>2. Require driftfun == "dailymodel0" and wavecal == "LFCplusThAr" (Wavelength calibration used)</p> <p>3. Start time of exposure lies between 17:30:00 and 22:12:00 (Removes data taken while wavelength calibration is changing rapidly)</p> <p>4. Exclude dates: October 2, 2021 to October 27, 2021 (due to a cabling issue)</p> <p>5. Require airmass <= 2.25 (Exclude data taken at high airmass)</p> <p>6. Require mean_pyroflux >= 10^2.95 (Require sufficient flux reaching the pyrheliometer)</p> <p>7. Require expmeter_mean >= 1.0e5 (Require sufficient flux reaching the exposure meter)</p> <p>8. Require rms_pyroflux <= 0.0035 * mean_pyroflux (Steady atmospheric transparency)</p> <p>9. Require expmeter_rms <= 0.003 * expmeter_mean (Steady transparency & pointing)</p> <p>10. Require expmeter_mean >= 150 * pyrflux_mean (Good pointing)</p> <p>11. Exclude dates: June 6, 2021, June 16, 2021, July 7, 2021, July 18, 2021, and July 19, 2021 (Dates with poor wavelength calibrations. This list may be updated upon further analysis.)</p>
Fig. 5 in Effect of Bacillus sphaericus Neide on Anopheles (Diptera: Culicidae) and associated insect fauna in fish ponds in the Amazon
Fig. 5. Regression analysis of diversity and richness data compared to application of Bacillus sphaericus.
Fig. 3 in Effect of Bacillus sphaericus Neide on Anopheles (Diptera: Culicidae) and associated insect fauna in fish ponds in the Amazon
Fig. 3. Abundance over time of aquatic insects and values LNMH at C3 and C4, Manaus, Amazonas, Brazil.
Fig. 2 in Effect of Bacillus sphaericus Neide on Anopheles (Diptera: Culicidae) and associated insect fauna in fish ponds in the Amazon
Fig. 2. Abundance over time of aquatic insects and values LNMH at C1 and C2, Manaus, Amazonas, Brazil.
Fig. 4 in Effect of Bacillus sphaericus Neide on Anopheles (Diptera: Culicidae) and associated insect fauna in fish ponds in the Amazon
Fig. 4. Abundance over time of Chironomidae and values LNMH at C5, Manaus, Amazonas, Brazil.
Confirmation of four hot Jupiters detected by TESS using follow-up spectroscopy from MaHPS at Wendelstein together with NEID and TRES
<p>Supplementary material to the paper 'Confirmation of four hot Jupiters detected by TESS using follow-up spectroscopy from MaHPS at Wendelstein together with NEID and TRES':</p> <p>Fig. Z1 - Z4: Fit of the photometric lightcurves (Sec. 2.2)</p> <p>ZT1 -ZT4: Tables showing the parameters, the prior distribution and the posteriors for the four targets after performing a joint fit with the Python package 'juliet' (Sec. 5.1)</p> <p>Fig. Z5_6: S/N values for the observations taken with MaHPS (Sec. 3.2.1)</p> <p>Fig. Z7: O-C diagrams for the search of TTVs (Sec. 5.3.2)</p> <p> </p> <p> </p>
Fig. 1 in Effect of Bacillus sphaericus Neide on Anopheles (Diptera: Culicidae) and associated insect fauna in fish ponds in the Amazon
Fig. 1. Location of breeding sites for applications of B. sphaericus, Manaus, Amazonas, Brazil.
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