Y1 w7 (22 10 26-10) scientific method
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The document describes the scientific method using the example of discovering which colors make green. It outlines the steps of the scientific method: observe, ask questions, make a hypothesis/prediction, experiment, and reach a conclusion. The experiment involves mixing blue and yellow color samples in measuring cups to test if they make green, following the scientific process to think like a scientist.
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Scientists follow a process of observation, hypothesis formation, experimentation, and conclusion to think like scientists. This involves first observing a phenomenon, then asking questions and making an educated guess or hypothesis about it, following up by designing and conducting an experiment to test the hypothesis, and finally analyzing the results to draw a conclusion.
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The document provides instructions for students to complete a "Do Now" activity by finding 6 differences in a picture, and then checks their understanding of scientific concepts like the scientific method, pH scale, acids, bases, and telescopes. It also lists leadership activities for students such as having a snack, reading To Kill a Mockingbird, counting cans, using the recreation room, and returning to the classroom.
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The primary targets of this project are Westerlund 1 and 2, the closest supermassive star clusters to the Sun.
Methods. The project is based primarily on recent observations conducted with the Chandra and JWST observatories. Specifically,
the Chandra survey of Westerlund 1 consists of 36 new ACIS-I observations, nearly co-pointed, for a total exposure time of 1 Msec.
Additionally, we included 8 archival Chandra/ACIS-S observations. This paper presents the resulting catalog of X-ray sources within
and around Westerlund 1. Sources were detected by combining various existing methods, and photon extraction and source validation
were carried out using the ACIS-Extract software.
Results. The EWOCS X-ray catalog comprises 5963 validated sources out of the 9420 initially provided to ACIS-Extract, reaching a
photon flux threshold of approximately 2 × 10−8 photons cm−2
s
−1
. The X-ray sources exhibit a highly concentrated spatial distribution,
with 1075 sources located within the central 1 arcmin. We have successfully detected X-ray emissions from 126 out of the 166 known
massive stars of the cluster, and we have collected over 71 000 photons from the magnetar CXO J164710.20-455217.
Bob Reedy - Nitrate in Texas Groundwater.pdf
Presented at June 6-7 Texas Alliance of Groundwater Districts Business Meeting
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