https://www.astroforrest.com/research daily 0.75 2024-10-18 https://images.squarespace-cdn.com/content/v1/5af1f9c531d4df31e5436bae/1527370946375-R2RD3O4JRPOOI73RY677/zfourge-logo.jpg Research https://images.squarespace-cdn.com/content/v1/5af1f9c531d4df31e5436bae/1528224074558-VK7LT09EHKCBUGGD26MU/method.png Research https://images.squarespace-cdn.com/content/v1/5af1f9c531d4df31e5436bae/1528224410917-FM6B6YNMFND3VHWPT2J2/F3.png Research https://images.squarespace-cdn.com/content/v1/5af1f9c531d4df31e5436bae/1528232140083-FO4XUSM0QYALRR8EGLPA/f1.png Research https://images.squarespace-cdn.com/content/v1/56d4a125e707eb7a02e4055f/1456851111610-486A5E4H0OE915O3XOHM/54.jpg Research https://images.squarespace-cdn.com/content/v1/5af1f9c531d4df31e5436bae/1528232958708-1AP58013PP6MAFDDWHZT/psb.png Research https://images.squarespace-cdn.com/content/v1/5af1f9c531d4df31e5436bae/1580969247353-409IY8SBFIIUT7ST0FN8/F1.png Research https://images.squarespace-cdn.com/content/v1/5af1f9c531d4df31e5436bae/1603242619473-4PD1YS5OA03PMG2DZ2Y7/Screen+Shot+2020-10-20+at+6.09.40+PM.png Research - Several spectra of emission-line galaxies https://images.squarespace-cdn.com/content/v1/5af1f9c531d4df31e5436bae/1603239732173-WGNAF4BOYWVUC6H0GAUY/Screen+Shot+2020-10-20+at+5.21.35+PM.png Research - SEDs and spectra for five of the UMGs. Models shown in red. Note the clear Balmer absorption features and lack of emission lines. https://images.squarespace-cdn.com/content/v1/5af1f9c531d4df31e5436bae/1729267755870-WASCJY0N0MOP9RNVU9GH/Screen+Shot+2024-10-18+at+12.09.00+PM.png Research - The C3VO Survey The Charting Cluster Construction with VUDS and ORELSE (C3VO) survey is an ongoing campaign designed to provide a nearly complete mapping of the five most significant overdensities detected in VIMOS Ultra–Deep Survey. The C3VO survey utilizes spectra from observations with both DEIMOS and MOSFIRE on the Keck I/II telescopes and VUDS, and employs the Voronoi Monte-Carlo algorithm for local environment measurement, originally developed within the framework of the ORELSE survey. The keck component of the C3VO survey is designed to target star-forming galaxies of all types to i_AB < 25.3 (or ∼ L*FUV at z ∼ 4.5 and < L*FUV at z ∼ 2.5) and Lyman-α emitting galaxies to fainter magnitudes. https://images.squarespace-cdn.com/content/v1/56d4a125e707eb7a02e4055f/1456783910525-KVZ7BMJMIIXGN1GDSHWI/12.jpg Research https://images.squarespace-cdn.com/content/v1/56d4a125e707eb7a02e4055f/1456785006090-WSZH5IFVLDISGJ3LL92P/77.jpg Research https://images.squarespace-cdn.com/content/v1/56d4a125e707eb7a02e4055f/1456851022917-I14CZYTKH20F3NT8F5T0/4.jpg Research https://images.squarespace-cdn.com/content/v1/56d4a125e707eb7a02e4055f/1456865071576-9LJLBGX0FSTBTYEQNUIM/25.jpg Research https://images.squarespace-cdn.com/content/v1/56d4a125e707eb7a02e4055f/1456869971895-A5SQFVQP8TDLHDK76R4P/11.jpg Research https://images.squarespace-cdn.com/content/v1/56d4a125e707eb7a02e4055f/1456944933692-TOA1PP8PC846S793GKKD/49.jpg Research https://www.astroforrest.com/about-1 daily 1.0 2024-10-18 https://images.squarespace-cdn.com/content/v1/5af1f9c531d4df31e5436bae/1603237685418-OUN8BITR2DSJQ62I5NEA/headshot_clnp.jpg About Crater Lake National Park https://www.astroforrest.com/teaching daily 0.75 2018-07-03