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The wide-field, multiplexed, spectroscopic facility WEAVE: Survey design, overview, and simulated implementation
Shoko Jin, Scott C. Trager, Gavin B. Dalton +212
WEAVE, the new wide-field, massively multiplexed spectroscopic survey facility for the William Herschel Telescope, will see first light in late 2022. WEAVE comprises a new 2-degree…
The cross-correlation of galaxies in absorption with the Lyman forest
Ignasi Pérez-Ràfols, Matthew M. Pieri, Michael Blomqvist +3
We present the first clustering measurement of Strong Blended Lyman (SBLA) absorption systems by measuring their cross-correlation with the Lyman forest. SBLAs are a new po…
New Photometric Calibration of the Wide Field Camera 3 Detectors
A. Calamida, V. Bajaj, J. Mack +6
We present a new photometric calibration of the WFC3-UVIS and WFC3-IR detectors based on observations collected from 2009 to 2020 for four white dwarfs, namely GRW+70~5824, GD~153,…
UV counterpart of an X-ray ultra-fast outflow in IRAS 17020+4544
Missagh Mehdipour, Gerard A. Kriss, Yair Krongold +7
We report on the discovery of a UV absorption counterpart of a low-ionization X-ray ultra-fast outflow (UFO) in the Narrow-Line Seyfert-1 galaxy IRAS 17020+4544. This UV signature…