VizieR Online Data Catalog: 5-55000Å spectrum of TOI 560 (Zhang+, 2022)

We used Keck/NIRSPEC to observe a full transit of TOI560.01 on 2021 March 18 (UTC) and a partial transit on April 19, 2021 UTC (40% of T14). All observations were obtained in Y band using the high-resolution mode with the 12x0.432" slit, resulting in a spectral resolution of 25000.

On April 21, XMM-Newton measured the star's X-ray and MUV spectrum, which are crucial for modeling photoevaporative mass loss and predicting the metastable helium population. We observed the system for a total of 13ks as part of XMM prop.ID088287 (PI: Michael Zhang). We configured the EPIC cameras to observe with the medium filter and small window, giving us 97% observing efficiency on the two MOS CCDs and 71% efficiency on the one pn CCD. We configured the Optical Monitor to observe the star in the UVM2 filter (231{+/-}48nm) for 7.2ks and the UVW2 filter (212{+/-}50nm) for 4.4ks.

(1 data file).