output
20022024
most citedThe Transiting Exoplanet Survey Satellite

4.1k citations

Showing 2020Show all

104 papers · 1 filter

astro-ph.GA202050 cited

Prospects for Galactic and stellar astrophysics with asteroseismology of giant stars in the Continuous Viewing Zones and beyond

J. Ted Mackereth, Andrea Miglio, Yvonne Elsworth +30

The NASA- mission presents a treasure trove for understanding the stars it observes and the Milky Way, in which they reside. We present a first look at the prospects for…

astro-ph.HE202015 cited

A possible bright ultraviolet flash from a galaxy at redshift z ~ 11

Linhua Jiang, Shu Wang, Bing Zhang +8

In the optical sky, minutes-duration transients from cosmological distances are rare. Known objects that give rise to such transients include gamma-ray bursts (GRBs), the most lumi…

astro-ph.HE202085 cited

Evidence for GN-z11 as a luminous galaxy at redshift 10.957

Linhua Jiang, Nobunari Kashikawa, Shu Wang +9

GN-z11 was photometrically selected as a luminous star-forming galaxy candidate at redshift z > 10 based on Hubble Space Telescope (HST) imaging data. Follow-up HST near-infrared g…

astro-ph.EP202010 cited

Revisiting the HD 21749 Planetary System with Stellar Activity Modeling

Tianjun Gan, Sharon Xuesong Wang, Johanna K. Teske +26

HD 21749 is a bright ( mag) K dwarf at 16 pc known to host an inner terrestrial planet HD 21749c as well as an outer sub-Neptune HD 21749b, both delivered by TESS. Follow-up…

cs.RO202018 cited

SDSS-V Algorithms: Fast, Collision-Free Trajectory Planning for Heavily Overlapping Robotic Fiber Positioners

Conor Sayres, José R. Sánchez-Gallego, Michael R. Blanton +8

Robotic fiber positioner (RFP) arrays are becoming heavily adopted in wide field massively multiplexed spectroscopic survey instruments. RFP arrays decrease nightly operational ove…

astro-ph.CO202032 cited

The Astrophysical Distance Scale III: Distance to the Local Group Galaxy WLM using Multi-Wavelength Observations of the Tip of the Red Giant Branch, Cepheids, and JAGB Stars

Abigail J. Lee, Wendy L. Freedman, Barry F. Madore +3

The local determination of the Hubble Constant sits at a crossroad. Current estimates of the local expansion rate of the Universe differ by about 1.7-sigma, derived from the Cephei…