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A quantitative assessment of completeness correction methods and public release of a versatile simulation code
Nicha Leethochawalit, Michele Trenti, Takahiro Morishita +2
Having accurate completeness functions is crucial to the determination of the rest-frame ultraviolet luminosity functions (UVLFs) all the way back to the epoch of reionization. Mos…
Dissecting Nearby Galaxies with piXedfit: I. Spatially Resolved Properties of Stars, Dust, and Gas as Revealed by Panchromatic SED Fitting
Abdurro'uf, Yen-Ting Lin, Hiroyuki Hirashita +5
We study spatially resolved properties (on spatial scales of kpc out to at least effective radii) of the stars, dust, and gas in ten nearby spiral galaxies. The prop…
Redshift identification of X-ray selected active galactic nuclei in the J1030 field: searching for large-scale structures and high-redshift sources
Stefano Marchesi, Marco Mignoli, Roberto Gilli +23
We publicly release the spectroscopic and photometric redshift catalog of the sources detected with Chandra in the field of the =6.3 quasar SDSS J1030+0525. This is currently th…
The Physical Properties of Luminous Galaxies and Implications for the Cosmic Star Formation Rate Density From 0.35 deg of (Pure-)Parallel HST Observations
Guido Roberts-Borsani, Takahiro Morishita, Tommaso Treu +2
We present the largest systematic, HST-based search to date for luminous galaxy candidates using 1267 arcmin of (pure-)parallel observations from a compilat…