{ "id": "2001.02720", "version": "v1", "published": "2020-01-08T20:04:29.000Z", "updated": "2020-01-08T20:04:29.000Z", "title": "Signatures of first galaxies at FIR/sub-mm wavelengths", "authors": [ "Maria Emilia De Rossi", "Volker Bromm" ], "comment": "3 pages, 2 figures. Accepted for publication in BAAA, Vol. 61B, 2020", "categories": [ "astro-ph.GA", "astro-ph.CO" ], "abstract": "We explore the possibility of detecting first galaxies with a generic far-infrared/sub-millimeter telescope by applying an analytical model of primordial dust emission. As shown in previous works, galaxies at redshifts $z>7$ experience a strong negative K-correction in such a way that systems of similar masses are brighter at higher $z$. In addition, at a given mass and $z$, our model predicts that luminosity fluxes increase proportionally to the dust-to-metal ratios ($D/M$) of primeval sources. We evaluate the observability of model sources at different $z>7$ as a function of the observed survey area ($\\Delta \\Omega$) and sensitivity ($S$) of a generic instrument. Assuming $\\Delta \\Omega \\sim 10~{\\rm deg}^2$ and a plausible $S \\sim 1~{\\mu}{\\rm Jy}$ for a near future survey, we could assure the detection of at least one typical source with $D/M \\sim 5\\times10^{-3}$ at $z>7$. For $S\\gtrsim 1~{\\mu}{\\rm Jy}$ and $\\Delta \\Omega \\lesssim 10~{\\rm deg}^2$, higher than typical $D/M$ are required to detect at least one individual source at $z>7$. The observability of model galaxies is also affected by the size distribution of dust grains, specially towards higher $z$.", "revisions": [ { "version": "v1", "updated": "2020-01-08T20:04:29.000Z" } ], "analyses": { "keywords": [ "first galaxies", "fir/sub-mm wavelengths", "signatures", "generic far-infrared/sub-millimeter telescope", "luminosity fluxes increase" ], "note": { "typesetting": "TeX", "pages": 3, "language": "en", "license": "arXiv", "status": "editable" } } }