4,181 datasets found

TEUV corrects synthetic stellar fluxes for interstellar absorption for wavelengths smaller than 91.1 nm. It simulates radiative bound-free absorption of the ground states of H,...

Split spectra from the CALIFA DR3 cubes. This service serves one spectrum each per pixel in each cube where there is at least one valid spaxel. Where both V500 and COMB data is...

These spectra are optical follow-up observations of the X-ray sources detected in the 942 ks exposure of the Chandra Deep Field-South (CDFS) using FORS.

The zCOSMOS redshift survey used 600h on the VIMOS spectrograph spread over five observing seasons (2005-2009) to obtain spectra of about 20,000 galaxies selected to have Iab...

This table contains basic metadata as well as the spectra from the Digital First Byurakan Survey (DFBS).

The First Byurakan Survey (FBS) is the largest and the first systematic objective prism survey of the extragalactic sky. It covers 17,000 sq.deg. in the Northern sky together...

We present extremely deep Hubble Space Telescope (HST) Wide Field Camera 3 (WFC3) observations of the MUSE Ultra Deep Field. This unique region of the sky contains two quasars...

Spectra from surveys hosted by Data Central. Most spectra were taken with the multi-object spectroscopy facilities 2dF (Anglo-Australian Telescope) and 6dF (UK Schmidt Telescope).

JWST is here. The early release observation (ERO) program provides us with the first look at the scientific data and the spectral capabilities. One of the targets from the ERO...

We present the first mid-IR detection of the linear polarization toward the star CygOB2-12, a luminous blue hypergiant that, with A_V_~10mag of foreground extinction, is a...

The study of substructure is an important step in determining how galaxy clusters form. We aim to gain new insights into the controversial dynamical status of MACS J0329-0211...

Spectra from the VIMOS Ultra–Deep Survey (VUDS) DR1 release

Spectra from the second data release (PDR-2) of VIPERS.

Spectra from the third data release (DR3) of GAMA.

Spectra from the third data release (DR3) of zCOSMOS 20k bright.

Spectra of MUSE-Wide (version 1.0) sources on GOODS-South field.

Wide Field Slitless Spectroscopy (WFSS) provides a powerful tool for detecting strong line emission in star-forming galaxies (SFGs) without the need for target preselection. As...

We determined the projected rotational velocity (vsini) of 238 southern O stars selected from the Galactic O-star Survey. The sample contains 130 spectroscopic single stars (C),...

We report the discovery of one possible neutron star binary (P_orb_=0.8666d) by using LAMOST low-resolution spectroscopic data. The visible companion is a late A-type dwarf...

We present results from an atmospheric retrieval analysis of Gl 229B using the Brewster retrieval code. We find the best fit model to be cloud-free, consistent with the T dwarf...