This dataset contains example data and R and Matlab scripts that reproduce the analyses and figures from the article 'Warping methods for spectroscopic and chromatographic...

Catalog contains three fits files, each containing one epoch of near-infrared spectra for TW Hya. Epoch 1 and 2 are archival ESO VLT-Xshooter spectra that were downloaded from...

Arecibo observations were taken with the L-band wideband receiver and the Wideband Arecibo Pulsar Processor (WAPP) autocorrelator backend with two polarizations, a bandpass of...

The data of the W3-W4-W5 (W345) complexes were collected between fall 2016 and winter 2017. The survey is made possible through the two Apache Point Observatory (APO) Galactic...

We built up the most complete spectral sample for the already known O-type population in Cygnus OB2 by complementing new observations with already available spectra (own and...

Table 1 contains the details of each Hubble Space Telescope/Cosmic Origins Spectrograph (HST/COS) observation on 2017 for the five quasars. The data analyzed here are part of a...

The observed sample consists of seven nearby M-dwarf binaries or higher hierarchical triple systems with a closely separated binary pair. Targets were observed from November...

For this work, optical photometry and spectroscopic data from the Steward Observatory spectropolarimetric monitoring project, a support program for the Fermi Gamma-Ray Space...

APOGEE-2 is a part of the Sloan Digital Sky Survey IV (Blanton+ 2017AJ....154...28B) and is collecting high-resolution (R=22500) spectra of ~300000 stars across the Milky Way...

We build a sample of 5175 red clump (RC) stars from Ting+ (2018, J/ApJ/858/L7), which is constructed using data from the APOGEE (Majewski+ 2017AJ....154...94M) and Large Sky...

The APOGEE instrument is a high-resolution (R~22500) near-infrared (1.51-1.70um) spectrograph. For the main survey the instrument was connected to the Sloan 2.5m telescope. To...

The observations were performed in July-August 2019 using the SEPIA660 receiver on the APEX 12m telescope under the project id: M-0103.F-9519C-2019. In addition to the results...

Combining data from Gaia DR2, SDSS DR14, and LAMOST DR6, we update the fit to model of the properties of the stellar stream GD-1 and find that it has an age of ~13Gyr, [Fe/H] of...

Emission lines observed during outburst and quiescence. The lines are classified as "double-peaked" or disk-like (Dsk), "PCygni profiles" (PC). Those with complex,...

The observations of the Serpens SVS 4 cluster were done with the Submillimeter Array (SMA), Mauna Kea, Hawaii, program code: 2016B-S022; with the Atacama Pathfinder EXperiment...

We reported on the results of an SDSS-IV eBOSS spectroscopic survey that covered 36.8deg^2^ of Stripe 82 in the fall of 2015. About half of this survey area (15.6deg^2^)...

The spectroscopic and photometric data of 3C 273 used in this paper are mainly derived from the Steward Observatory (SO) spectropolarimetric monitoring project, which is a...

V506 Oph was observed spectroscopically with two different instruments. Between 2010 May and 2017 February, we monitored the binary with the Center for Astrophysics Harvard...

Spectra of the companion to PSR J1306-40 were obtained using SOAR/Goodman from 2017 July 11 to 2018 June 9. The spectra covered a wavelength range of ~5485-6740{AA}. Besides,...

The observations were performed using the 40m Yebes antenna and the 30m IRAM telescope. Daily spectra are in velocity and flux density units.