-
SSHADE bandlist library
SSHADE bandlist library. -
IACOB Spectroscopic Database
OB-stars multi-epoch optical spectra from FIES@NOT and Hermes@Mecator at ORM/La Palma -
SSHADE bandlist library (dev)
SSHADE bandlist library. -
SSHADE bandlist library (dev)
SSHADE bandlist library. -
S-type asteroids reflect. spectra param.
The search for asteroidal parent bodies of chondrites through various techniques is an ongoing endeavor. A link between ordinary chondrites (OCs) and S-type asteroids has... -
Solar activity components intensity profiles
The detection of Earth-like planets with the radial-velocity method is currently limited by the presence of stellar activity signatures. On rotational timescales, spots and... -
Single and double peaked type 2 AGN
Driven by the imminent need to rapidly process and classify millions of AGN spectra drawn from next generation astronomical facilities, we present a spectral fitting routine for... -
A compilation of optical spectra from 361 SNe Ia
We present a data-driven method based on long short-term memory (LSTM) neural networks to analyze spectral time series of Type Ia supernovae (SNeIa). The data set includes 3091... -
Multiwavelength monitoring of the type Ib SN 2014C
SN 2014C was originally classified as a Type Ib supernova, but at phase {phi}=127d, post-explosion strong H{alpha} emission was observed. SN 2014C has since been observed in... -
HCT spectroscopic obs. of the type IIP SN 2020jfo
We present spectroscopic and photometric observations of the Type IIP supernova, SN2020jfo, in ultraviolet and optical wavelengths. SN2020jfo occurred in the spiral galaxy M61... -
Massive YSOs in the GC. II. IRTF spectra
To study the demographics of interstellar ices in the Central Molecular Zone (CMZ) of the Milky Way, we obtain near-infrared spectra of 109 red point sources using NASA... -
ASAS-SN light curves of SDSS AGNs
Low luminosity active galactic nuclei (LLAGN) probe accretion physics in the low Eddington regime can provide additional clues about galaxy evolution. AGN variability is... -
DES DR1 galaxies in the field of FRB 180924
Fast radio burst (FRB) dispersion measures (DMs) record the presence of ionized baryons that are otherwise invisible to other techniques enabling resolution of the matter... -
Stars of the LMS-1 stream with sp. obs.
Stellar streams produced from dwarf galaxies provide direct evidence of the hierarchical formation of the Milky Way. Here, we present the first comprehensive study of the LMS-1... -
54 years S-index measurements for {lambda} Ser
The bright star {lambda}Ser hosts a hot Neptune with a minimum mass of 13.6M{Earth} and a 15.5day orbit. It also appears to be a solar analog, with a mean rotation period of... -
Abundances in M67 open cluster
We report on the first detailed infrared chemical analysis of five binary members (S277, S997, S975, S1031, and S1195) in the open cluster M67 (NGC2682). These stars are located... -
TESS-Keck Survey. XVI. 8 systems Radial velocity
With JWST's successful deployment and unexpectedly high fuel reserves, measuring the masses of sub-Neptunes transiting bright, nearby stars will soon become the bottleneck for... -
Gaia Ultra-Cool Dwarf candidates IR spectra
The local census of very low-mass stars and brown dwarfs is crucial to improving our understanding of the stellar-substellar transition and their formation history. These... -
S CrA full L- and M-band spectra
The Cryogenic IR echelle Spectrometer (CRIRES) instrument at the Very Large Telescope (VLT) was in operation from 2006 to 2014. Great strides in characterizing the inner regions... -
C-19 stream members
Stellar ejecta gradually enrich the gas out of which subsequent stars form, making the least chemically enriched stellar systems direct fossils of structures formed in the early...
