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Magnetar XTEJ1810-197 follow-up 300-1450MHz GMRT obs.
We present the long-term spectro-temporal evolution of the average radio emission properties of the magnetar XTE J1810-197 (PSRJ1809-1943), following its most recent outburst in... -
z~2-10 galaxies magnified by HFF clusters. I.
We assemble a large comprehensive sample of 2534 z~2, 3, 4, 5, 6, 7, 8, and 9 galaxies lensed by the six clusters from the Hubble Frontier Fields (HFF) program. Making use of... -
The GALEX-PTF experiment. II. Core-collapse SNe
The radius and surface composition of an exploding massive star, as well as the explosion energy per unit mass, can be measured using early ultraviolet (UV) observations of... -
Subaru/HSC imaging of SQuIGGLE z~0.7 galaxies
We present structural measurements of 145 spectroscopically selected intermediate-redshift (z~0.7), massive (M_*~10^11^M{sun}_) post-starburst galaxies from the SQuIGG->LE... -
Galaxy Zoo: Clump Scout: clumpy SDSS gal. at z~<0.2
Massive, star-forming clumps are a common feature of high-redshift star-forming galaxies. How they formed, and why they are so rare at low redshift, remains unclear. In this... -
Variability of Sgr A* in 2019 July
We report a timing analysis of near-infrared (NIR), X-ray, and submillimeter data during a 3 day coordinated campaign observing Sagittarius A. Data were collected at 4.5um with... -
The factory & the beehive. IV. Praesepe & Hyades
X-ray observations of low-mass stars in open clusters are critical to understanding the dependence of magnetic activity on stellar properties and their evolution. Praesepe and... -
LBT/MODS spectrum of the host galaxy of GRB 200826A
Gamma-ray bursts (GRBs) are classified into long and short events. Long GRBs (LGRBs) are associated with the end states of very massive stars, while short GRBs (SGRBs) are... -
A multiwavelength study of GRS 1716-249 in outburst
We present a detailed study of the evolution of the Galactic black hole transient GRS 1716-249 during its 2016-2017 outburst at optical (Las Cumbres Observatory), mid-infrared... -
Ly{beta} dark gaps in z<~6 QSOs spectra
We present a new investigation of the intergalactic medium near reionization using dark gaps in the Ly{beta} forest. With its lower optical depth, Ly{beta} offers a potentially... -
The redshift evolution of ULXs out to z~0.5
Ultraluminous X-ray sources (ULXs) are thought to be powerful X-ray binaries (XRBs) and may contribute significantly to the redshift-dependent X-ray emission from star-forming... -
Insight-HXMT high energy X-ray obs. of EXO1846-031
We study the spectral evolution of the black hole candidate EXO1846-031 during its 2019 outburst, in the 1-150keV band, with the Hard X-ray Modulation Telescope. The continuum... -
0.4-10keV X-ray monitoring of Eta Car
We report high-precision X-ray monitoring observations in the 0.4-10keV band of the luminous, long-period colliding wind binary Eta Carinae, up to and through its most recent... -
TDSS. Changing-look quasars candidates
Active galactic nuclei (AGN) can vary significantly in their rest-frame optical/UV continuum emission, and with strong associated changes in broad line emission, on much shorter... -
NIR HST photometry of SNIa from the RAISIN survey
Type Ia supernovae (SNe Ia) are more precise standardizable candles when measured in the near-infrared (NIR) than in the optical. With this motivation, from 2012 to 2017 we... -
Brightest cluster galaxies from SDSS-IV MaNGA
Although it is generally accepted that massive galaxies form in a two-phased fashion, beginning with a rapid mass buildup through intense starburst activities followed by... -
F125W and UV mag of 6.0<z<8.2 galaxies candidates
Reionization is an inhomogeneous process, thought to begin in small ionized bubbles of the intergalactic medium (IGM) around overdense regions of galaxies. Recent Ly{alpha}... -
WISE-2MASS (W2M) quasars and red QSOs with sp.
We present a highly complete sample of broad-line (Type 1) QSOs out to z~3 selected by their mid-infrared colors, a method that is minimally affected by dust reddening. We... -
PS1 3{pi} analysis of z~0.3 QSOs host galaxies
We investigate the star-forming main sequence of the host galaxies of a large, well-defined sample of 453 redshift ~0.3 quasars with previously available star formation rates by... -
Combination of Planck and SPT cluster catalogs
We provide the first combined cosmological analysis of the South Pole Telescope (SPT) and Planck cluster catalogs. The aim is to provide an independent calibration for Planck...