Search Publications

Structural Parameters and Possible Association of the Ultra-faint Dwarfs Pegasus III and Pisces II from Deep Hubble Space Telescope Photometry
DOI: 10.3847/1538-4357/ac7226 Bibcode: 2022ApJ...933..217R

Choi, Yumi; van der Marel, Roeland P.; Geha, Marla +17 more

We present deep Hubble Space Telescope (HST) photometry of the ultra-faint dwarf (UFD) galaxies Pegasus III (Peg III) and Pisces II (Psc II), two of the most distant satellites in the halo of the Milky Way (MW). We measure the structure of both galaxies, derive mass-to-light ratios with newly determined absolute magnitudes, and compare our finding…

2022 The Astrophysical Journal
Gaia eHST 14
Validation of a Wave Heated 3D MHD Coronal-wind Model using Polarized Brightness and EUV Observations
DOI: 10.3847/1538-4357/ac56da Bibcode: 2022ApJ...929...75P

Pinto, Rui F.; Réville, Victor; Strugarek, Antoine +5 more

The physical properties responsible for the formation and evolution of the corona and heliosphere are still not completely understood. 3D MHD global modeling is a powerful tool to investigate all the possible candidate processes. To fully understand the role of each of them, we need a validation process where the output from the simulations is qua…

2022 The Astrophysical Journal
SOHO 14
New Time-resolved, Multi-band Flares in the GJ 65 System with gPhoton
DOI: 10.3847/1538-4357/ac5037 Bibcode: 2022ApJ...928....8F

Brasseur, C. E.; Osten, Rachel A.; Fleming, Scott W. +2 more

Characterizing the distribution of flare properties and occurrence rates is important for understanding habitability of M-dwarf exoplanets. The Galaxy Evolution Explorer (GALEX) space telescope observed the GJ 65 system, composed of the active, flaring M stars BL Cet and UV Cet, for 15,900 s (~4.4 hr) in two ultraviolet (UV) bands. The contrast in…

2022 The Astrophysical Journal
Gaia 14
A Mass Model for the Lensing Cluster SDSS J1004+4112: Constraints from the Third Time Delay
DOI: 10.3847/1538-4357/ac8c40 Bibcode: 2022ApJ...937...35F

Kochanek, C. S.; Muñoz, J. A.; Mediavilla, E. +1 more

We have built a new model for the lens system SDSS J1004+4112 including the recently measured time delay of the fourth quasar image. This time delay has a strong influence on the inner mass distribution of the lensing cluster (ρ ∝ r ) allowing us to determine $\alpha ={1.18}_{-0.03(-0.18)}^{+0.02(+0.11)}$ at the 68% (95%) confidence …

2022 The Astrophysical Journal
eHST 14
A Multiwavelength View of IC 860: What Is in Action inside Quenching Galaxies
DOI: 10.3847/1538-4357/ac8b7d Bibcode: 2022ApJ...938...63L

Heckman, Timothy; Aalto, Susanne; French, K. Decker +15 more

We present a multiwavelength study of IC 860, a nearby post-starburst galaxy at the early stage of transitioning from blue and star forming to red and quiescent. Optical images reveal a galaxy-wide, dusty outflow originating from a compact core. We find evidence for a multiphase outflow in the molecular and neutral gas phase from the CO position-v…

2022 The Astrophysical Journal
AKARI Herschel eHST 14
Lyα Halos around [O III]-selected Galaxies in HETDEX
DOI: 10.3847/2041-8213/ac82e5 Bibcode: 2022ApJ...934L..26L

Finkelstein, Steven L.; Schneider, Donald P.; Gebhardt, Karl +13 more

We present extended Lyα emission out to 800 kpc of 1034 [O III]-selected galaxies at redshifts 1.9 < z < 2.35 using the Hobby-Eberly Telescope Dark Energy Experiment. The locations and redshifts of the galaxies are taken from the 3D-HST survey. The median-stacked surface brightness profile of the Lyα emission of the [O III]-selected galaxies…

2022 The Astrophysical Journal
eHST 14
The Donor of the Black Hole X-Ray Binary MAXI J1820+070
DOI: 10.3847/1538-4357/ac6099 Bibcode: 2022ApJ...930....9M

Mikołajewska, Joanna; Casares, Jorge; Zdziarski, Andrzej A. +2 more

We estimate the parameters of the donor of the accreting black hole binary MAXI J1820+070. The measured values of the binary period, rotational and radial velocities, and constraints on the orbital inclination imply the donor is a subgiant with the mass of ${M}_{2}\approx {0.49}_{-0.10}^{+0.10}{M}_{\odot }$ and the radius of ${R}_{2}\approx {1.19}…

2022 The Astrophysical Journal
Gaia 13
Genesis and Coronal-jet-generating Eruption of a Solar Minifilament Captured by IRIS Slit-raster Spectra
DOI: 10.3847/1538-4357/ac8d65 Bibcode: 2022ApJ...939...25P

Tiwari, Sanjiv K.; De Pontieu, Bart; Panesar, Navdeep K. +2 more

We present the first Mg II slit-raster spectra from the Interface Region Imaging Spectrograph (IRIS) that fully capture the genesis and coronal-jet-generating eruption of a central-disk solar minifilament. The minifilament arose in a negative-magnetic-polarity coronal hole. The Mg II spectroheliograms verify that the minifilament plasma temperatur…

2022 The Astrophysical Journal
IRIS 13
Ultrafaint Dwarf Galaxy Candidates in the M81 Group: Signatures of Group Accretion
DOI: 10.3847/2041-8213/ac8e5e Bibcode: 2022ApJ...937L...3B

Bell, Eric F.; Monachesi, Antonela; Bailin, Jeremy +8 more

The faint and ultrafaint dwarf galaxies in the Local Group form the observational bedrock upon which our understanding of small-scale cosmology rests. In order to understand whether this insight generalizes, it is imperative to use resolved-star techniques to discover similarly faint satellites in nearby galaxy groups. We describe our search for u…

2022 The Astrophysical Journal
eHST 13
Constraints on Cosmological Parameters with a Sample of Type Ia Supernovae from JWST
DOI: 10.3847/1538-4357/ac9f49 Bibcode: 2022ApJ...941...71L

Koekemoer, Anton M.; Baade, Dietrich; Wang, Lifan +7 more

We investigate the potential of using a sample of very high-redshift (2 ≲ z ≲ 6) (VHZ) Type Ia supernovae (SNe Ia) attainable by JWST on constraining cosmological parameters. At such high redshifts, the age of the universe is young enough that the VHZ SN Ia sample comprises the very first SNe Ia of the universe, with progenitors among the very fir…

2022 The Astrophysical Journal
eHST 13