activity
20132026
most citedK2 Observations of SN 2018oh Reveal a Two-Component Rising Light Curve for a Type Ia Supernova

106 citations · 665 across the 20 of their papers we have counts for

collaborators

21 papers

astro-ph.IM2026

The Roman Coronagraph Community Participation Program: data reduction pipeline design and implementation

Jason J. Wang, Maxwell A. Millar-Blanchaer, Marie Ygouf +39

The Roman Space Telescope Coronagraph Instrument will demonstrate a series of technologies and techniques to enable the direct detection of reflected-light planets with space-based…

astro-ph.EP2025

NIRCam yells at cloud: JWST MIRI imaging can directly detect exoplanets of the same temperature, mass, age, and orbital separation as Saturn and Jupiter

Rachel Bowens-Rubin, James Mang, Mary Anne Limbach +9

NIRCam and MIRI coronagraphy have successfully demonstrated the ability to directly image young sub-Jupiter mass and mature gas-giant exoplanets. However, these modes struggle to r…

astro-ph.SR2024

HST Survey of the Orion Nebula Cluster in ACS/Visible and WFC3/IR Bands. IV. A Bayesian multi-wavelength study of stellar parameters in the ONC

Giovanni M. Strampelli, Massimo Robberto, Laurent Pueyo +4

We have performed a comprehensive study of the Orion Nebula Cluster (ONC) combining the photometric data obtained by the two \textit{HST} Treasury programs that targeted this regio…

astro-ph.GA2023

A HST Study of the Substellar Population of NGC 2024

Massimo Robberto, Mario Gennaro, Nicola Da Rio +6

We performed a HST/WFC3-IR imaging survey of the young stellar cluster NGC 2024 in three filters probing the 1.4~m HO absorption feature, characteristic of the population of…

astro-ph.IM2022★ 1 cited

StraKLIP: A novel pipeline for detection and characterization of close-in faint companions through Karhunen-Loêve Image Processing algorithm

Giovanni M. Strampelli, Laurent Pueyo, Jonathan Aguilar +3

We present a new pipeline developed to detect and characterize faint astronomical companions at small angular separation from the host star using sets of wide-field imaging observa…

astro-ph.SR2022★ 15 cited

Searching for a Hypervelocity White Dwarf Companion: A Proper Motion Survey of SN 1006

Joshua V. Shields, Wolfgang Kerzendorf, Matthew W. Hosek +7

Type Ia Supernovae (SNe Ia) are securely understood to come from the thermonuclear explosion of a white dwarf as a result of binary interaction, but the nature of that binary inter…

astro-ph.SR2020★ 16 cited

HST astrometry in the Orion Nebula Cluster: census of low-mass runaways

Imants Platais, Massimo Robberto, Andrea Bellini +6

We present a catalog of high-precision proper motions in the Orion Nebula Cluster (ONC), based on Treasury Program observations with the Hubble Space Telescope's (HST) ACS/WFC came…

astro-ph.SR2020★ 8 cited

HST survey of the Orion Nebula Cluster in the HO 1.4 m absorption band: III. The population of sub-stellar binary companions

Giovanni M. Strampelli, Jonathan Aguilar, Laurent Pueyo +4

We present new results concerning the sub-stellar binary population in the Orion Nebula Cluster (ONC). Using the Karhunen-Loève Image Projection (KLIP) algorithm, we have reprocess…

astro-ph.SR2020★ 22 cited

HST survey of the Orion Nebula Cluster in the HO 1.4 m absorption band: I. A census of substellar and planetary mass objects

Massimo Robberto, Mario Gennaro, Maria Giulia Ubeira Gabellini +15

In order to obtain a complete census of the stellar and sub-stellar population, down to a few M in the Myr old Orion Nebula Cluster, we used the infrared channel of…

astro-ph.SR2020★ 19 cited

The not so simple stellar system Omega Cen. II. Evidence in support of a merging scenario

Annalisa Calamida, Alice Zocchi, Giuseppe Bono +7

We present multi-band photometry covering 5° 5°across Cen collected with the Dark Energy Camera, combined to Hubble Space Telescope and Wide Field Imager data fo…

astro-ph.HE2018★ 40 cited

Nebular Spectroscopy of Kepler's Brightest Supernova

G. Dimitriadis, C. Rojas-Bravo, C. D. Kilpatrick +9

We present late-time (240-260 days after peak brightness) optical photometry and nebular (+236 and +264 days) spectroscopy of SN 2018oh, the brightest Type Ia supernova (SN I…

astro-ph.HE2018★ 106 cited

K2 Observations of SN 2018oh Reveal a Two-Component Rising Light Curve for a Type Ia Supernova

G. Dimitriadis, R. J. Foley, A. Rest +145

We present an exquisite, 30-min cadence Kepler (K2) light curve of the Type Ia supernova (SN Ia) 2018oh (ASASSN-18bt), starting weeks before explosion, covering the moment of explo…

astro-ph.IM2018★ 37 cited

Sub-percent Photometry: Faint DA White Dwarf Spectophotometric Standards for Astrophysical Observatories

Gautham Narayan, Thomas Matheson, Abhijit Saha +18

We have established a network of 19 faint (16.5 mag 19 mag) northern and equatorial DA white dwarfs as spectrophotometric standards for present and future wide-field observ…

astro-ph.SR2018★ 73 cited

Light-echoes from the plateau in Eta Carinae's Great Eruption reveal a two-stage shock-powered event

Nathan Smith, Jennifer E. Andrews, Armin Rest +7

We present multi-epoch photometry and spectroscopy of a light echo from eta Carinae's 19th century Great Eruption. This echo shows a steady decline over a decade, sampling the 1850…

astro-ph.HE2018★ 87 cited

Seeing Double: ASASSN-18bt Exhibits a Two-Component Rise in the Early-Time K2 Light Curve

B. J. Shappee, T. W. -s. Holoien, M. R. Drout +109

On 2018 Feb. 4.41, the All-Sky Automated Survey for SuperNovae (ASAS-SN) discovered ASASSN-18bt in the K2 Campaign 16 field. With a redshift of z=0.01098 and a peak apparent magnit…

astro-ph.HE2018★ 1 cited

A Fast-Evolving, Luminous Transient Discovered by K2/Kepler

A. Rest, P. M. Garnavich, D. Khatami +12

For decades optical time-domain searches have been tuned to find ordinary supernovae, which rise and fall in brightness over a period of weeks. Recently, supernova searches have im…

astro-ph.SR2017★ 44 cited

A Search for a Surviving White Dwarf Companion in SN 1006

W. E. Kerzendorf, G. Strampelli, K. J. Shen +5

Multiple channels have been proposed to produce Type Ia supernovae, with many scenarios suggesting that the exploding white dwarf accretes from a binary companion pre-explosion. In…

astro-ph.SR2017★ 73 cited

Connecting the progenitors, pre-explosion variability, and giant outbursts of luminous blue variables with Gaia16cfr

Charles D. Kilpatrick, Ryan J. Foley, Maria R. Drout +10

We present multi-epoch, multi-colour pre-outburst photometry and post-outburst light curves and spectra of the luminous blue variable (LBV) outburst Gaia16cfr discovered by the Gai…

astro-ph.GA2017★ 26 cited

The not so simple globular cluster Cen. I. Spatial distribution of the multiple stellar populations

A. Calamida, G. Strampelli, A. Rest +8

We present a multi-band photometric catalog of 1.7 million cluster members for a field of view of 2x2 degree across Cen. Photometry is based on images colle…

astro-ph.HE2016★ 57 cited

A DECam Search for an Optical Counterpart to the LIGO Gravitational Wave Event GW151226

P. S. Cowperthwaite, E. Berger, M. Soares-Santos +97

We report the results of a Dark Energy Camera (DECam) optical follow-up of the gravitational wave (GW) event GW151226, discovered by the Advanced LIGO detectors. Our observations c…

astro-ph.SR2013

The soundtrack of RR Lyrae in Omega Cen at high-frequency

A. Calamida, S. K. Randall, M. Monelli +8

We present preliminary Sloan u',g'-band light curves for a sample of known RR Lyrae variables in the Galactic globular cluster Omega Cen. Results are based on the partial reduction…