activity
20002023
most citedThe Man Behind the Curtain: X-rays Drive the UV through NIR Variability in the 2013 AGN Outburst in NGC 2617

1.9k citations · 15.3k across the 197 of their papers we have counts for

collaborators
Showing 2022Show all

11 papers · 1 filter

astro-ph.GA2022★ 52 cited

The Pan-STARRS1 z>5.6 quasar survey II: Discovery of 55 Quasars at 5.6<z<6.5

Eduardo Banados, Jan-Torge Schindler, Bram P. Venemans +20

The identification of bright quasars at z>6 enables detailed studies of supermassive black holes, massive galaxies, structure formation, and the state of the intergalactic medium w…

astro-ph.SR2022

A Survey for C II Emission-Line Stars in the Large Magellanic Cloud. II. Final Results and the Origin of C II Emission in [WC] Spectra

Bruce Margon, Nidia Morrell, Philip Massey +2

We present the final results of an imaging and spectroscopic search for stars in the Large Magellanic Cloud (LMC) with C II 7231, 7236 emission lines. The goal is to identify and s…

astro-ph.HE2022★ 15 cited

Carnegie Supernova Project-II: Near-infrared spectral diversity and template of Type Ia Supernovae

Jing Lu, Eric Y. Hsiao, Mark M. Phillips +30

We present the largest and most homogeneous collection of near-infrared (NIR) spectra of Type Ia supernovae (SNe Ia): 339 spectra of 98 individual SNe obtained as part of the Carne…

astro-ph.HE2022★ 36 cited

A JWST Near- and Mid-Infrared Nebular Spectrum of the Type Ia Supernova 2021aefx

Lindsey A. Kwok, Saurabh W. Jha, Tea Temim +55

We present JWST near- and mid-infrared spectroscopic observations of the nearby normal Type Ia supernova SN 2021aefx in the nebular phase at days past maximum light. Our Nea…

astro-ph.HE2022★ 9 cited

Near-infrared and Optical Nebular-phase Spectra of Type Ia Supernovae SN 2013aa and SN 2017cbv in NGC 5643

Sahana Kumar, Eric Y. Hsiao, Chris Ashall +23

We present multi-wavelength time-series spectroscopy of SN 2013aa and SN 2017cbv, two Type Ia supernovae (SNe Ia) on the outskirts of the same host galaxy, NGC 5643. This work util…

astro-ph.HE2022★ 23 cited

The Absolute Magnitudes of 1991T-like Supernovae

M. M. Phillips, C. Ashall, Christopher R. Burns +20

1991T-like supernovae are the luminous, slow-declining extreme of the Branch shallow-silicon (SS) subclass of Type Ia supernovae. They are distinguished by extremely weak Ca II H &…

astro-ph.GA2022★ 4 cited

Examining the Properties of Low-Luminosity Hosts of Type Ia Supernovae from ASAS-SN

Thomas W. -S. Holoien, Vera L. Berger, Jason T. Hinkle +14

We present a spectroscopic analysis of 44 low-luminosity host galaxies of Type Ia supernovae (SNe Ia) detected by the All-Sky Automated Survey for Supernovae (ASAS-SN), using the e…

astro-ph.SR2022★ 20 cited

The origin and evolution of the normal Type Ia SN 2018aoz with infant-phase reddening and excess emission

Yuan Qi Ni, Dae-Sik Moon, Maria R. Drout +40

SN~2018aoz is a Type Ia SN with a -band plateau and excess emission in the infant-phase light curves 1 day after first light, evidencing an over-density of surface ir…

astro-ph.SR2022★ 33 cited

WO-Type Wolf-Rayet Stars: the Last Hurrah of Massive Star Evolution

Erin Aadland, Philip Massey, D. John Hillier +3

Are WO-type Wolf Rayet (WR) stars in the final stage of massive star evolution before core-collapse? Although WC- and WO-type WRs have very similar spectra, WOs show a much stronge…

astro-ph.HE2022★ 32 cited

Infant-phase reddening by surface Fe-peak elements in a normal Type Ia Supernova

Yuan Qi Ni, Dae-Sik Moon, Maria R. Drout +41

Type Ia Supernovae are thermonuclear explosions of white dwarf stars. They play a central role in the chemical evolution of the Universe and are an important measure of cosmologica…

astro-ph.HE2022★ 16 cited

SN 2012ij: A low-luminosity type Ia supernova and evidence for continuous distribution from 91bg-like explosion to normal ones

Zhitong Li, Tianmeng Zhang, Xiaofeng Wang +24

In this paper, we present photometric and spectroscopic observations of a subluminous type Ia supernova (SN Ia) 2012ij, which has an absolute -band peak magnitude $M_{B,\rm{max}…