activity
20052025
most citediPTF16geu: A multiply imaged, gravitationally lensed type Ia supernova

246 citations · 839 across the 13 of their papers we have counts for

collaborators

12 papers

astro-ph.CO2025★ 1 cited

SN 2025ogs: A Spectroscopically-Normal Type Ia Supernova at z = 2 as a Benchmark for Redshift Evolution

M. R. Siebert, J. D. R. Pierel, M. Engesser +20

The Nancy Grace Roman Space Telescope will provide a revolutionary measurement of the Universe's expansion kinematics, driven by dark matter and dark energy, out to .…

astro-ph.HE2025★ 1 cited

Discovery of a likely Type II SN at =3.6 with JWST

D. A. Coulter, J. D. R. Pierel, C. DeCoursey +30

Transient astronomy in the early, high-redshift (z > 3) Universe is an unexplored regime that offers the possibility of probing the first stars and the Epoch of Reionization. Durin…

astro-ph.CO2024

Testing for Intrinsic Type Ia Supernova Luminosity Evolution at z>2 with JWST

J. D. R. Pierel, D. A. Coulter, M. R. Siebert +38

The James Webb Space Telescope} (JWST) is opening new frontiers of transient discovery and follow-up at high-redshift. Here we present the discovery of a spectroscopically confirme…

astro-ph.HE2017★ 144 cited

Light curves of hydrogen-poor Superluminous Supernovae from the Palomar Transient Factory

Annalisa De Cia, A. Gal-Yam, A. Rubin +24

We investigate the light-curve properties of a sample of 26 spectroscopically confirmed hydrogen-poor superluminous supernovae (SLSNe-I) in the Palomar Transient Factory (PTF) surv…

astro-ph.HE2017★ 40 cited

A tale of two transients: GW170104 and GRB170105A

V. Bhalerao, M. M. Kasliwal, D. Bhattacharya +30

We present multi-wavelength follow-up campaigns by the AstroSat-CZTI and GROWTH collaborations to search for an electromagnetic counterpart to the gravitational wave event GW170104…

astro-ph.HE2017★ 28 cited

iPTF17cw: An engine-driven supernova candidate discovered independent of a gamma-ray trigger

A. Corsi, S. B. Cenko, M. M. Kasliwal +21

We present the discovery, classification, and radio-to-X-ray follow-up observations of iPTF17cw, a broad-lined (BL) type Ic supernova (SN) discovered by the intermediate Palomar Tr…

astro-ph.HE2017★ 114 cited

Hydrogen-poor Superluminous Supernovae With Late-time H-alpha Emission: Three Events From the Intermediate Palomar Transient Factory

Lin Yan, R. Lunnan, D. Perley +20

We present observations of two new hydrogen-poor superluminous supernovae (SLSN-I), iPTF15esb and iPTF16bad, showing late-time H-alpha emission with line luminosities of (1-3)e+41…

astro-ph.CO2016★ 246 cited

iPTF16geu: A multiply imaged, gravitationally lensed type Ia supernova

A. Goobar, R. Amanullah, S. R. Kulkarni +31

We report the discovery of a multiply-imaged gravitationally lensed Type Ia supernova, iPTF16geu (SN 2016geu), at redshift . This phenomenon could be identified because th…

astro-ph.HE2014★ 87 cited

A Luminous, Fast Rising UV-Transient Discovered by ROTSE: a Tidal Disruption Event?

J. Vinko, F. Yuan, R. M. Quimby +6

We present follow-up observations of an optical transient (OT) discovered by ROTSE on Jan. 21, 2009. Photometric monitoring was carried out with ROTSE-IIIb in the optical and Swift…

astro-ph.HE2011★ 85 cited

Sn 2008in - bridging the gap between normal and faint supernovae of type IIP

Rupak Roy, Brijesh Kumar, Stefano Benetti +18

We present optical photometric and low-resolution spectroscopic observations of the Type II plateau supernova (SN) 2008in, which occurred in the outskirts of the nearly face-on spi…

astro-ph2007★ 26 cited

M31N-2007-06b: A Nova in the M31 Globular Cluster Bol 111

A. W. Shafter, R. M. Quimby

We report spectroscopic observations of the nova M31N-2007-06b, which was found to be spatially coincident with the M31 globular cluster Bol 111. This nova is the first out of more…

astro-ph2005★ 41 cited

Spectroscopic Observations and Analysis of the Unusual Type Ia SN 1999ac

The Supernova Cosmology Project, :, G. Garavini +55

We present optical spectra of the peculiar Type Ia supernova (SN Ia) 1999ac. The data extend from -15 to +42 days with respect to B-band maximum and reveal an event that is unusual…