A. Canto

Universidad Complutense de Madrid

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M. Kowalski

Humboldt-Universität zu Berlin

K. Runge

Lawrence Berkeley National Laboratory

S. Perlmutter

Lawrence Berkeley National Laboratory

ÉG

É. Gangler

Centre National de la Recherche Scientifique

N. Chotard

Centre National de la Recherche Scientifique

P. Nugent

Lawrence Berkeley National Laboratory

R. Pereira

Eduardo Mondlane University

P. Antilogus

Centre National de la Recherche Scientifique

S. Bongard

Laboratoire de Physique Nucléaire et de Hautes Énergies

C. Baltay

Yale University

Cooperative Institutions

Lawrence Berkeley National Laboratory

Centre National de la Recherche Scientifique

Institut National de Physique Nucléaire et de Physique des Particules

University of California, Berkeley

Université Paris Cité

Laboratoire de Physique Nucléaire et de Hautes Énergies

Max Planck Institute for Astrophysics

Université Claude Bernard Lyon 1

Sorbonne Université

Max Planck Society

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Spectrophotometric time series of SN 2011fe from the Nearby Supernova Factory

Astronomy and Astrophysics (2013)

R. Pereira R. C. Thomas G. Aldering P. Antilogus C. Baltay

We present 32 epochs of optical (3300-9700 \AA) spectrophotometric observations of the nearby quintessential "normal" type Ia supernova (SN Ia) SN 2011fe in the galaxy M101, extending from -15 to +97 d with respect to B-band maximum, obtained by the Nearby Supernova Factory collaboration. SN 2011fe is the closest (\mu = 29.04) and brightest (Bmax = 9.94 mag) SN Ia observed since the advent of modern large scale programs for the intensive periodic followup of supernovae. Both synthetic light curve measurements and spectral feature analysis attest to the normality of SN 2011fe. There is very little evidence for reddening in its host galaxy. The homogeneous calibration, intensive time sampling, and high signal-to-noise ratio of the data set make it unique. Thus it is ideal for studying the physics of SN Ia explosions in detail, and for furthering the use of SNe Ia as standardizable candles for cosmology. Several such applications are shown, from the creation of a bolometric light curve and measurement of the 56Ni mass, to the simulation of detection thresholds for unburned carbon, direct comparisons with other SNe Ia, and existing spectral templates.

Factory (object-oriented programming)

10.1051/0004-6361/201221008

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Spectroscopic classification of Two LSQ supernovae by the Nearby Supernova Factory II

The astronomer's telegram (2012)

G. Aldering D. Birchall M. Childress H. Fakhouri A. Kim

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Nearby Supernova Factory II Spectroscopic Classification of LSQ13aze, LSQ13bbv and LSQ13bbz

The astronomer's telegram (2013)

Y. Copin N. Chotard É. Gangler R. Pereira M. Rigault

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Principal Component Analysis of Type Ia Supernova Spectrophotometric Time Series

American Astronomical Society Meeting Abstracts #223 (2014)

C. Saunders G. Aldering S. Bailey D. Birchall M. Childress

Component (thermodynamics)

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Measuring cosmic bulk flows with Type Ia supernovae from the Nearby Supernova Factory(Corrigendum)

Astronomy and Astrophysics (2015)

U. Feindt M. Kerschhaggl M. Kowalski G. Aldering P. Antilogus

Author(s): Feindt, U; Kerschhaggl, M; Kowalski, M; Aldering, G; Antilogus, P; Aragon, C; Bailey, S; Baltay, C; Bongard, S; Buton, C; Canto, A; Cellier-Holzem, F; Childress, M; Chotard, N; Copin, Y; Fakhouri, HK; Gangler, E; Guy, J; Kim, A; Nugent, P; Nordin, J; Paech, K; Pain, R; Pecontal, E; Pereira, R; Perlmutter, S; Rabinowitz, D; Rigault, M; Runge, K; Saunders, C; Scalzo, R; Smadja, G; Tao, C; Thomas, RC; Weaver, BA; Wu, C

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10.1051/0004-6361/201321880e

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Spectroscopic Observation of the Bright PSN in NGC2857 by the Nearby Supernova Factory II

The astronomer's telegram (2012)

F. Cellier-Holzem A. Canto P. Antilogus S. Bongard R. Pain

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Classification of SN 2010hb, an early Type II supernova

ATel (2010)

G. Aldering M. Childress H. Fakhouri E. Y. Hsiao S. Loken

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Nearby Supernova Factory II classification of three SNe and two non-detections

ATel (2013)

G. Aldering D. Birchall H. Fakhouri A. Kim J. Nordin

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Understanding U-band Spectroscopic Variations in Type Ia Supernovae

American Astronomical Society Meeting Abstracts #223 (2014)

J. Nordin G. Aldering S. Bailey D. Birchall M. Childress

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Local host galaxy properties of type Ia supernovae from the Nearby SuperNovae Factory

M. Rigault Y. Copin G. Aldering P. Antilogus C. Aragon

Type Ia supernovae are key tools to study accelerating expansion of the Universe. However despite active research, physics of such objects remain uncertain. To better understand potential systematics we investigate on local host galaxy properties. In this preliminary analysis, we find gas derived quantities such as metallicity and star formation rate compatible to those present in literature. Finally we show a relationship between SALT2 color and x_1 with star formation activity.

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