Showing 1–20 of 134 results
/ Date/ Name
Feb 21, 2013Determining accurate measurements of the growth rate from the galaxy correlation function in simulationsFeb 21, 2013The WiggleZ Dark Energy Survey: measuring the cosmic growth rate with the two-point galaxy correlation functionFeb 12, 2025Modified Homotopic approach for diffractive productionMar 27, 2018SN 2012fr: Ultraviolet, Optical, and Near-Infrared Light Curves of a Type Ia Supernova Observed Within a Day of ExplosionMay 4, 2020The Relationship between Mid-Infrared and Sub-Millimetre Variability of Deeply Embedded ProtostarsMar 15, 2023Photometric and Spectroscopic monitoring of YSOs in nearby star forming regions. I. Eruptive YSOsJan 25, 2024On the incidence of episodic accretion in Class I YSOs from VVVNov 29, 2004Determination of the b-mass using renormalon cancellationApr 30, 2025"Oh FUors where art thou": A search for long-lasting YSO outbursts hiding in infrared surveysJun 26, 2018DGLAP evolution for DIS diffraction production of high massesAug 12, 2009SN 2003bg: The First Type IIb HypernovaJul 24, 2008A New Distance to The Antennae Galaxies (NGC 4038/39) Based on the Type Ia Supernova 2007srFeb 20, 2013The Stellar Masses of ~40,000 UV Selected Galaxies from the WiggleZ Survey at 0.3<z<1.0: Analogues of Lyman Break Galaxies?Jun 12, 2014VISTA Variables in the Vía Láctea (VVV): Halfway Status and ResultsJun 4, 2014Non linear evolution: revisiting the solution in the saturation regionJul 24, 2014Supernova 2010as: the Lowest-Velocity Member of a Family of Flat-Velocity Type IIb SupernovaeSep 12, 2002Determination of $α_s$ from Gross-Llewellyn Smith sum rule by accounting for infrared renormalonJul 19, 2018Red vs Blue: Early observations of thermonuclear supernovae reveal two distinct populations?Sep 22, 2020The value of the Hubble-Lemaître constant queried by Type Ia Supernovae: A journey from the Calán-Tololo Project to the Carnegie Supernova ProgramOct 18, 2018Carnegie Supernova Project-II: Extending the Near-Infrared Hubble Diagram for Type Ia Supernovae to $z\sim0.1$