Neurophysiology: Sensing temperature without ion channels

By Brandon R. Brown. Nature, 2008

403 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/75c8ce13a937b05df446efc4ed9848e205bfa9fe

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Citations in the corpus

• Resolving the effect of climate change on fish populations (2009, background): “Some elasmobranchs are extremely sensitive to temperature variation (e.g. they can respond to changes of ,0.0018C; Brown, 2003) and some sharks move to deeper water before the onset of severe storms (Heupel et al., 2003).”
• EARLY SUPERNOVAE LIGHT CURVES FOLLOWING THE SHOCK BREAKOUT (2010, background): “The development during the recent decade of sensitive UV, X-ray and soft gamma-ray detectors, with relatively large fields of view, lead to the discovery of several shock breakout candidates (Campana et al. 2006; Soderberg et al. 2008; Gezari et al. 2008; Schawinski et al. 2008; Modjaz et al. 2009).”
• Core-collapse explosions of Wolf–Rayet stars and the connection to Type IIb/Ib/Ic supernovae (2011, background): “It cannot be due to a large progenitor radius since analysis of the early X-ray light curve (Soderberg et al. 2008; Modjaz et al. 2009) supports a progenitor radius ofR∗ ∼ < 1R⊙.”
• SUPERNOVA LIGHT CURVES POWERED BY FALLBACK ACCRETION (2012, background): “Example fits are shown in Figure 5 for SN 1998bw (Galama et al. 1998) and SN 2008D (Soderberg et al. 2008).”
• A cocoon shock breakout as the origin of the γ-ray emission in GW170817 (2017, background): “Similar bulk to breakout energy ratios are seen in breakout candidates such as SN2008D (Soderberg et al. 2008) and low-luminosity long GRBs (e.g., Kulkarni et al. 1998; ?).”
• Nearby Supernova Rates from the Lick Observatory Supernova Search. II. The Observed Luminosity Functions and Fractions of Supernovae in a Complete Sample (2010, background): “This doublepeak light curve behaviour has most recently also been seen in the Type Ib SN 2008D (Soderberg et al. 2008; Modjaz et al. 2009).”
• OPTICAL SPECTRA OF 73 STRIPPED-ENVELOPE CORE-COLLAPSE SUPERNOVAE (2014, background): “SN 2008D. SN 2008D and its X-ray outburst 080109 have been well studied (e.g., Soderberg et al. 2008; Mazzali et al. 2008; Modjaz et al. 2009; Malesani et al. 2009; Maund et al. 2009; Tanaka et al. 2009).”
• The Carnegie Supernova Project I: analysis of stripped-envelope supernova light curves (2017, background): “Evidence of this phenomenon was first documented in the peculiar Type II SN 1987A (e.g., Catchpole et al. 1987), the Type IIb SN 1993J (e.g., Van Driel et al. 1993), the Type Ib/c SN 1999ex (Stritzinger et al. 2002) and the Type Ib SN 2008D (e.g., Mazzali et al. 2008; Soderberg et al. 2008).”
• Real world contexts in PISA science : implications for context-based science education (2009, background): “It was the explosion of a dying star, 7.5 billion light years away, as the star collapsed into a black hole, driving bright gas jets into space (Soderberg et al, 2008) It was “one of the biggest bangs since the big one”, and “the most distant astronomical object ever seen by humans” – claims for…”
• On the nature of supernovae Ib and Ic (2012, background): “Several nearby events received special attention, such as the SN Ib 2008D (Soderberg et al. 2008; Modjaz et al. 2009) or the SN Ic 1994I (Filippenko et al. 1995; Clocchiatti et al. 1996; Richmond et al. 1996).”
• SHOCK BREAKOUT IN DENSE MASS LOSS: LUMINOUS SUPERNOVAE (2011, unknown): “The breakout detection of SN 2008D with Swift (Soderberg et al. 2008) was fortunate.”
• The Zwicky Transient Facility: Science Objectives (2019, background): “…early photometry from the ground and from space, available only for a handful of serendipitously observed events so far (e.g., Campana et al. 2006; Soderberg et al. 2008; Gezari et al. 2008; Garnavich et al. 2016; Bersten et al. 2018) probes the early physics of explosion shock breakout and…”
• Bolometric light curves and explosion parameters of 38 stripped-envelope core-collapse supernovae (2014, methodology): “Tanaka et al. (2009) determine a vph for SN 2008D via spectral modelling of 9000 km s−1 and determine the velocity of Si II as 9300 km s−1 (Soderberg et al. 2008, also find a similar Si II velocity).”
• THE ULTRAVIOLET-BRIGHT, SLOWLY DECLINING TRANSIENT PS1-11af AS A PARTIAL TIDAL DISRUPTION EVENT (2013, background): “This is true for objects ranging from normal SNe II (e.g., Leonard et al. 2002) and Ib/c (Soderberg et al. 2008; Modjaz et al. 2009) to the SN IIn 2007pk (Pritchard et al. 2012) and even SLSNe (Miller et al. 2009; Gezari et al. 2009a; Quimby et al. 2011; Chomiuk et al. 2011; Lunnan et al. 2013;…”
• FROM SHOCK BREAKOUT TO PEAK AND BEYOND: EXTENSIVE PANCHROMATIC OBSERVATIONS OF THE TYPE Ib SUPERNOVA 2008D ASSOCIATED WITH SWIFT X-RAY TRANSIENT 080109 (2008, methodology): “There is evidence that the XRT 080109 late-time X-ray spectrum (from the Chandra data) was also softer with Γ = 3.6+1.7−1.4 (Pooley & Soderberg 2008; Soderberg et al. 2008b) than the early-time spectrum.”
• OBSERVING THE NEXT GALACTIC SUPERNOVA (2013, methodology): “The breakout pulse from ccSNe has only been observed a few times (GRB 060218/SN 2006aj, XRT 080109/SN 2008D, and SNLS-04D2dc; Campana et al. 2006; Soderberg et al. 2008; Schawinski et al. 2008) because its characteristic duration roughly corresponds to the light crossing time of the star, R∗/c.”
• The THESEUS space mission concept: science case, design and expected performances (2017, background): “This has been spectacularly captured just once, in a serendipitous Swift XRT observation of SN2008D (Soderberg et al., 2008): SNe are usually found only days to weeks after the explosion, as radioactive heating powers optical brightening.”