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In 2014 we adjusted the subscription prices of 26 journal titles downwards to reflect falls in subscription article volume .

Price adjustments for 2014

Title 2013 Price ($)
Adjusted Price
Increase 2014 2014 Price ($)
PROGRESS IN PLANNING 1,201 0.00% 1,201
JOURNAL OF MOLECULAR BIOLOGY 9,273 -8.19% 8,513
Mechanisms of Development 3,472 -10.00% 3,125
CORTEX 2,082 -2.92% 2,021
Molecular and Biochemical Parasitology 5,561 -3.71% 5,355
DNA Repair 2,288 -6.22% 2,146
Biophysical Chemistry 5,375 -7.89% 4,951
Mutation Research/Fundamental and Molecular Mechanisms of Mutagenesis 7,403 -4.63% 7,060
BIOSYSTEMS 2,484 -5.32% 2,352
Theoretical Population Biology 1,516 -4.63% 1,446
Gene Expression Patterns 2,538 -5.50% 2,398
TRENDS IN BIOTECHNOLOGY (Pers Ed) 2,347 0.00% 2,347
MOLECULAR IMMUNOLOGY 4,568 -8.10% 4,198
MATHEMATICAL BIOSCIENCES 3,861 -4.50% 3,687
Toxicology 7,473 -4.98% 7,101
VISION RESEARCH 5,152 -2.75% 5,010
JOURNAL OF CATALYSIS 6,381 -2.19% 6,241
Behaviour Research and Therapy 2,498 -5.60% 2,358
Clinical Immunology 3,366 -4.29% 3,222
Marine Chemistry 3,248 -6.48% 3,038
Virology 7,546 -5.12% 7,160
INT JNL OF MACHINE TOOLS & MANUFACTURE 4,430 -6.49% 4,143
INT. JNL. OF SOLIDS AND STRUCTURES 9,837 -3.11% 9,531
JNL OF MATERIALS PROCESSING TECHNOLOGY 7,688 -10.00% 6,919
Cancer Letters 7,987 -2.93% 7,753
Ecological Modelling 5,919 -2.61% 5,764
• Prices of subscription journals can rise or
fall.
• Elsevier subscription prices depend
(among other factors) on the number of
subscription articles only.
• If the number of subscription articles goes
down in a structured way, we will reduce
the subscription price of the journal.
• In 2014 we adjusted the subscription
prices of 26 journal titles downwards to
reflect falls in subscription article volume .
• In some cases, hybrid titles with declining
subscription revenue and an increasing
number of open access articles will
transition towards a full open access
model as a result of this process.

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Context. WASP-76 b has been a recurrent subject of study since the detection of a signature in high-resolution transit spectroscopy data indicating an asymmetry between the two limbs of the planet. The existence of this asymmetric signature has been confirmed by multiple studies, but its physical origin is still under debate. In addition, it contrasts with the absence of asymmetry reported in the infrared (IR) phase curve. Aims. We provide a more comprehensive dataset of WASP-76 b with the goal of drawing a complete view of the physical processes at work in this atmosphere. In particular, we attempt to reconcile visible high-resolution transit spectroscopy data and IR broadband phase curves. Methods. We gathered 3 phase curves, 20 occultations, and 6 transits for WASP-76 b in the visible with the CHEOPS space telescope. We also report the analysis of three unpublished sectors observed by the TESS space telescope (also in the visible), which represents 34 phase curves. Results. WASP-76 b displays an occultation of 260±11 and 152±10 ppm in TESS and CHEOPS bandpasses respectively. Depending on the composition assumed for the atmosphere and the data reduction used for the IR data, we derived geometric albedo estimates that range from 0.05 ± 0.023 to 0.146 ± 0.013 and from <0.13 to 0.189 ± 0.017 in the CHEOPS and TESS bandpasses, respectively. As expected from the IR phase curves, a low-order model of the phase curves does not yield any detectable asymmetry in the visible either. However, an empirical model allowing for sharper phase curve variations offers a hint of a flux excess before the occultation, with an amplitude of ∼40 ppm, an orbital offset of ∼−30◦ , and a width of ∼20◦ . We also constrained the orbital eccentricity of WASP-76 b to a value lower than 0.0067, with a 99.7% confidence level. This result contradicts earlier proposed scenarios aimed at explaining the asymmetry observed in high-resolution transit spectroscopy. Conclusions. In light of these findings, we hypothesise that WASP-76 b could have night-side clouds that extend predominantly towards its eastern limb. At this limb, the clouds would be associated with spherical droplets or spherically shaped aerosols of an unknown species, which would be responsible for a glory effect in the visible phase curves.

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We explore different scenarios to explain the chemical difference found in the remarkable giant-giant binary system HD138202+CD−3012303. For the first time, we suggest how to distinguish these scenarios by taking advantage of the extensive convective envelopes of giant stars. Methods. We carried out a high-precision determination of stellar parameters and abundances by applying a full line-by-line differential analysis on GHOST high-resolution spectra. We used the FUNDPAR program with ATLAS12 model atmospheres and specific opacities calculated for an arbitrary composition through a doubly iterated method. Physical parameters were estimated with the isochrones package and evolutionary tracks were calculated via MIST models. Results. We found a significant chemical difference between the two stars (∆[Fe/H]∼0.08dex), which is largely unexpected considering the insensitivity of giant stars to planetary ingestion and diffusion effects. We tested the possibility of engulfment events by using several different combinations of stellar mass, ingested mass, metallicity of the engulfed object and different convective envelopes. However, the planetary ingestion scenario does not seem to explain the observed differences. For the first time, we distinguished the source of chemical differences using a giant-giant binary system. By ruling out other possible scenarios such as planet formation and evolutionary effects between the two stars, we suggest that primordial inhomogeneities might explain the observed differences. This remarkable result implies that the metallicity differences that were observed in at least some main-sequence binary systems might be related to primordial inhomogeneities rather than engulfment events. We also discuss the important implications of finding primordial inhomogeneities, which affect chemical tagging and other fields such as planet formation. We strongly encourage the use of giantgiant pairs. They are a relevant complement to main-sequence pairs for determining the origin of the observed chemical differences in multiple systems.

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Disentangling the origin of chemical differences using GHOST

Disentangling the origin of chemical differences using GHOST

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Biological Classification BioHack (3).pdf

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Recombinant DNA technology (Immunological screening)

Recombinant DNA technology (Immunological screening)

Recombinant DNA technology (Immunological screening)

Disentangling the origin of chemical differences using GHOST

Disentangling the origin of chemical differences using GHOST

Disentangling the origin of chemical differences using GHOST

Botany 4th semester file By Sumit Kumar yadav.pdf

Botany 4th semester file By Sumit Kumar yadav.pdf

Botany 4th semester file By Sumit Kumar yadav.pdf

Price adjustment slide

1. Price adjustments for 2014 Title 2013 Price ($) Adjusted Price Increase 2014 2014 Price ($) PROGRESS IN PLANNING 1,201 0.00% 1,201 JOURNAL OF MOLECULAR BIOLOGY 9,273 -8.19% 8,513 Mechanisms of Development 3,472 -10.00% 3,125 CORTEX 2,082 -2.92% 2,021 Molecular and Biochemical Parasitology 5,561 -3.71% 5,355 DNA Repair 2,288 -6.22% 2,146 Biophysical Chemistry 5,375 -7.89% 4,951 Mutation Research/Fundamental and Molecular Mechanisms of Mutagenesis 7,403 -4.63% 7,060 BIOSYSTEMS 2,484 -5.32% 2,352 Theoretical Population Biology 1,516 -4.63% 1,446 Gene Expression Patterns 2,538 -5.50% 2,398 TRENDS IN BIOTECHNOLOGY (Pers Ed) 2,347 0.00% 2,347 MOLECULAR IMMUNOLOGY 4,568 -8.10% 4,198 MATHEMATICAL BIOSCIENCES 3,861 -4.50% 3,687 Toxicology 7,473 -4.98% 7,101 VISION RESEARCH 5,152 -2.75% 5,010 JOURNAL OF CATALYSIS 6,381 -2.19% 6,241 Behaviour Research and Therapy 2,498 -5.60% 2,358 Clinical Immunology 3,366 -4.29% 3,222 Marine Chemistry 3,248 -6.48% 3,038 Virology 7,546 -5.12% 7,160 INT JNL OF MACHINE TOOLS & MANUFACTURE 4,430 -6.49% 4,143 INT. JNL. OF SOLIDS AND STRUCTURES 9,837 -3.11% 9,531 JNL OF MATERIALS PROCESSING TECHNOLOGY 7,688 -10.00% 6,919 Cancer Letters 7,987 -2.93% 7,753 Ecological Modelling 5,919 -2.61% 5,764 • Prices of subscription journals can rise or fall. • Elsevier subscription prices depend (among other factors) on the number of subscription articles only. • If the number of subscription articles goes down in a structured way, we will reduce the subscription price of the journal. • In 2014 we adjusted the subscription prices of 26 journal titles downwards to reflect falls in subscription article volume . • In some cases, hybrid titles with declining subscription revenue and an increasing number of open access articles will transition towards a full open access model as a result of this process.