Mellostalgia::looking forward to looking back

Nostalgia has predominantly been situated as a positive orientation to the past – a function of either personal or vicarious rose – tinted memory, triggered by circumstances in the present – a past/present dichotomy. Yet, nostalgia has no counterpart, a concept to explain a longing for the future, anchored in the present and determined by actions taken in the present. This paper details such an emotion by proposing the concept of “Mellostalgia.” Drawing on a study of visitors to the site of a British TV drama, the process of experiencing mellostalgia through a series of triggers and actions is examined. These include; stimulating mellostalgia; mellostalgia, the present and the future, and, capturing the mellostalgic experience, or “looking forward to looking back.

Dress, transformation and conformity in the heavy rock subculture

International audienc

The consumption of tattoos and tattooing : the body as permanent text

In this thesis, I investigate permanence through exploring tattoo consumption in terms of the social-historical context of being tattooed. The analysis is based on four years of data collection adopting a grounded theory approach. I present an analysis of how permanence occurs in terms of tattoo consumption, with particular interest in the physical permanence in relation to identity creation. This is set within the framework of Consumer Culture Theory (CCT). The reason for this is twofold, firstly to illustrate the ability of using tattooing as an instrument to investigate permanence within CCT. Secondly, to show the lack of use of the socio-historical perspective within such an investigation, and to show that the use of such data is a valid strategy and which adds depth and context to such an investigation. Furthermore, I suggest that tattoo consumption has become a site of embodied expression that is bounded by physicality, and permanence. I present a typology of tattooed consumers based on levels of commitment and explore in depth two main categories, physicality, and, permanence. I find that the physical permanence is shown through the commitment to tattoo usage. Its permanent nature determines the tattoo as an act of consumption that is dualistic in nature; both accepted, and yet equally rejected, which is seen within the consumers‘ negotiation of its use, in terms of mimicry and placement. Being tattooed represents a form of consumption that contravenes certain rules and norms of society, and yet at the same time is the basis for community membership and adherence to a set of sub-cultural norms and values.EThOS - Electronic Theses Online ServiceGBUnited Kingdo

Cyprus' image—a sun and sea destination—as a detrimental factor to seasonal fluctuations. Exploration into motivational factors for holidaying in Cyprus

Cyprus is established as a summer destination. To aid the destination in developing its winter season as well, this research uses a qualitative inductive approach to explore the tourists’ current image of the island and their motivations of visiting it. The research indicates that the current image, which essentially portrays Cyprus as a sun-and-sea destination is thought to dissuade tourists from perceiving the island as a year-round destination. Nonetheless, increasing the pull factors of the destination through the development of unique special interest products can help in extending the tourism season as well as broaden its narrow image

JWST UNCOVER: Discovery of z>9z>9 Galaxy Candidates Behind the Lensing Cluster Abell 2744

We present the results of a search for high-redshift ($z>9$) galaxy candidates in the JWST UNCOVER survey, using deep NIRCam and NIRISS imaging in 7 bands over $\sim45$ arcmin$^2$ and ancillary HST observations. The NIRCam observations reach a $5-\sigma$ limiting magnitude of $\sim 29.2$ AB. The identification of high$-z$ candidates relies on a combination of a dropout selection and photometric redshifts. We find 16 candidates at $9<z<12$ and 3 candidates at $12<z<13$, eight candidates are deemed very robust. Their lensing amplification ranges from $\mu=1.2$ to 11.5. Candidates have a wide range of (lensing-corrected) luminosities and young ages, with low stellar masses ($6.8<$ log(M$_{\star}$/M$_{\odot}$) $<9.5$) and low star formation rates (SFR=0.2-7 M$_{\odot}$ yr$^{-1}$), confirming previous findings in early JWST observations of $z>9$. A few galaxies at $z\sim9-10$ appear to show a clear Balmer break between the F356W and F444W/F410M bands, which helps constrain their stellar mass. We estimate blue UV continuum slopes between $\beta=-1.8$ and $-2.3$, typical for early galaxies at $z>9$ but not as extreme as the bluest recently discovered sources. We also find evidence for a rapid redshift-evolution of the mass-luminosity relation and a redshift-evolution of the UV continuum slope for a given range of intrinsic magnitude, in line with theoretical predictions. These findings suggest that deeper JWST observations are needed to reach the fainter galaxy population at those early epochs, and follow-up spectroscopy will help better constrain the physical properties and star formation histories of a larger sample of galaxies.Comment: Submitted to MNRA

Little Red Dots: an abundant population of faint AGN at z∼5z\sim5 revealed by the EIGER and FRESCO JWST surveys

Characterising the prevalence and properties of faint active galactic nuclei (AGN) in the early Universe is key for understanding the formation of supermassive black holes (SMBHs) and determining their role in cosmic reionization. We perform a spectroscopic search for broad H$\alpha$ emitters at $z\approx4-6$ using deep JWST/NIRCam imaging and wide field slitless spectroscopy from the EIGER and FRESCO surveys. We identify 20 H$\alpha$ lines at $z = 4.2 - 5.5$ that have broad components with line widths from $\sim1200 - 3700$ km s$^{-1}$, contributing $\sim 30 - 90$ % of the total line flux. We interpret these broad components as being powered by accretion onto SMBHs with implied masses $\sim10^{7-8}$ M$_{\odot}$. In the UV luminosity range M$_{\rm UV}$ = -21 to -18, we measure number densities of $\approx10^{-5}$ cMpc$^{-3}$. This is an order of magnitude higher than expected from extrapolating quasar UV luminosity functions. Yet, such AGN are found in only $<1$% of star-forming galaxies at $z\sim5$. The SMBH mass function agrees with large cosmological simulations. In two objects we detect narrow red- and blue-shifted H$\alpha$ absorption indicative, respectively, of dense gas fueling SMBH growth and outflows. We may be witnessing early AGN feedback that will clear dust-free pathways through which more massive blue quasars are seen. We uncover a strong correlation between reddening and the fraction of total galaxy luminosity arising from faint AGN. This implies that early SMBH growth is highly obscured and that faint AGN are only minor contributors to cosmic reionization.Comment: 23 pages, 17 figures. Submitted to ApJ. Main Figs 4, 10, 15 (faint AGN UV luminosity function) and 16 (SMBH mass function). Fig. 17 summarises the results. Comments welcom

UNCOVER: Illuminating the Early Universe -- JWST/NIRSpec Confirmation of z>12z > 12 Galaxies

Observations of high-redshift galaxies provide a critical direct test to the theories of early galaxy formation, yet to date, only four have been spectroscopically confirmed at $z>12$. Due to strong gravitational lensing over a wide area, the galaxy cluster field Abell~2744 is ideal for searching for the earliest galaxies. Here we present JWST/NIRSpec observations of two galaxies: a robust detection at $z_{\rm spec} = 12.393^{+0.004}_{-0.001}$, and a plausible candidate at $z_{\rm spec} = 13.079^{+0.013}_{-0.001}$. The galaxies are discovered in JWST/NIRCam imaging and their distances are inferred with JWST/NIRSpec spectroscopy, all from the JWST Cycle 1 UNCOVER Treasury survey. Detailed stellar population modeling using JWST NIRCam and NIRSpec data corroborates the primeval characteristics of these galaxies: low mass ($\sim 10^8~{\rm M_\odot}$), young, rapidly-assembling, metal-poor, and star-forming. Interestingly, both galaxies are spatially resolved, having lensing-corrected rest-UV effective radii on the order of 300-400 pc, which are notably larger than other spectroscopically confirmed $z \gtrsim 12$ systems. The observed dynamic range of $z \gtrsim 12$ size spans over an order of magnitude, implying a significant scatter in the size-mass relation at early times. Deep into the epoch of reionization, these discoveries elucidate the emergence of the first galaxies.Comment: submitted to ApJL; 13 pages, 4 figures, 2 table