Record-breaking carbon emissions, and more — this week’s best science graphics

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Global carbon dioxide emissions from fossil fuels are projected to hit a new record of 37.5 billion tonnes in 2022 COP27 That's one of this week's key science graphics

, scientists announced at the United Nations Climate Change Conference of the Parties in Sharm El-Sheikh, Egypt. The fastest emissions growth comes from India, where rising coal and oil consumption are driving an estimated 6% increase compared with 2021.

’s graduate-student survey say that they would most like to work in academia — down from 56% in 2019, whenlast surveyed PhD students. Those who want to pursue careers outside academia point to reasons including lack of funding, stiff competition for jobs and lack of work–life balance. More than 3,200 self-selected respondents from around the world

 

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It was an easy prediction to make, but as soon as they put us in lockdown I said when we come out of it people would 'party' harder and things would get worse...

If US military forces were a nation, they would have the highest per-capita CO2 emissions in the world, above that of Qatar and Kuwait

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A First Look into the Nature of JWST/MIRI 7.7 micron Sources from SMACS 0723Until now, our knowledge of the extragalactic Universe at mid-IR wavelengths (| 5 microns) was limited to rare active galactic nuclei (AGN) and the brightest normal galaxies up to z~3. The advent of the JWST with its Mid-Infrared Instrument (MIRI) will revolutionise the ability of the mid-IR regime as a key wavelength domain to probe the high-z Universe. In this work we present a first study of JWST MIRI 7.7 micron sources selected with | 3 sigma significance from the lensing cluster field SMACS J0723.3-7327. We model their spectral energy distribution fitting with 13 JWST and HST broad bands, in order to obtain photometric redshifts and derived physical parameters for all these sources. We find that this 7.7 micron galaxy sample is mainly composed of normal galaxies up to z=4 and has a tail of about 2% of sources at higher redshifts to z~ 9-10. The vast majority of our galaxies have [3.6]-[7.7]|0 colours and very few of them need high dust extinction values (A_V=3 -6 mag) for their SED fitting. The resulting lensing-corrected stellar masses span the range 10^7-10^{11} Msun. Overall, our results clearly show that the first MIRI 7.7 micron observations of deep fields are already useful to probe the high-redshift Universe and suggest that the deeper 7.7 micron observations to be available very soon will open up, for the first time, the epoch of reionisation at mid-IR wavelengths.
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