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304 results on '"Valentino F."'

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1. Streamlined, single-step non-viral CRISPR-Cas9 knockout strategy enhances gene editing efficiency in primary human chondrocyte populations

2. The Brownian loop soup stress-energy tensor

3. Exact correlation functions in the Brownian Loop Soup

4. Bulk reconstruction for spinor fields in AdS/CFT

5. TT¯ $$ T\overline{T} $$ type deformation in the presence of a boundary

6. Noema formIng Cluster survEy (NICE): Discovery of a starbursting galaxy group with a radio-luminous core at z = 3.95

7. Frontal Tendon Lengthening Plasty for Treatment of Structural Patella Baja

11. Actin modulates shape and mechanics of tubular membranes.

13. A dusty compact object bridging galaxies and quasars at cosmic dawn

15. The cold interstellar medium of a normal sub-L⋆ galaxy at the end of reionization.

16. Unveiling the hidden Universe with JWST: the contribution of dust-obscured galaxies to the stellar mass function at z ~ 3 – 8.

23. The large molecular gas fraction of post-starburst galaxies at z > 1.

25. ESICM LIVES 2016: part two: Milan, Italy. 1–5 October 2016

26. An extremely young massive clump forming by gravitational collapse in a primordial galaxy

30. CO excitation and line energy distributions in gas-selected galaxies.

33. Platform session

36. GOODS-ALMA 2.0: Starbursts in the main sequence reveal compact star formation regulating galaxy evolution prequenching.

41. GRB host galaxies with strong H2 absorption: CO-dark molecular gas at the peak of cosmic star formation.

42. Absorption-selected galaxies trace the low-mass, late-type, star-forming population at z ∼ 2–3.

44. A contribution of star-forming clumps and accreting satellites to the mass assembly of z ∼ 2 galaxies.

45. Sunyaev-Zel'dovich detection of the galaxy cluster Cl J1449+0856 at z = 1.99: The pressure profile in uv space.

46. Suppressed CO emission and high G/D ratios in z = 2 galaxies with sub-solar gas-phase metallicity.

47. Deciphering an evolutionary sequence of merger stages in infrared-luminous starburst galaxies at z ∼ 0.7.

50. PAHs as tracers of the molecular gas in star-forming galaxies.

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