Asosiy kontentga oʻtish
AkademScholar
Mualliflar

H. T. Diehl

Soʻnggi maʼlum muassasa:
Fermi National Accelerator Laboratory
ORCID:
0000-0002-8357-7467
8
h-indeks
6
i10-indeksi
328
Iqtiboslar
91
Asarlar
Vaqt boʻyicha

Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
05101520025507510020172018201920202021202220232024202520262017: Nashrlar 1, Iqtiboslar 12018: Nashrlar 6, Iqtiboslar 12019: Nashrlar 4, Iqtiboslar 22020: Nashrlar 4, Iqtiboslar 02021: Nashrlar 12, Iqtiboslar 32022: Nashrlar 9, Iqtiboslar 42023: Nashrlar 3, Iqtiboslar 102024: Nashrlar 7, Iqtiboslar 662025: Nashrlar 1, Iqtiboslar 772026: Nashrlar 2, Iqtiboslar 81

Iqtibos tarixi

025507510020172018201920202021202220232024202520262017: Iqtiboslar 12018: Iqtiboslar 12019: Iqtiboslar 22020: Iqtiboslar 02021: Iqtiboslar 32022: Iqtiboslar 42023: Iqtiboslar 102024: Iqtiboslar 662025: Iqtiboslar 772026: Iqtiboslar 81

Nashr tarixi

0510152020172018201920202021202220232024202520262017: Nashrlar 12018: Nashrlar 62019: Nashrlar 42020: Nashrlar 42021: Nashrlar 122022: Nashrlar 92023: Nashrlar 32024: Nashrlar 72025: Nashrlar 12026: Nashrlar 2

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

03581020172018201920202021202220232024202520262017: h-indeks 42018: h-indeks 42019: h-indeks 42020: h-indeks 42021: h-indeks 42022: h-indeks 42023: h-indeks 42024: h-indeks 52025: h-indeks 72026: h-indeks 8

Eng koʻp iqtibos qilingan asarlar

  1. SPT clusters with DES and HST weak lensing. II. Cosmological constraints from the abundance of massive halos20243 iqtibos
  2. Dark Energy Survey: Galaxy sample for the baryonic acoustic oscillation measurement from the final dataset20243 iqtibos
  3. Quasi-Model-Independent Search for New High<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi>T</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math>Physics at D020012 iqtibos
  4. Search for Second-Generation Leptoquark Pairs in<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mrow><mml:mover><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi>¯</mml:mi></mml:mrow></mml:mover></mml:mrow></mml:mrow><mml:mi mathvariant="italic">p</mml:mi></mml:math>Collisions at<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>√</mml:mi><mml:mi mathvariant="italic">s</mml:mi><mml:mspace/><mml:mo>=</mml:mo><mml:mspace/><mml:mn>1.8</mml:mn><mml:mn/><mml:mi/><mml:mi>TeV</mml:mi></mml:math>20002 iqtibos
  5. Differential Production Cross Section of<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi mathvariant="italic">Z</mml:mi></mml:math>Bosons as a Function of Transverse Momentum at<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msqrt><mml:mrow><mml:mi mathvariant="italic">s</mml:mi></mml:mrow></mml:msqrt><mml:mspace/><mml:mo>=</mml:mo><mml:mspace/><mml:mn>1.8</mml:mn><mml:mn/><mml:mi/><mml:mi>TeV</mml:mi></mml:math>TeV20002 iqtibos
  6. Direct measurement of the top quark mass by the DØ Collaboration19982 iqtibos
  7. SPT clusters with DES and HST weak lensing. I. Cluster lensing and Bayesian population modeling of multiwavelength cluster datasets20241 iqtibos
  8. Determination of the mass of theWboson using the D∅ detector at the Fermilab Tevatron19981 iqtibos
  9. Search for<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>Charge</mml:mi><mml:mi>−</mml:mi><mml:mn>1</mml:mn><mml:mo>/</mml:mo><mml:mn>3</mml:mn></mml:math>Third-Generation Leptoquarks in<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi mathvariant="italic">p</mml:mi><mml:mrow><mml:mrow><mml:mover><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi>¯</mml:mi></mml:mrow></mml:mover></mml:mrow></mml:mrow><mml:mi mathvariant="italic"/></mml:math>Collisions at<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msqrt><mml:mrow><mml:mi>s</mml:mi></mml:mrow></mml:msqrt><mml:mspace/><mml:mo>=</mml:mo><mml:mspace/><mml:mn>1.8</mml:mn><mml:mn/><mml:mi/><mml:mi>TeV</mml:mi></mml:math>19981 iqtibos
  10. Limits on anomalous<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>WW</mml:mi><mml:mi>γ</mml:mi></mml:math>and<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>WWZ</mml:mi></mml:math>couplings19980 iqtibos

Hammualliflar

  1. M. Šako0 ta umumiy asarSkelet yozuvlar: 1
  2. E. Berger0 ta umumiy asarSkelet yozuvlar: 1
  3. D. Brown0 ta umumiy asarSkelet yozuvlar: 1
  4. Brian D. Metzger0 ta umumiy asarSkelet yozuvlar: 1
  5. P. S. Cowperthwaite0 ta umumiy asarSkelet yozuvlar: 1
  6. V. Ashley Villar0 ta umumiy asarSkelet yozuvlar: 1
  7. P. K. Blanchard0 ta umumiy asarSkelet yozuvlar: 1
  8. K. D. Alexander0 ta umumiy asarSkelet yozuvlar: 1
  9. Z. Doctor0 ta umumiy asarSkelet yozuvlar: 1
  10. Tarraneh Eftekhari0 ta umumiy asarSkelet yozuvlar: 1

Yana 24 ta asar katta kollaboratsiyada (50 dan ortiq muallif) — hammualliflar roʻyxatiga kiritilmagan

Skelet yozuvlar: 66 — katta kollaboratsiyada (50 dan ortiq muallif), hammualliflar roʻyxatiga kiritilmagan

Barcha hammualliflar →