Christopher Martin
Affiliations: | 1993- | Physics | California Institute of Technology, Pasadena, CA |
Area:
Astronomy; PhysicsWebsite:
https://www.pma.caltech.edu/content/christopher-martinGoogle:
"Christopher Martin"Bio:
http://rscience.gsfc.nasa.gov/phd_alpha.html
http://adsabs.harvard.edu/abs/1986PhDT........11M
http://www.osti.gov/scitech/biblio/6640967
Mean distance: 15.64 | S | N | B | C | P |
Cross-listing: Astronomy Tree
Parents
Sign in to add mentorC. Stuart Bowyer | grad student | 1986 | UC Berkeley | |
(The Physical Origins of the Cosmic Ultraviolet Background) |
Children
Sign in to add traineeDavid Schiminovich | grad student | 1998 | Columbia (Astronomy Tree) |
Thiago S. Goncalves | grad student | 2012 | Caltech |
Erika T. Hamden | post-doc | 2014 | Caltech |
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Publications
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O’Sullivan DB, Martin C, Matuszewski M, et al. (2020) The FLASHES Survey. I. Integral Field Spectroscopy of the CGM around 48 z ≃ 2.3–3.1 QSOs The Astrophysical Journal. 894: 3 |
Darvish B, Scoville NZ, Martin C, et al. (2020) Spectroscopic confirmation of a Coma Cluster progenitor at z~2.2 The Astrophysical Journal. 892: 8 |
Wasserman A, van Dokkum P, Romanowsky AJ, et al. (2019) Spatially Resolved Stellar Kinematics of the Ultra-diffuse Galaxy Dragonfly 44. II. Constraints on Fuzzy Dark Matter The Astrophysical Journal. 885: 155 |
van Dokkum P, Wasserman A, Danieli S, et al. (2019) Spatially Resolved Stellar Kinematics of the Ultra-diffuse Galaxy Dragonfly 44. I. Observations, Kinematics, and Cold Dark Matter Halo Fits The Astrophysical Journal. 880: 91 |
Li Q, Cai Z, Prochaska JX, et al. (2019) Discovery of a Lyα-emitting Dark Cloud within the z ∼ 2.8 SMM J02399-0136 System The Astrophysical Journal. 875: 130 |
Relatores NC, Newman AB, Simon JD, et al. (2019) The Dark Matter Distributions in Low-mass Disk Galaxies. I. Hα Observations Using the Palomar Cosmic Web Imager The Astrophysical Journal. 873: 5 |
Cai Z, Hamden E, Matuszewski M, et al. (2018) Keck/Palomar Cosmic Web Imagers Reveal an Enormous Ly α Nebula in an Extremely Overdense Quasi-stellar Object Pair Field at z = 2.45 The Astrophysical Journal. 861: L3 |
Darvish B, Scoville NZ, Martin C, et al. (2018) Similar Scaling Relations for the Gas Content of Galaxies Across Environments to z ∼ 3.5 The Astrophysical Journal. 860: 111 |
Darvish B, Martin C, Gonçalves TS, et al. (2018) Quenching or Bursting: The Role of Stellar Mass, Environment, and Specific Star Formation Rate to z ~ 1 The Astrophysical Journal. 853: 155 |
Jewell AD, Hamden ET, Ong HR, et al. (2015) Detector performance for the FIREBall-2 UV experiment Proceedings of Spie - the International Society For Optical Engineering. 9601 |