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Dr. Spencer  Lubin  Md image

Dr. Spencer Lubin Md

447 Atlantic Ave
Brooklyn NY 11217
718 978-8430
Medical School: State University Of New York Downstate Medical Center - 1986
Accepts Medicare: Yes
Participates In eRX: No
Participates In PQRS: No
Participates In EHR: No
License #: 179844
NPI: 1285666420
Taxonomy Codes:
207L00000X

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Awards & Recognitions

About Us

Practice Philosophy

Conditions

Dr. Spencer Lubin is associated with these group practices

Procedure Pricing

HCPCS Code Description Average Price Average Price
Allowed By Medicare
HCPCS Code:00810 Description:Anesth low intestine scope Average Price:$886.92 Average Price Allowed
By Medicare:
$182.66

Medical Malpractice Cases

None Found

Medical Board Sanctions

None Found

Referrals

NPI
Doctor Name
Specialty
Count
1861452245
Gastroenterology
119
1588605588
Gastroenterology
69
1447217302
Internal Medicine
68
1710926134
Diagnostic Radiology
23
1700876281
Diagnostic Radiology
15
*These referrals represent the top 10 that Dr. Lubin has made to other doctors

Publications

Joint analysis of BICEP2/keck array and Planck Data. - Physical review letters
We report the results of a joint analysis of data from BICEP2/Keck Array and Planck. BICEP2 and Keck Array have observed the same approximately 400  deg^{2} patch of sky centered on RA 0 h, Dec. -57.5°. The combined maps reach a depth of 57 nK deg in Stokes Q and U in a band centered at 150 GHz. Planck has observed the full sky in polarization at seven frequencies from 30 to 353 GHz, but much less deeply in any given region (1.2  μK deg in Q and U at 143 GHz). We detect 150×353 cross-correlation in B modes at high significance. We fit the single- and cross-frequency power spectra at frequencies ≥150  GHz to a lensed-ΛCDM model that includes dust and a possible contribution from inflationary gravitational waves (as parametrized by the tensor-to-scalar ratio r), using a prior on the frequency spectral behavior of polarized dust emission from previous Planck analysis of other regions of the sky. We find strong evidence for dust and no statistically significant evidence for tensor modes. We probe various model variations and extensions, including adding a synchrotron component in combination with lower frequency data, and find that these make little difference to the r constraint. Finally, we present an alternative analysis which is similar to a map-based cleaning of the dust contribution, and show that this gives similar constraints. The final result is expressed as a likelihood curve for r, and yields an upper limit r_{0.05}<0.12 at 95% confidence. Marginalizing over dust and r, lensing B modes are detected at 7.0σ significance.

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447 Atlantic Ave Brooklyn, NY 11217
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