東華大學圖書館 |

Language: English

Help

回圖書館首頁

手機版館藏查詢

Back

Switch To: Labeled | MARC Mode | ISBD

Linked to FindBook

Google Book

Amazon

博客來

Properties of the color-magnitude diagrams of Type Ia Supernovae

Record Type:	Electronic resources : Monograph/item
Title/Author:	Properties of the color-magnitude diagrams of Type Ia Supernovae/ by Lauren Aldoroty.
Author:	Aldoroty, Lauren.
Published:	Cham :Springer Nature Switzerland : : 2024.,
Description:	xviii, 86 p. :ill. (some col.), digital ;24 cm.
Notes:	"Doctoral thesis accepted by Texas A&M University, USA."
[NT 15003449]:	1 Introduction -- 2 Data -- 3 Methods -- 4 Results and Discussion -- 5 Conclusions.
Contained By:	Springer Nature eBook
Subject:	Supernovae - Spectra. -
Online resource:	https://doi.org/10.1007/978-3-031-72447-3
ISBN:	9783031724473

Properties of the color-magnitude diagrams of Type Ia Supernovae
Aldoroty, Lauren.

Properties of the color-magnitude diagrams of Type Ia Supernovae[electronic resource] /by Lauren Aldoroty. - Cham :Springer Nature Switzerland :2024. - xviii, 86 p. :ill. (some col.), digital ;24 cm. - Springer theses,2190-5061. - Springer theses..

"Doctoral thesis accepted by Texas A&M University, USA."

1 Introduction -- 2 Data -- 3 Methods -- 4 Results and Discussion -- 5 Conclusions.

This thesis presents a novel analysis of a photometric observational feature of Type Ia Supernovae (SNe Ia), the most precise distance indicators available for cosmological studies. While SNe Ia are crucial for understanding modern cosmology, there are systematic uncertainties associated with them that prevent use to their full potential. It is therefore vital that sources of systematic error in SN Ia standardization are better understood. In this thesis, the author robustly connects the color-magnitude diagram to SN Ia spectra and their physics for the first time, and shows that for the SN sample in the dissertation, this feature is important to consider as a contributor to scatter in the Hubble residual. There is no prior work in the literature that examines this feature in such depth, and it is rare to be able to paint such a thorough picture in a SN Ia study rooted in a single photometric feature. This work opens up many avenues for future observational and theoretical studies.

ISBN: 9783031724473

Standard No.: 10.1007/978-3-031-72447-3doiSubjects--Topical Terms:

3735249
Supernovae
--Spectra.

LC Class. No.: QB843.S95

Dewey Class. No.: 523.84465

Properties of the color-magnitude diagrams of Type Ia Supernovae
LDR:02195nmm a2200349 a 4500 001 2381250
003 DE-He213
005 20241126115340.0
006 m d
007 cr nn 008maaau
008 250418s2024 sz s 0 eng d
020 $a 9783031724473 $q (electronic bk.)
020 $a 9783031724466 $q (paper)
024 7 $a 10.1007/978-3-031-72447-3 $2 doi
035 $a 978-3-031-72447-3
040 $a GP $c GP
041 0 $a eng
050 4 $a QB843.S95
072 7 $a PHVB $2 bicssc
072 7 $a SCI005000 $2 bisacsh
072 7 $a PHVB $2 thema
082 0 4 $a 523.84465 $2 23
090 $a QB843.S95 $b A364 2024
100 1 $a Aldoroty, Lauren. $3 3735248
245 1 0 $a Properties of the color-magnitude diagrams of Type Ia Supernovae $h [electronic resource] / $c by Lauren Aldoroty.
260 $a Cham : $b Springer Nature Switzerland : $b Imprint: Springer, $c 2024.
300 $a xviii, 86 p. : $b ill. (some col.), digital ; $c 24 cm.
490 1 $a Springer theses, $x 2190-5061
500 $a "Doctoral thesis accepted by Texas A&M University, USA."
505 0 $a 1 Introduction -- 2 Data -- 3 Methods -- 4 Results and Discussion -- 5 Conclusions.
520 $a This thesis presents a novel analysis of a photometric observational feature of Type Ia Supernovae (SNe Ia), the most precise distance indicators available for cosmological studies. While SNe Ia are crucial for understanding modern cosmology, there are systematic uncertainties associated with them that prevent use to their full potential. It is therefore vital that sources of systematic error in SN Ia standardization are better understood. In this thesis, the author robustly connects the color-magnitude diagram to SN Ia spectra and their physics for the first time, and shows that for the SN sample in the dissertation, this feature is important to consider as a contributor to scatter in the Hubble residual. There is no prior work in the literature that examines this feature in such depth, and it is rare to be able to paint such a thorough picture in a SN Ia study rooted in a single photometric feature. This work opens up many avenues for future observational and theoretical studies.
650 0 $a Supernovae $x Spectra. $3 3735249
650 0 $a Astronomical photometry. $3 1530588
650 1 4 $a Astrophysics. $3 535904
650 2 4 $a Astronomy, Observations and Techniques. $3 1066822
650 2 4 $a Classical and Quantum Gravity. $3 3538892
650 2 4 $a Optical Spectroscopy. $3 3596595
710 2 $a SpringerLink (Online service) $3 836513
773 0 $t Springer Nature eBook
830 0 $a Springer theses. $3 1314442
856 4 0 $u https://doi.org/10.1007/978-3-031-72447-3
950 $a Physics and Astronomy (SpringerNature-11651)