DARTS/Astro Query System - SQL Search -

All the tables available for SQL Search and information on each table are listed in the Available Data page. Please see the User Guide for the usage of "SQL Search".

total 1

No.
object_name
center_ra
center_dec
center_ra_b1950
center_dec_b1950
center_ecliptic_lon
center_ecliptic_lat
center_galactic_lon
center_galactic_lat
roll_angle
observation_start_time_mjd
observation_start_time
observation_end_time_mjd
observation_end_time
observation_id
exposure
awarded_exposure
xis0_exposure
xis1_exposure
xis2_exposure
xis3_exposure
xis0_observation_mode
xis1_observation_mode
xis2_observation_mode
xis3_observation_mode
hxd_observation_mode
hxd_coarse_clock_rate_exposure
hxd_first_clock_rate_exposure
hxd_normal_clock_rate_exposure
hxd_all_clock_rate_exposure
hxd_wam_exposure
quantity_of_hxd_burst
processing_status
processing_date_mjd
processing_date
public_date_mjd
public_date
distribution_date_mjd
distribution_date
processing_version
processing_count
processing_software
proposal_id
proposal_abstract
proposal_category
proposal_category_code
proposal_priority
pi_name
co_pi_name
proposal_affiliated_country
proposal_cycle
observation_type
proposal_title
main_instrument
has_xis_injection
data_access_url
ql_access_url
ql_image_url
1 N103B 77.15 -68.7359 77.208253 -68.79772 330.089921 -84.667648 279.60217418 -34.399508 199.4598 55194.4728356482 2009-12-29 11:20:53 55200.6044560185 2010-01-04 14:30:25 804039010 223.8999 150 224.0108 223.8999 0 224.0028 2 2 0 2 1 0 0 46.096 46.096 129.9558 0 PROCESSED 57550.0511805556 2016-06-11 01:13:42 55584 2011-01-23 00:00:00 55218.4707060185 2010-01-22 11:17:49 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 040080 We aim to detect very low abundance lines, Cr and Mn, from SNR N103B in the Large Magellanic Cloud which is a low metaricity galaxy. It is known that a mass ratio of Mn to Cr synthesized in Type Ia supernovae is strongly correrated with the metaricity of the progenitor white dwarf. In the early Suzaku observation, we already detected the Cr line with about 3-sigma confidence level. In this follow-up observation, we detect the Cr and Mn lines with significant confidence, and determine the metaricity of the progenitor of SNR N103B. This will be the first measurement of the white dwarf's metaricity in the extra-galactic object. EXTRAGALACTIC DIFFUSE SOURCES 8 B TORU TAMAGAWA JAP 4 AO4 A MANGANESE LINE DETECTION FROM SNR N103B IN A LOW METARICITY GALAXY XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/804039010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '804039010'

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