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
|
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1 | W49B | 287.7847 | 9.1157 | 287.186344 | 9.032042 | 290.655059 | 31.28998 | 43.28157058 | -0.18360003 | 89.2671 | 54919.1063888889 | 2009-03-29 02:33:12 | 54920.4689583333 | 2009-03-30 11:15:18 | 503084010 | 52.1549 | 40 | 52.1549 | 52.1549 | 0 | 52.1549 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 43.9512 | 43.9512 | 117.7099 | 2 | PROCESSED | 57547.7422685185 | 2016-06-08 17:48:52 | 55330 | 2010-05-14 00:00:00 | 54931.3622106482 | 2009-04-10 08:41:35 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 030142 | Observations of the W49B supernova remnant for 40 ks is proposed to reveal whether it is a remnant of an anomalous Type Ia supernova or not. To determine the type of the supernova, detailed measurement of less abundand elements such as Cr and Mn will be performed, and abundance of Ni and Ti will be examined. The abundance pattern of those elements in W49B will be compared to that of Tycho's SNR we measured by Suzaku. | GALACTIC DIFFUSE EMISSION | 5 | C | TORU TAMAGAWA | JAP | 3 | AO3 | IS W49B A REMNANT OF AN ANOMALOUS TYPE IA SUPERNOVA? | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/503084010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '503084010'
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