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 | G296.1-0.5S | 177.6962 | -62.7172 | 177.080034 | -62.439005 | 216.307928 | -55.355417 | 296.04515802 | -0.65925146 | 111.5869 | 54482.7727662037 | 2008-01-17 18:32:47 | 54484.6668402778 | 2008-01-19 16:00:15 | 502069010 | 69.213 | 67 | 69.213 | 69.213 | 0 | 69.213 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 61.0096 | 61.0096 | 163.6237 | 2 | PROCESSED | 57541.3665740741 | 2016-06-02 08:47:52 | 54929 | 2009-04-08 00:00:00 | 54563.4417824074 | 2008-04-07 10:36:10 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 021218 | Supernova (SN) explosions within wind-blown bubbles are common among core-collapse (CC) SNe, and are expected to occur for some Type Ia SNe. We propose observations of an X-ray bright supernova remnant (SNR), G296.1-0.5, with very strong evidence for an explosion within a bubble. Spectroscopy with Suzaku will provide us with temperatures, abundances, and ionization ages of the X-ray emitting gas. If we detect SN ejecta, we will distinguish between a CC or a Type Ia progenitor. Gas temperatures will provide us with the shock speeds, while ionization ages will tell us when this gas was shocked. We will infer how progenitor winds affected the ambient medium prior to the explosion. The proposed observations will advance our knowledge of poorly understood SNR evolution in wind-blown bubbles. | GALACTIC DIFFUSE EMISSION | 5 | C | KAZIMIERZ BORKOWSKI | USA | 2 | AO2 | G296.1-0.5: A SUPERNOVA EXPLOSION WITHIN A BUBBLE | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/502069010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '502069010'
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