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 | IKT25 | 16.5704 | -72.153 | 16.175469 | -72.420209 | 314.528049 | -65.245772 | 301.32642461 | -44.92895011 | 33.6181 | 54601.2130208333 | 2008-05-15 05:06:45 | 54603.3675810185 | 2008-05-17 08:49:19 | 803002010 | 107.3223 | 100 | 107.3303 | 107.3303 | 0 | 107.3223 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 124.1064 | 124.1064 | 186.1339 | 1 | PROCESSED | 57542.58375 | 2016-06-03 14:00:36 | 54981 | 2009-05-30 00:00:00 | 54613.1905439815 | 2008-05-27 04:34:23 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 030016 | In order for the white dwarf, the progenitor of SN Ia, to increase its mass to the Chandrasekhar limit, stellar wind driven by Fe contained in the accreting matter needs to be strong enough. For this reason, SN Ia is difficult to take place in the galaxy with low metallicity. We propose the observation on IKT 25, a type Ia SNR candidate in SMC, in order to decide its origin. Since the Fe abundance of SMC (0.2 solar) is lower than that of any other galaxys where SN Ia (or its remnant) had already been discovered, this observation will give the strongest restriction to the theory of the white dwarf evolution. | EXTRAGALACTIC DIFFUSE SOURCES | 8 | A | HIROYA YAMAGUCHI | JAP | 3 | AO3 | IKT25: TYPE IA SNR CANDIDATE IN SMALL MAGELLANIC CLOUD | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/803002010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '803002010'
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