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 | G352.7-0.1 | 261.9227 | -35.1119 | 261.088463 | -35.070764 | 263.245639 | -11.859611 | 352.75195989 | -0.12120729 | 94.0335 | 55988.8605671296 | 2012-03-02 20:39:13 | 55993.5536111111 | 2012-03-07 13:17:12 | 506052010 | 201.5474 | 200 | 201.5474 | 201.5474 | 0 | 201.5474 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 171.544 | 171.544 | 405.4396 | 4 | PROCESSED | 57604.9422569445 | 2016-08-04 22:36:51 | 56375 | 2013-03-24 00:00:00 | 56008.397337963 | 2012-03-22 09:32:10 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 061315 | Supernova remnants showing strong Fe K emission are relatively rare, and primarily of Type Ia. We propose a long observation of one of the least well-studied Fe-rich Galactic SNRs, G352.7-0.1, with the goal of characterizing the Fe emission, confirming its likely identification as the remnant of a Type Ia supernova, and constraining the properties of ejected material and the dynamics of the explosion. Its thermal X-ray spectrum is strikingly similar to Tycho's SNR, but unexpectedly X-rays are uniformly distributed throughout the remnant. Our proposed observation will produce high-quality spectra, adequate for detailed studies with some spatial information, that will greatly aid in understanding of this very interesting young remnant. | GALACTIC DIFFUSE EMISSION | 5 | C | KAZIMIERZ BORKOWSKI | USA | 6 | AO6 | STRONG IRON EMISSION IN THE SUPERNOVA REMNANT G352.7-0.1 | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/506052010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '506052010'
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