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 | TYCHO SNR | 6.3139 | 64.1469 | 5.613879 | 63.870082 | 42.846574 | 53.765969 | 120.08177164 | 1.42013769 | 53.7834 | 54682.0646759259 | 2008-08-04 01:33:08 | 54686.9529398148 | 2008-08-08 22:52:14 | 503085010 | 312.892 | 400 | 312.916 | 312.892 | 0 | 312.908 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 289.9494 | 289.9494 | 307.8699 | 3 | PROCESSED | 57543.3766782407 | 2016-06-04 09:02:25 | 54557 | 2008-04-01 00:00:00 | 54707.038287037 | 2008-08-29 00:55:08 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 031003 | Recent Suzaku studies of the Type Ia supernova remnant, Tycho, have revealed tantalizing evidence for secondary Fe-peak elements (specifically Cr and Mn) in the integrated X-ray spectrum. Here we propose to confirm and extend these detections by measuring the spatial variation of Cr/Fe line fluxes across the remnant, paying particular attention to the composition of a previously known Fe-rich region along the eastern limb. The unique capabilities of the XIS onboard Suzaku (high spectral resolution and large effective area) are crucial to the proposed study and no other operating instrument can detect the weak lines from these trace species within reasonable exposure times. | GALACTIC DIFFUSE EMISSION | 5 | A | JOHN HUGHES | USA | 3 | AO3 | SECONDARY FE-PEAK ELEMENTS AS A PROBE OF SN IA EXPLOSION PHYSICS | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/503085010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '503085010'
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