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 FERMI_JET_COCOON_4 313.0188 -30.9125 312.254939 -31.101111 306.880758 -12.815318 13.57103518 -38.16097703 249.0341 56968.206412037 2014-11-07 04:57:14 56968.8473958333 2014-11-07 20:20:15 509050010 21.6767 20 21.6767 21.8127 0 21.8207 2 2 0 2 0 0 0 0 0 0 0 PROCESSED 57616.7496412037 2016-08-16 17:59:29 57358 2015-12-02 00:00:00 56982.4333333333 2014-11-21 10:24:00 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 091322 The Fermi bubbles are two large gamma-ray emitting objects near the Galactic center that may result from a time when Sgr A* was active, expelling mass and energy into the Galactic halo. Additional data from Fermi reinforce this hypothesis due to the detection of jet and cocoon structures in the southern bubble. There are signatures of the bubbles at X-ray energies, implying they contain relatively cool gas (10^6 K) and/or are influencing the Milky Way's hot gas halo. We propose Suzaku XIS observations to analyze the soft X-ray emission from these regions, which will allow us to constrain the density, temperature, and expansion velocity of these features. These observations will be crucial in understanding the evolution of the Fermi bubbles and their role in the evolution of the Milky Way. GALACTIC DIFFUSE EMISSION 5 C MATTHEW MILLER USA 9 AO9 OBSERVING THE ''JET'' AND ''COCOON'' FEATURES OF THE FERMI BUBBLES XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/509050010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '509050010'

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