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 NGC 6888 302.9954 38.2382 302.538596 38.087534 320.045193 56.092572 75.36419968 2.38310331 253.873 55139.4126388889 2009-11-04 09:54:12 55141.3127777778 2009-11-06 07:30:24 504085010 77.349 75 77.461 77.349 0 77.461 3 2 0 2 1 0 0 62.1002 62.1002 164.1558 0 PROCESSED 57549.1334837963 2016-06-10 03:12:13 55518 2010-11-18 00:00:00 55152.1455671296 2009-11-17 03:29:37 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 041321 Fast winds from massive stars create large cavities in the surrounding interstellar medium filled with hot gas, known as Wind-Blown Bubbles (WBB). We propose to obtain XIS imaging spectroscopy of the prototype WBB NGC 6888. Thanks to the XIS excellent sensitivity and energy resolution in the soft X-ray band, we will: (i) obtain a high quality CCD spectrum which can be used to constrain the temperature of the hot plasma and the efficiency of thermal conduction across the bubble wall, (ii) determine the spatial distribution and properties of X-ray emitting plasma, (iii) therefore, test and refine shock physics models of bubbles by a direct confrontation of their results with observations. GALACTIC DIFFUSE EMISSION 5 A SVETOZAR ZHEKOV USA 4 AO4 X-RAYS FROM THE PROTOTYPE WIND-BLOWN BUBBLE NGC 6888 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/504085010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '504085010'

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