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 IRAS 19254-7245 292.8508 -72.6492 291.381636 -72.754038 280.373528 -50.031737 322.5078751 -28.76929596 279.8892 54041.9830208333 2006-11-02 23:35:33 54044.5967476852 2006-11-05 14:19:19 701052010 113.5123 120 113.5203 113.5203 113.5123 113.5203 2 2 2 2 1 0 0 151.9778 151.9778 225.8099 1 PROCESSED 57536.068125 2016-05-28 01:38:06 54455 2007-12-21 00:00:00 54088.8285185185 2006-12-19 19:53:04 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 011342 We propose a 120 ksec Suzaku exposure of the ULIRG IRAS19254-7245. A previous XMM-Newton observation revealed the presence of a strong iron emission line and a flat continuum, both suggesting that this source hosts a Compton-thick AGN. In this scenario, the 2-10 keV luminosity of IRAS19254-7245 could be greater than 10e44 erg/s. However since no direct continuum is visible in the XMM bandpass, a direct measure of the absorbing column density was not feasible, thus the intrinsic X-ray luminosity of this source was derived only through indirect arguments. The unique bandpass and sensititvity of Suzaku above 10 keV will allow us to confirm the Compton-thick nature of this source and to measure for the first time the intrinsic X-ray luminosity of the AGN hosted in IRAS 19254-7245. EXTRAGALACTIC COMPACT SOURCES 7 C VALENTINA BRAITO USA 1 AO1 ASSESSING THE ENERGETIC BUDGET IN THE SUPERANTENNAE XIS N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/701052010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '701052010'

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