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 | NGC 1553 | 64.0253 | -55.7788 | 63.753175 | -55.901382 | 28.715493 | -73.694617 | 265.63371114 | -43.7014546 | 176.9406 | 54429.7042939815 | 2007-11-25 16:54:11 | 54431.9029976852 | 2007-11-27 21:40:19 | 802050010 | 98.7222 | 95 | 98.7222 | 98.7222 | 0 | 98.7222 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 87.7903 | 87.7903 | 189.9159 | 2 | PROCESSED | 57540.6454976852 | 2016-06-01 15:29:31 | 54806 | 2008-12-06 00:00:00 | 54438.4258101852 | 2007-12-04 10:13:10 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 021401 | As driving engines of metal enrichment, early-type galaxies provide vital laboratories to investigate how it operates. In our Chandra survey of galaxies, we found solar ISM abundances (Zfe), similar to the stars and implying enrichment homology from clusters to moderate-Lx galaxies. The only outlier was NGC1553, for which we found a tantalizing hint of very subsolar Zfe, inconsistent with simple models. Unlike other galaxies with recent reports of low Zfe, NGC1553 has a bright gas halo, so the results are insensitive to the modelling of unresolved LMXB. We propose an 80ks observation of NGC1553 to measure definitively the ISM abundances of Fe and other crucial diagnostic elements. These data will either confirm enrichment bimodality or provide a vital low-Lx data-point to anchor models. | EXTRAGALACTIC DIFFUSE SOURCES | 8 | C | PHILIP HUMPHREY | USA | 2 | AO2 | NGC 1553: PROOF OF BIMODAL METAL ENRICHMENT? | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/802050010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '802050010'
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